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w_20251207_112654900696
|
ENDF/B-VIII.1: Updated Nuclear Data Sheets for G.P.A. Nobre et al.
|
ENDF/B-VIII.1: Updated Nuclear Data Sheets for G.P.A. Nobre et al.
|
[] | 1
|
medium
|
universal
|
physics
|
arxiv
|
2511.03564v1
|
https://arxiv.org/abs/2511.03564v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
09cd61bd166ead93fb7cf3fe28aabddda1cfa2c32b9e6388ed3c350faca3d0df
|
Extracted from ArXiv paper 2511.03564v1 (chunk 83)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 83,
"paper_id": "2511.03564v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T11:26:54.900696Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251209_170640107420
|
The paper introduces a novel approach to discretize the coupling terms and equations of motion for plasma simulations using stacked vector and matrix notations.
|
The paper introduces a novel approach to discretize the coupling terms and equations of motion for plasma simulations using stacked vector and matrix notations.
|
[] | 1
|
medium
|
universal
|
physics
|
arxiv
|
2510.04385v2
|
https://arxiv.org/abs/2510.04385v2
|
[
"physics.comp-ph",
"math.NA",
"physics.plasm-ph"
] |
440d16559750c0fcd97832ba10f9aec5281dac890f18b5512c283ed740e912d0
|
Extracted from ArXiv paper 2510.04385v2 (chunk 17)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 17,
"paper_id": "2510.04385v2"
}
|
science
|
WO-ARX-01
|
2025-12-09T17:06:40.107420Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251209_192239300767
|
Computed values for accidentally nearly degenerate vibronic transitions pairs with transition wavenumber difference in PaF3+, including enhancement factors, electronic sensitivity factors, natural radiative linewidths, and expected frequency shifts.
|
Computed values for accidentally nearly degenerate vibronic transitions pairs with transition wavenumber difference in PaF3+, including enhancement factors, electronic sensitivity factors, natural radiative linewidths, and expected frequency shifts.
|
[] | 1
|
medium
|
universal
|
physics
|
arxiv
|
2511.10791v1
|
https://arxiv.org/abs/2511.10791v1
|
[
"physics.chem-ph",
"physics.atom-ph"
] |
7455e46a4558c75987eff696192cf68212f1a494d101acd34683e1fec53db5bc
|
Extracted from ArXiv paper 2511.10791v1 (chunk 17)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 17,
"paper_id": "2511.10791v1"
}
|
science
|
WO-ARX-01
|
2025-12-09T19:22:39.300767Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_120720063621
|
The data is reproduced within the quoted experimental uncertainties.
|
The data is reproduced within the quoted experimental uncertainties.
|
[
"1.23"
] | 0.95
|
medium
|
universal
|
physics
|
arxiv
|
2511.12717v1
|
https://arxiv.org/abs/2511.12717v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
43e7db2e6ad744f9217914d853850c573092366a70da5c7fde4a1c6276cb8328
|
Extracted from ArXiv paper 2511.12717v1 (chunk 16)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 16,
"paper_id": "2511.12717v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:07:20.063621Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_121950790748
|
Redshift values for several GRB events were measured using spectroscopic data from various telescopes, including ESO VLT UT3 (Melipal) and Gemini-North.
|
Redshift values for several GRB events were measured using spectroscopic data from various telescopes, including ESO VLT UT3 (Melipal) and Gemini-North.
|
[
"ESO VLT UT3 (Melipal)",
"Gemini-North",
"GRB 250101A: z = 2.49",
"GRB 250103A: not spectroscopic",
"GRB 250103B: z = 1.416",
"GRB 250108B: z = 0.29, 2.197"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.14858v1
|
https://arxiv.org/abs/2511.14858v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
7044827765188406025744d783dfafa6f912d2f7fe2a950d2100e425f5d5730a
|
Extracted from ArXiv paper 2511.14858v1 (chunk 44)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 44,
"paper_id": "2511.14858v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:19:50.790748Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_123759183023
|
The cross section of πβ² photoproduction has been measured at various angles and πsettings, but lacks data in the forward and backward angular regions.
|
The cross section of πβ² photoproduction has been measured at various angles and πsettings, but lacks data in the forward and backward angular regions.
|
[
"SAPHIR",
"CLAS",
"CBELSA/TAPS",
"A2MAMI",
"LEPS",
"JLab E12-17-003 experiment"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.17030v1
|
https://arxiv.org/abs/2511.17030v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ce5ac30f3ea29271d66a08f6e9c2213042b0aa8563de917112f64440b2e8304c
|
Extracted from ArXiv paper 2511.17030v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2511.17030v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:37:59.183023Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_113109405403
|
Cosmogenic muon-induced neutron yield per muon measured with a track length-dependent efficiency, yielding an average of 89.8 Β± 3.7 neutrons per muon
|
Cosmogenic muon-induced neutron yield per muon measured with a track length-dependent efficiency, yielding an average of 89.8 Β± 3.7 neutrons per muon
|
[
"OWL hits β₯5",
"Calibrated PMT hits β₯1238",
"13,690 selected cosmogenic muons",
"1,412 neutron followers"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.04600v2
|
https://arxiv.org/abs/2511.04600v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d0b8b6894647f61e6bef4eea8ac3d1278426026736cd4e84905bedb1c810f400
|
Extracted from ArXiv paper 2511.04600v2 (chunk 6)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 6,
"paper_id": "2511.04600v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T11:31:09.405403Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_113847475709
|
The ERECO distribution is measured to be sensitive to the Higgs boson CP properties, providing complementary sensitivity to the CP-odd admixture in the Higgs sector.
|
The ERECO distribution is measured to be sensitive to the Higgs boson CP properties, providing complementary sensitivity to the CP-odd admixture in the Higgs sector.
|
[
"ATLAS detector",
"ERECO variable",
"ISR energy spectrum",
"cross-section Ο(e+eββHZ)"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2511.06353v1
|
https://arxiv.org/abs/2511.06353v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
1492f44f306084eb455f628f0daa96c75591139caec025d547ea47a36cac00a8
|
Extracted from ArXiv paper 2511.06353v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2511.06353v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T11:38:47.475709Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_113941462344
|
A broad Feshbach resonance in the atom-molecule mixture was observed at magnetic field B0 = 217.3(4) G, with a measured peak loss rate coefficient about 3 times larger than the universal loss rate coefficient.
|
A broad Feshbach resonance in the atom-molecule mixture was observed at magnetic field B0 = 217.3(4) G, with a measured peak loss rate coefficient about 3 times larger than the universal loss rate coefficient.
|
[
"Belle II detector",
"loss features after ramping the magnetic field",
"measured loss rate coefficients vs. magnetic fields (inset of Fig. 1)",
"Lorentzian fit to the data"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2511.06772v1
|
https://arxiv.org/abs/2511.06772v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
584b2fb12a738770db3fcc1243574aba9d79a711abbd72e15f4b7197664dae3f
|
Extracted from ArXiv paper 2511.06772v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2511.06772v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T11:39:41.462344Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_120654206938
|
Neutrino telescopes have been developed with detectors in deep subsurface locations to detect extraterrestrial neutrinos, spanning volumes up to a cubic kilometer.
|
Neutrino telescopes have been developed with detectors in deep subsurface locations to detect extraterrestrial neutrinos, spanning volumes up to a cubic kilometer.
|
[
"IceCube Neutrino Observatory",
"Antarctic ice location",
"Baikal-GVD telescope in Lake Baikal",
"KM3NeT in the Mediterranean Sea"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2511.13111v2
|
https://arxiv.org/abs/2511.13111v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e6717a91dbef131a4ff6f8172c7ac0f5d78e4d1c992faa44539336d0d12c13d2
|
Extracted from ArXiv paper 2511.13111v2 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2511.13111v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:06:54.206938Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_122417321645
|
The LHAASO-KM2A detector registered a 10Ο photon-like event lasting 6000 s with energy up to βΌ18 TeV, and the Carpet-2 collaboration detected a single photon with E = 251 TeV from the BOAT position.
|
The LHAASO-KM2A detector registered a 10Ο photon-like event lasting 6000 s with energy up to βΌ18 TeV, and the Carpet-2 collaboration detected a single photon with E = 251 TeV from the BOAT position.
|
[
"LHAASO-KM2A detector",
"Significance: 10Ο",
"Energy range: up to βΌ18 TeV",
"Carpet-2 collaboration, detection of E = 251 TeV photon"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2511.15542v1
|
https://arxiv.org/abs/2511.15542v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
367e0d9e7b1fde5e5845eeb0822447eacb7df9a1343329dbc9ac9ec9735873e7
|
Extracted from ArXiv paper 2511.15542v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2511.15542v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:24:17.321645Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_123200524019
|
The CMS detector recorded a total luminosity of 139.0 Β± 2.4 fb^(-1) during the 2017 data-taking period at a center-of-mass energy of 13 TeV.
|
The CMS detector recorded a total luminosity of 139.0 Β± 2.4 fb^(-1) during the 2017 data-taking period at a center-of-mass energy of 13 TeV.
|
[
"CMS detector",
"2017 data-taking period",
"Total luminosity: 139.0 Β± 2.4 fb^(-1)",
"Center-of-mass energy: 13 TeV"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.16394v2
|
https://arxiv.org/abs/2511.16394v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d2b8649fb67866cb09896222d9142259e33db60252d69b86bc1012c8d14ed13c
|
Extracted from ArXiv paper 2511.16394v2 (chunk 16)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 16,
"paper_id": "2511.16394v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:32:00.524019Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_123237753705
|
A bulk field of 3.1 kV/cm was measured at 95% survival probability in GAr, with upper and lower bounds of 2.8 kV/cm and 3.4 kV/cm.
|
A bulk field of 3.1 kV/cm was measured at 95% survival probability in GAr, with upper and lower bounds of 2.8 kV/cm and 3.4 kV/cm.
|
[
"GAr atmosphere",
"1.0 bar pressure",
"4.97 cm gap distance",
"293 K temperature"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.16408v1
|
https://arxiv.org/abs/2511.16408v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
f5b4863766673032182495db16621501070fdf0706a4cad7bcb5a36982024b73
|
Extracted from ArXiv paper 2511.16408v1 (chunk 22)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 22,
"paper_id": "2511.16408v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:32:37.753705Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_124007222022
|
Temperature of the Milky Way's X-ray-emitting halo measured as 0.19 Β± 0.05 keV using various observations
|
Temperature of the Milky Way's X-ray-emitting halo measured as 0.19 Β± 0.05 keV using various observations
|
[
"XMM-Newton sightlines",
"HaloSat all-sky survey",
"Suzaku observations",
"eFEDS field"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.17313v1
|
https://arxiv.org/abs/2511.17313v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
6df9f59a3c05a963cf7d27be7c103941ee89ccc7db0aedf34228ffc347393043
|
Extracted from ArXiv paper 2511.17313v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2511.17313v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T12:40:07.222022Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_130028425363
|
The in-medium nucleon-nucleon elastic cross sections are parameterized based on thermodynamic T-matrix calculations, showing a significant suppression of the cross sections during Au+Au collisions at βsNN = 2.4 GeV.
|
The in-medium nucleon-nucleon elastic cross sections are parameterized based on thermodynamic T-matrix calculations, showing a significant suppression of the cross sections during Au+Au collisions at βsNN = 2.4 GeV.
|
[
"HAD-ES experiment",
"Local density of nucleons Ο",
"Total kinetic energy of two scattering nucleons Tc.m.",
"In-medium correction parameter Ξ± = 1.8"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.20387v1
|
https://arxiv.org/abs/2511.20387v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
1107588774a222d8a5635cdb6465eead23f1079248e1ab8f86117cd67fececf6
|
Extracted from ArXiv paper 2511.20387v1 (chunk 6)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 6,
"paper_id": "2511.20387v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:00:28.425363Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_131722501562
|
We present a study on the performance of the ATLAS detector at the LHC, achieving an efficiency of 92% for muon reconstruction with a misidentification rate of 2.5%
|
We present a study on the performance of the ATLAS detector at the LHC, achieving an efficiency of 92% for muon reconstruction with a misidentification rate of 2.5%
|
[
"ATLAS detector",
"2022 LHC run",
"Muon reconstruction efficiency: 92%",
"Misidentification rate: 2.5%"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.23091v1
|
https://arxiv.org/abs/2511.23091v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
5c529cf4fd1c7aa82553875903423afc78f10b573b056d1ef4a00580316129a9
|
Extracted from ArXiv paper 2511.23091v1 (chunk 33)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 33,
"paper_id": "2511.23091v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:17:22.501562Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_131916903573
|
A parameterised simulation in DELPHES estimates the tracking and vertexing performance of the IDEA detector concept, with a resolution of 3 Β΅m for the inner detector and 100 Β΅m for the drift chamber.
|
A parameterised simulation in DELPHES estimates the tracking and vertexing performance of the IDEA detector concept, with a resolution of 3 Β΅m for the inner detector and 100 Β΅m for the drift chamber.
|
[
"DELPHES simulation software",
"IDEA detector concept",
"5 Monolithic silicon pixel (MAPS) layers",
"High-transparency and high-resolution drift chamber"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.23337v1
|
https://arxiv.org/abs/2511.23337v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ec5671798dd6c44443c0e1f9af77b13c66317cc5eaa63ac1facdf5b132d7f5a9
|
Extracted from ArXiv paper 2511.23337v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2511.23337v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:19:16.903573Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_132004479392
|
The sensitivity of Tera-Z factories for discovering heavy neutral leptons and ALPs is determined by the detector dimensions, integrated luminosity, and background removal algorithms.
|
The sensitivity of Tera-Z factories for discovering heavy neutral leptons and ALPs is determined by the detector dimensions, integrated luminosity, and background removal algorithms.
|
[
"Tera-Z factory setup",
"Detector dimensions: not specified",
"Integrated luminosity: not specified",
"Background removal algorithms: improved"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2511.23461v1
|
https://arxiv.org/abs/2511.23461v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
38f2c0873d5c82d0b37b682491c78be97f532629756e447949aee921d1ca8b20
|
Extracted from ArXiv paper 2511.23461v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2511.23461v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:20:04.479392Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_132156251478
|
Electromagnetic shower physics is adapted to new geometric configurations, preserving fundamental particle shower physics while adjusting to changes in spatial scale and detector granularity
|
Electromagnetic shower physics is adapted to new geometric configurations, preserving fundamental particle shower physics while adjusting to changes in spatial scale and detector granularity
|
[
"ILD detector",
"Compact ILD geometry",
"CaloChallenge dataset 3",
"Cylindrical calorimeter geometry"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2512.00187v1
|
https://arxiv.org/abs/2512.00187v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e8806423d8dd4c6d23e184dd807b5f1db33598f213ff79691dca231cd8e5eaa3
|
Extracted from ArXiv paper 2512.00187v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2512.00187v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:21:56.251478Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_133327324996
|
The cross section ratio ΟLTβ²/Ο0 was measured in exclusive pion electroproduction from the proton, with a fairly flat Q2-dependence over the explored range.
|
The cross section ratio ΟLTβ²/Ο0 was measured in exclusive pion electroproduction from the proton, with a fairly flat Q2-dependence over the explored range.
|
[
"KaonLT experiment at Jefferson Lab Hall C",
"10.6 GeV longitudinally polarized electron beam",
"Unpolarized liquid hydrogen target",
"Cross section ratio ΟLTβ²/Ο0 determined at fixed Q2 and xB over a range of kinematics"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2512.01928v1
|
https://arxiv.org/abs/2512.01928v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
3d1262951448eb8294e8d1dc3f17c65eae9df53f0103bdc43493a04aff3fe9e5
|
Extracted from ArXiv paper 2512.01928v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2512.01928v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T13:33:27.325515Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251209_211028756125
|
Evaporation rate (ER) measured for water, silica slurry, and tailing suspensions at varying solid concentrations
|
Evaporation rate (ER) measured for water, silica slurry, and tailing suspensions at varying solid concentrations
|
[
"sailboat evaporator setup",
"wind velocity: 4 m/s",
"silica slurry ER: 4.9 kg/(m2h)",
"tailing suspension ER: 4 kg/(m2h)"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2512.02939v1
|
https://arxiv.org/abs/2512.02939v1
|
[
"physics.app-ph"
] |
49e9c11e39ed402bf147aa1c82b218a763d405aeaf3d7162de1138befd85822e
|
Extracted from ArXiv paper 2512.02939v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2512.02939v1"
}
|
science
|
WO-ARX-01
|
2025-12-09T21:10:28.756125Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100746007652
|
Spin-polarized tritium scattering cross sections calculated for a range of magnetic fields and temperatures, advancing beyond previous literature.
|
Spin-polarized tritium scattering cross sections calculated for a range of magnetic fields and temperatures, advancing beyond previous literature.
|
[
"Calculations based on the Distorted Wave Born Approximation (DWBA) and coupled-channel formalisms",
"Benchmarked against results from atomic hydrogen by Stoof et. al. [56]",
"Comprehensive set of cross sections spanning magnetic field and temperature ranges"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.13426v1
|
https://arxiv.org/abs/2509.13426v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
09b3d3a9de64fa23603b6d35ae1564182ce3b3b86c92373b8e14bcbde5adf7f4
|
Extracted from ArXiv paper 2509.13426v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2509.13426v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:07:46.007652Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100838502977
|
The phase shift in an optical detector can be directly related to the Riemann tensor, which is gauge-invariant.
|
The phase shift in an optical detector can be directly related to the Riemann tensor, which is gauge-invariant.
|
[
"null geodesic calculation",
"Riemann tensor: Rx0x0 = Β¨h/2",
"Eq. (3) and Eq. (4)"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.15841v2
|
https://arxiv.org/abs/2509.15841v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e2d3558644b2a5b88e2aafc968da827464d17fe5416733adb237380c40571919
|
Extracted from ArXiv paper 2509.15841v2 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2509.15841v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:08:38.502977Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100844768708
|
A proposed gravitational wave detector design enables the detection of any polarisation through correlation of signals between three measurement channels.
|
A proposed gravitational wave detector design enables the detection of any polarisation through correlation of signals between three measurement channels.
|
[
"Two ultrastable lasers at frequencies fA and fB",
"One optical atomic reference at frequency fatom",
"Detection sensitivity improved by βN with N detectors across different geographical locations"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.15841v2
|
https://arxiv.org/abs/2509.15841v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
7e921e84feef861bed13c73afdd343a20695920eab4bc5e72949bfa9b4c03800
|
Extracted from ArXiv paper 2509.15841v2 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2509.15841v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:08:44.768708Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100850829901
|
A proposed detector utilizing optical frequency metrology is capable of detecting compact binaries in the Milky Way and black hole mergers at cosmological distances, with potential to probe GW background beyond cosmological indirect limits for frequencies below 10^(-2) Hz
|
A proposed detector utilizing optical frequency metrology is capable of detecting compact binaries in the Milky Way and black hole mergers at cosmological distances, with potential to probe GW background beyond cosmological indirect limits for frequencies below 10^(-2) Hz
|
[
"optical atomic reference cavities",
"global network of clocks",
"compact binaries in the Milky Way"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.15841v2
|
https://arxiv.org/abs/2509.15841v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
81b821a13fc0c55cc047f2f1a2c32f438c0a76bb58a5049ed6945c24e35727d5
|
Extracted from ArXiv paper 2509.15841v2 (chunk 7)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 7,
"paper_id": "2509.15841v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:08:50.829901Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100832631610
|
Rovibrational spectra of the hydronium ion H3O+ were measured for two strongest first overtone bands, with band origins determined to be 6845.610(14) cmβ1 and 6878.393(13) cmβ1.
|
Rovibrational spectra of the hydronium ion H3O+ were measured for two strongest first overtone bands, with band origins determined to be 6845.610(14) cmβ1 and 6878.393(13) cmβ1.
|
[
"temperature-variable cryogenic 22 pole ion trap",
"leak-out spectroscopy (LOS)",
"energy range of 6750β6950 cmβ1"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.16009v1
|
https://arxiv.org/abs/2509.16009v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
1bdeb44c7397ec50acc2f8f33117d01fc59d24338c703af1737c7ed8b2e1ec18
|
Extracted from ArXiv paper 2509.16009v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2509.16009v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:08:32.631610Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100848564396
|
The overtone spectrum of H3O+ was measured and simulated, with 68 out of 85 transitions assigned to either the 2Ξ½2+ or 2Ξ½2- band.
|
The overtone spectrum of H3O+ was measured and simulated, with 68 out of 85 transitions assigned to either the 2Ξ½2+ or 2Ξ½2- band.
|
[
"20 K re-measured spectrum",
"Linear extrapolations from Yu et al. (2015)",
"68/85 transitions fitted using PGOPHER"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.16009v1
|
https://arxiv.org/abs/2509.16009v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
fcffea407624568592f580986c0381647329ad5dfdbf146f0c39ee27162973ee
|
Extracted from ArXiv paper 2509.16009v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2509.16009v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:08:48.564396Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100913707701
|
Long-range AFM correlations are observed in the system, revealing striped phase order with a period of two lattice sites.
|
Long-range AFM correlations are observed in the system, revealing striped phase order with a period of two lattice sites.
|
[
"ArXiv Paper 2509.16200v1 experimental results",
"Structure factor peaks at (Ο, 0) indicating AFM stripes",
"Finite inter-chain coupling Vx = Vy stabilizes the confined phase"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.16200v1
|
https://arxiv.org/abs/2509.16200v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
6c966687576e1310bc1f1194a899be71e10bd85ae34acd87e43cb36622b2ed87
|
Extracted from ArXiv paper 2509.16200v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2509.16200v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:09:13.707701Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100916447497
|
Super-stripes with a period of three lattice sites are observed in the system at one-third filling, stabilized by low temperature and finite inter-chain coupling.
|
Super-stripes with a period of three lattice sites are observed in the system at one-third filling, stabilized by low temperature and finite inter-chain coupling.
|
[
"Finite magnetization regime |m| β0.15",
"Low tunneling rate tx/Vx = 0.137",
"Inter-chain coupling Vy = Vx"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.16200v1
|
https://arxiv.org/abs/2509.16200v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
cc758567b626703f8ad4b90f4c788af63c502a87eb64333863e58efc2b227826
|
Extracted from ArXiv paper 2509.16200v1 (chunk 10)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 10,
"paper_id": "2509.16200v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:09:16.447497Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_100921081337
|
The group velocity of dark spin waves vanishes near a critical point, leading to a divergent total cross section.
|
The group velocity of dark spin waves vanishes near a critical point, leading to a divergent total cross section.
|
[
"Numerical calculations in Fig. 2(c1)",
"Critical energy dependence on incoming relative momentum q",
"Diverging inverse group velocity vβ1g β βEβ1/2"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.17085v1
|
https://arxiv.org/abs/2509.17085v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
af599f12e65e86dd45f150a8270aacb1a485e0055d2ebc3a79046298837204df
|
Extracted from ArXiv paper 2509.17085v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2509.17085v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:09:21.081337Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101023461155
|
We characterise the performance of two-qubit entangling gates with measured Bell-state fidelities: 99.8% for the LS gate, 99.6% for the stretch-Zeeman MS gate, and 96% for the clock-Zeeman MS gate.
|
We characterise the performance of two-qubit entangling gates with measured Bell-state fidelities: 99.8% for the LS gate, 99.6% for the stretch-Zeeman MS gate, and 96% for the clock-Zeeman MS gate.
|
[
"partial state tomography",
"Bell state |βββ©and |βββ©populations measured",
"parity contrast observed using two-point method"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.17893v1
|
https://arxiv.org/abs/2509.17893v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
aa2fef790bd9af7b4406c8dac4d6bbf35592012d227e590ed83934f8ae43acd1
|
Extracted from ArXiv paper 2509.17893v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2509.17893v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:10:23.461155Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101027838374
|
A compressibility maximum is observed in the doped Hubbard model at low temperatures and strong interactions.
|
A compressibility maximum is observed in the doped Hubbard model at low temperatures and strong interactions.
|
[
"DQMC simulations",
"Compressibility maxima observed at various interaction strengths (U/t = 4.67, 5.72, 7.00, 10.29)",
"Not observed at U/t = 2.79 or 3.69"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.18075v1
|
https://arxiv.org/abs/2509.18075v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
fc3b1bf04db019526d0e4c626003dee010811b4d1eae0c991c6c670a595c24ca
|
Extracted from ArXiv paper 2509.18075v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2509.18075v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:10:27.838374Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101138192319
|
Averaged cross-sectional area SI for photon retrieval and conversion was measured to be equal to the effective absorption volume SM, enabling precise tuning of average MW photon number.
|
Averaged cross-sectional area SI for photon retrieval and conversion was measured to be equal to the effective absorption volume SM, enabling precise tuning of average MW photon number.
|
[
"Collinear configuration",
"Mean beam radius: 66 ΞΌm",
"Pulse duration t0"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.18834v1
|
https://arxiv.org/abs/2509.18834v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
40c0ad43fd5b9480f03cd3f735bb41feec1a54aa125dd722211209e93f9bb84b
|
Extracted from ArXiv paper 2509.18834v1 (chunk 17)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 17,
"paper_id": "2509.18834v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:11:38.192319Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101122726544
|
HHG from a BEC yields distinct quantum states above and below the critical temperature, with entanglement and squeezing observed in the pure state.
|
HHG from a BEC yields distinct quantum states above and below the critical temperature, with entanglement and squeezing observed in the pure state.
|
[
"Bose-Einstein condensate",
"High harmonic generation process",
"Critical temperature Tc"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.19022v2
|
https://arxiv.org/abs/2509.19022v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
afb246d6696dba2066e05623de17a5740cec3917c91d8e3e5c9826cf6b5ff69e
|
Extracted from ArXiv paper 2509.19022v2 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2509.19022v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:11:22.726544Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101231678362
|
A 100 kHz linewidth for the 1S0 to 3P1 intercombination line of 88Sr at 689 nm is measured in a microfabricated Sr vapor cell, representing a factor of 10 reduction in observed atomic linewidth compared to previous narrowest optical-transition linewidths.
|
A 100 kHz linewidth for the 1S0 to 3P1 intercombination line of 88Sr at 689 nm is measured in a microfabricated Sr vapor cell, representing a factor of 10 reduction in observed atomic linewidth compared to previous narrowest optical-transition linewidths.
|
[
"Microfabricated Sr vapor cell",
"Strontium atomic density: β1011 cmβ3",
"Cell operating temperature: 350 β¦C"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.20619v1
|
https://arxiv.org/abs/2509.20619v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
c16b85e0f561ee225b6595ff4fa30bbeb7ff992948d4fceaf96cebcc6a14c042
|
Extracted from ArXiv paper 2509.20619v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2509.20619v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:12:31.678886Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101241020203
|
Linewidth of the 689 nm Sr intercombination line measured to be 100 kHz in a microfabricated vapor cell, with an upper bound on residual gas pressure of 10 mTorr.
|
Linewidth of the 689 nm Sr intercombination line measured to be 100 kHz in a microfabricated vapor cell, with an upper bound on residual gas pressure of 10 mTorr.
|
[
"Microfabricated vapor cell",
"100 kHz broadening attributed to residual Doppler broadening and laser linewidth",
"Estimated upper bound: 10 mTorr residual Ar gas pressure"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.20619v1
|
https://arxiv.org/abs/2509.20619v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
5a80438025643dacb7666d96570b94f07dc5361d5bc3213d5c6e3a974223607a
|
Extracted from ArXiv paper 2509.20619v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2509.20619v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:12:41.020717Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101251738607
|
The Rydberg sensor's sensitivity was measured to be 10.6 Β΅V/T with a resolution bandwidth of 10 Hz, and the system's dominant noise source was identified as the probe laser.
|
The Rydberg sensor's sensitivity was measured to be 10.6 Β΅V/T with a resolution bandwidth of 10 Hz, and the system's dominant noise source was identified as the probe laser.
|
[
"Spectrum analyzer measurements at various beatnote frequencies (10 kHz to 10 MHz)",
"Optical homodyne technique used to separate signal from noise",
"Calibration factor obtained using Autler-Townes splitting"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.20632v1
|
https://arxiv.org/abs/2509.20632v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
71b93543226b9c131eaa037c8c26926acd35bafde114c81ba2a317b8c49cd17d
|
Extracted from ArXiv paper 2509.20632v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2509.20632v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:12:51.738607Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101255208361
|
The sensitivity of a Rydberg sensor is measured to be 9.9(4) Β΅V/m/βHz at 100 kHz with a coupling power of 140 mW, while the system is dominated by probe laser noise.
|
The sensitivity of a Rydberg sensor is measured to be 9.9(4) Β΅V/m/βHz at 100 kHz with a coupling power of 140 mW, while the system is dominated by probe laser noise.
|
[
"Spectrum analyzer traces with resolution bandwidth of 10 Hz from 10 kHz to 10 MHz",
"RF signal field power sweep versus SNR in Figure (3a)",
"Beatnote frequencies up to 8 MHz"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.20632v1
|
https://arxiv.org/abs/2509.20632v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9d1a3c84409eeca36a2f8bfa83d44046c811357cd3e42636a2c908ac0cc6b6d5
|
Extracted from ArXiv paper 2509.20632v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2509.20632v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:12:55.208361Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101248152455
|
Resonant monopole-dipole energy transfer observed between Rydberg atoms and polar molecules, with evidence of charge-dipole interaction
|
Resonant monopole-dipole energy transfer observed between Rydberg atoms and polar molecules, with evidence of charge-dipole interaction
|
[
"Low-temperature (βΌ80 mK) collisions in helium",
"Ammonia molecules undergo inversion transitions",
"Rydberg-electron and molecular wavefunctions have spatial overlap"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.21582v1
|
https://arxiv.org/abs/2509.21582v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
361645d6f2fa81777ce5c71a2b054d125a1e763f49351456b2d1897ac5642968
|
Extracted from ArXiv paper 2509.21582v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2509.21582v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:12:48.152455Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101411992770
|
Static and dynamic polarizabilities of the 1S0 and 3P0 states in Al+ measured at 397 nm, 866 nm, and 1068 nm with uncertainties ranging from 10^-18 to 14
|
Static and dynamic polarizabilities of the 1S0 and 3P0 states in Al+ measured at 397 nm, 866 nm, and 1068 nm with uncertainties ranging from 10^-18 to 14
|
[
"CI+all-order+AC approximation",
"Tables V, VI, VII",
"Uncertainties calculated for various effects"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.22525v1
|
https://arxiv.org/abs/2509.22525v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ffe79bdcb4f771bd2e9c42246c795a5544469c779d603f67b1621a3bd9d91758
|
Extracted from ArXiv paper 2509.22525v1 (chunk 16)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 16,
"paper_id": "2509.22525v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:14:11.992770Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101349874822
|
Electronic vortex states are observed in multiphoton ionization of Xe and H atoms using a single elliptically polarized intense laser pulse, with spiral patterns in the photoelectron momentum distribution indicating interference between states of different OAM.
|
Electronic vortex states are observed in multiphoton ionization of Xe and H atoms using a single elliptically polarized intense laser pulse, with spiral patterns in the photoelectron momentum distribution indicating interference between states of different OAM.
|
[
"3D velocity map imaging (3DVMI) apparatus",
"Intensity at the focus: β2 Γ 10^13 W/cm2 (Keldysh parameter Ξ³ β2)",
"Data analysis provides clean above-threshold ionization (ATI) spectra"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.22817v1
|
https://arxiv.org/abs/2509.22817v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
1474f4c2d43404d96e11ca372b4c620d7a90ae16bb4d7fb3753b44c48b44e19b
|
Extracted from ArXiv paper 2509.22817v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2509.22817v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:13:49.874822Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101438554600
|
Double differential cross section (DDCS) for electron impact energy EI = 250eV and ejected electron energy Ea = 10eV shows a broad peak-shaped pattern in the binary zone, aligning with Shyn's experimental findings.
|
Double differential cross section (DDCS) for electron impact energy EI = 250eV and ejected electron energy Ea = 10eV shows a broad peak-shaped pattern in the binary zone, aligning with Shyn's experimental findings.
|
[
"Current calculations",
"Das et al. (1995)",
"Shyn's results"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.23953v2
|
https://arxiv.org/abs/2509.23953v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
2f9115d807eb1277f16a5b6b519dcef4964920cd141bc2ee85ea5a81f67735f8
|
Extracted from ArXiv paper 2509.23953v2 (chunk 7)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 7,
"paper_id": "2509.23953v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:14:38.554600Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101441513510
|
Double differential cross sections (DDCS) for ionization of a metastable hydrogen atom (3S state) after electron impact have been calculated and compared with existing theories.
|
Double differential cross sections (DDCS) for ionization of a metastable hydrogen atom (3S state) after electron impact have been calculated and compared with existing theories.
|
[
"Second Born approximation, Das et al. [1] theory",
"Ejected electron energies: Ea = 10eV, 20eV, 50eV",
"Scattering angles: ππ(deg) from Table-1"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.23953v2
|
https://arxiv.org/abs/2509.23953v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
f6214bd424293e13fb8cedfdb49beeb199100496c54ab8538580ba7fc9e675d8
|
Extracted from ArXiv paper 2509.23953v2 (chunk 8)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 8,
"paper_id": "2509.23953v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:14:41.513510Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101443843701
|
The β-resonance contribution to the unpolarized elastic scattering cross sections remains at the permille level, with no significant kinematic enhancements.
|
The β-resonance contribution to the unpolarized elastic scattering cross sections remains at the permille level, with no significant kinematic enhancements.
|
[
"Charged-current (anti)neutrino-nucleon elastic scattering study",
"Accelerator neutrino energies considered",
"Virtual contributions of the βintermediate state determined"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.24011v1
|
https://arxiv.org/abs/2509.24011v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d658565fc357ce7de89a5f6c6cb795860f6afa27c8f9d012c512d65b36843caa
|
Extracted from ArXiv paper 2509.24011v1 (chunk 6)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 6,
"paper_id": "2509.24011v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:14:43.843701Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101607972468
|
Branching ratios for Ξ²p decay channel of 55Zn and 2p radioactivity of 54Zn measured with high precision
|
Branching ratios for Ξ²p decay channel of 55Zn and 2p radioactivity of 54Zn measured with high precision
|
[
"RIBF accelerator data",
"BR(55Cu; Ξ²p) = (4.3 Β± 0.6)%",
"250 events recorded in Ξ²p decay channel"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.25061v1
|
https://arxiv.org/abs/2509.25061v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
4c25fb94875bb6b2e38874e2106390c26d87bf1f87d8ba941b2965ddb9ced70b
|
Extracted from ArXiv paper 2509.25061v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2509.25061v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:16:07.972468Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101603625308
|
Rapidity-odd directed flow for Kβ0 mesons is measured to be positive in mid-central Au+Au collisions at βsNN = 19.6 GeV, indicating late-stage hadronic interactions.
|
Rapidity-odd directed flow for Kβ0 mesons is measured to be positive in mid-central Au+Au collisions at βsNN = 19.6 GeV, indicating late-stage hadronic interactions.
|
[
"STAR experiment at RHIC",
"Minimum-bias data from BES-II program",
"10-40% centralities"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.25735v1
|
https://arxiv.org/abs/2509.25735v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
614b452c623e0f6f55392f3322e61b06c558bcfda635cfe3699858119be12974
|
Extracted from ArXiv paper 2509.25735v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2509.25735v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:16:03.625817Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101635740762
|
Nuclear shape transition in light gold isotopes observed, with implications for nuclear structure and properties
|
Nuclear shape transition in light gold isotopes observed, with implications for nuclear structure and properties
|
[
"Nucl. Phys. A 493, 224 (1989)",
"K. Wallmeroth et al.",
"Shape coexistence studied in Pt isotopes"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.25789v2
|
https://arxiv.org/abs/2509.25789v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d78ddff117c1af0cdf8db05363421ebd88e6ca681538d19152699ddb81aecf0f
|
Extracted from ArXiv paper 2509.25789v2 (chunk 14)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 14,
"paper_id": "2509.25789v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:16:35.740762Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101634119689
|
The instantaneous bandwidth of the receiver is measured as 5 MHz at each chosen position, with a 3 dB power attenuation.
|
The instantaneous bandwidth of the receiver is measured as 5 MHz at each chosen position, with a 3 dB power attenuation.
|
[
"Individual cell measurement",
"21 positions examined",
"Spectrum analyzer used to analyze output beat notes"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.26026v1
|
https://arxiv.org/abs/2509.26026v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ab484e5d87ccc7da17e488a1fae630827434e2f8339167a6b3e6f2daa3c340d8
|
Extracted from ArXiv paper 2509.26026v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2509.26026v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:16:34.119689Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101638778038
|
Tritium breeding ratio measured six-fold improved compared to initial experiments, with good agreement between experiment and OpenMC simulations
|
Tritium breeding ratio measured six-fold improved compared to initial experiments, with good agreement between experiment and OpenMC simulations
|
[
"BABY 1L experiment, MIT Plasma Science and Fusion Center",
"Four irradiation experiments using sealed-tube DT neutron generators",
"Tritium collected by water bubblers measured via liquid scintillation counting"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2509.26174v1
|
https://arxiv.org/abs/2509.26174v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
fa6463fdfc95e138c85442f42779110983e32951a35a0cf21a340726d37ccc41
|
Extracted from ArXiv paper 2509.26174v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2509.26174v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:16:38.778038Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101711139196
|
Hydrogen introduction enhances tritium release, with significantly faster release observed when introduced from the beginning.
|
Hydrogen introduction enhances tritium release, with significantly faster release observed when introduced from the beginning.
|
[
"BABY experiment",
"Run 4 data showing enhanced release after switching to H2",
"96% of tritium collected in water-insoluble forms (HT, T2)"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.26174v1
|
https://arxiv.org/abs/2509.26174v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
f0859a953448d2685c245e5869cc0022a0a09e97cc75a0b4a769c518fc82348b
|
Extracted from ArXiv paper 2509.26174v1 (chunk 10)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 10,
"paper_id": "2509.26174v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:17:11.139196Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101705420937
|
Direct-photon elliptic flow measured as v2 = 0 in high pT region, consistent with expected early photon production
|
Direct-photon elliptic flow measured as v2 = 0 in high pT region, consistent with expected early photon production
|
[
"PHENIX detector, Au+Au collisions at βsNN = 200 GeV",
"Data taken in 2014, large data set analyzed",
"pT range: 12-18 GeV/c"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.26456v1
|
https://arxiv.org/abs/2509.26456v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
85e0923c717a18ff6a9950641881a4788e8f4b19a802784320b3fd7ef3558a7f
|
Extracted from ArXiv paper 2509.26456v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2509.26456v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:17:05.420937Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101720484428
|
Laser-cooled atoms are imaged and measured via fluorescence and absorption techniques, with images acquired using three cameras.
|
Laser-cooled atoms are imaged and measured via fluorescence and absorption techniques, with images acquired using three cameras.
|
[
"Three cameras used for imaging: ex-camera, ey-camera, ez-camera",
"Fluorescence and absorption imaging methods employed",
"Images acquired under various experimental conditions"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2509.26479v1
|
https://arxiv.org/abs/2509.26479v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9a637932364240c90ca1a318fd158d1b530e136214d178ed82c06c5f62d89856
|
Extracted from ArXiv paper 2509.26479v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2509.26479v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:17:20.484428Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101747045785
|
Sucrose crystals were operated as a particle detector at milliKelvin temperatures for the first time, with potential applications in direct dark matter detection.
|
Sucrose crystals were operated as a particle detector at milliKelvin temperatures for the first time, with potential applications in direct dark matter detection.
|
[
"sucrose monocrystal",
"milliKelvin temperatures",
"first results of the SWEET project"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.00068v1
|
https://arxiv.org/abs/2510.00068v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
35f8c269d70d37358c0dbd7a0d535c7c07d7df886bb831c408c8bf96282cd4ae
|
Extracted from ArXiv paper 2510.00068v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2510.00068v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:17:47.046303Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101902096867
|
Plasmoid instability onset observed at Lundquist number Sc β1.5 Γ 104, transitioning reconnection rate from Sweet-Parker to tearing-dominated regime
|
Plasmoid instability onset observed at Lundquist number Sc β1.5 Γ 104, transitioning reconnection rate from Sweet-Parker to tearing-dominated regime
|
[
"High-resolution 2D MHD simulations",
"Lundquist numbers ranging from 103 to 2 Γ 105",
"Tearings instabilities and numerical errors estimated"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.01060v2
|
https://arxiv.org/abs/2510.01060v2
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
82cb028fb99a973f50160cbccb599b31b1e658f312b0a4279dfe6cf799d4fe01
|
Extracted from ArXiv paper 2510.01060v2 (chunk 15)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 15,
"paper_id": "2510.01060v2"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:19:02.096867Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101906836761
|
Intermediate- and high-spin states in the odd-even 69Ga nucleus were populated following the 26Mg(48Ca, p4n) reaction, producing a new level scheme with collective sequences observed at high spins.
|
Intermediate- and high-spin states in the odd-even 69Ga nucleus were populated following the 26Mg(48Ca, p4n) reaction, producing a new level scheme with collective sequences observed at high spins.
|
[
"Gammasphere detector array",
"195-MeV 48Ca beam from ATLAS accelerator system",
"High-purity germanium detectors with BGO Compton suppressors"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.01423v1
|
https://arxiv.org/abs/2510.01423v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
dba427694dbb7328ed0e58969fa599c115b69220cf72078a67e516b2449f7adc
|
Extracted from ArXiv paper 2510.01423v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.01423v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:19:06.836761Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_101959270466
|
The narrow resonance at Ecm β 366keV has a strength of (9.3Β±0.6)Γ10^(-14)meV, measured with improved precision
|
The narrow resonance at Ecm β 366keV has a strength of (9.3Β±0.6)Γ10^(-14)meV, measured with improved precision
|
[
"LUNA400 accelerator",
"natural neon gas target, 2 mbar pressure",
"200 Β΅A beam current"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.01884v1
|
https://arxiv.org/abs/2510.01884v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9691d60eaf06affd86822134937096cd8caf3b8cf470741f535e31d706cbc403
|
Extracted from ArXiv paper 2510.01884v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2510.01884v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:19:59.270466Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102115288158
|
Significant elliptic and triangular flow harmonics observed in oxygen-oxygen and neon-neon collisions, with ratios between the two systems revealing sensitivity to quadrupole correlations in nuclear wave functions.
|
Significant elliptic and triangular flow harmonics observed in oxygen-oxygen and neon-neon collisions, with ratios between the two systems revealing sensitivity to quadrupole correlations in nuclear wave functions.
|
[
"CMS detector at CERN LHC",
"Center-of-mass energy per nucleon pair: 5.36 TeV",
"Integrated luminosities: 7 nbβ1 and 0.8 nbβ1 for OO and NeNe collisions"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.02580v1
|
https://arxiv.org/abs/2510.02580v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
054b88a13a874dc749e1ea09e883a51a29969875628eeacd85f1c685422a87e0
|
Extracted from ArXiv paper 2510.02580v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2510.02580v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:21:15.288158Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102134067146
|
The azimuthal anisotropy of charged-particle emission is measured in oxygen-oxygen and neon-neon collisions, revealing sensitivity to the underlying geometry.
|
The azimuthal anisotropy of charged-particle emission is measured in oxygen-oxygen and neon-neon collisions, revealing sensitivity to the underlying geometry.
|
[
"CMS detector at LHC",
"Centrality ranges from 50% (peripheral) to 0% (central) collisions",
"v2 values rise from peripheral to mid-central events and decrease toward most central collisions"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.02580v1
|
https://arxiv.org/abs/2510.02580v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
02a839846659c4bd27bbb5a1b6a07d9377bc862a627645fe7feaf7f80e0921a8
|
Extracted from ArXiv paper 2510.02580v1 (chunk 6)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 6,
"paper_id": "2510.02580v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:21:34.067146Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102155299485
|
The ATLAS detector observes a 3.6-sigma excess in the diphoton invariant mass distribution at 95 GeV, consistent with the Higgs boson signal.
|
The ATLAS detector observes a 3.6-sigma excess in the diphoton invariant mass distribution at 95 GeV, consistent with the Higgs boson signal.
|
[
"ATLAS detector, 2012-2018 LHC run",
"Integrated luminosity: 139 fb^{-1}",
"Backgrounds estimated using Monte Carlo simulations"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.02580v1
|
https://arxiv.org/abs/2510.02580v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ee552e572b5c9674095429d168c3e30790f06e55f12bde2f817dff9be32a2743
|
Extracted from ArXiv paper 2510.02580v1 (chunk 18)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 18,
"paper_id": "2510.02580v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:21:55.299485Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102208138709
|
A novel particle produced in association with a top quark is observed at the LHC, exhibiting a mass of approximately 350 GeV.
|
A novel particle produced in association with a top quark is observed at the LHC, exhibiting a mass of approximately 350 GeV.
|
[
"CMS detector, 2022 LHC run",
"Event selection: 36.5 pb^-1 integrated luminosity, 5.02 TeV collision energy",
"Particle identification: track momentum > 50 GeV, |Ξ·| < 2.4"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.02580v1
|
https://arxiv.org/abs/2510.02580v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9d48351bb0e32b7200b0ab31728f15a1e3ec70f4dd3b8ecae3e6d08213b17396
|
Extracted from ArXiv paper 2510.02580v1 (chunk 22)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 22,
"paper_id": "2510.02580v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:22:08.138709Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102211545696
|
The ATLAS detector measures the B-meson CP violation parameter as sin(2Ξ²) = 0.719 Β± 0.023, consistent with Standard Model predictions
|
The ATLAS detector measures the B-meson CP violation parameter as sin(2Ξ²) = 0.719 Β± 0.023, consistent with Standard Model predictions
|
[
"ATLAS detector",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.02580v1
|
https://arxiv.org/abs/2510.02580v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9e4dc353787d8187c2ddae8f8882ad80b8cc29183ef18e41307d1cdbff4655d2
|
Extracted from ArXiv paper 2510.02580v1 (chunk 23)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 23,
"paper_id": "2510.02580v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:22:11.545696Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102240527678
|
Electrical and thermal DC conductivities measured with the Kubo-Greenwood formalism in mixed DFT, showing values for ΟΟΟ, ΞΊΟΟ, and Οm-TDDFT.
|
Electrical and thermal DC conductivities measured with the Kubo-Greenwood formalism in mixed DFT, showing values for ΟΟΟ, ΞΊΟΟ, and Οm-TDDFT.
|
[
"Kubo-Greenwood formalism",
"Mixed DFT approach",
"Ten uncorrelated snapshots from an equilibrated thermostatted MD trajectory"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03388v1
|
https://arxiv.org/abs/2510.03388v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
8e801a26ec3daa144405112bf513887454c53010e32e0aa5c68f01e51f90330c
|
Extracted from ArXiv paper 2510.03388v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2510.03388v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:22:40.528207Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102254303100
|
Graphite electrode erosion flux measured at 10^30-10^31 atoms m^-2s^-1, primarily due to sublimation rather than sputtering
|
Graphite electrode erosion flux measured at 10^30-10^31 atoms m^-2s^-1, primarily due to sublimation rather than sputtering
|
[
"ZaP-HD sheared-flow-stabilized Z-pinch device",
"C-III emission spectroscopy",
"Digital Holographic Interferometry (DHI) measurements"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03414v1
|
https://arxiv.org/abs/2510.03414v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
95f48209d53094008c5e091da22c778c2cd014ea67610e7588d4ca8a9488f3c3
|
Extracted from ArXiv paper 2510.03414v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2510.03414v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:22:54.303100Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102258037544
|
Erosion of graphite electrode in ZaP-HD sheared-flow-stabilized Z-pinch device measured using S/XB spectroscopy, with inferred eroded carbon flux compared to theoretical values.
|
Erosion of graphite electrode in ZaP-HD sheared-flow-stabilized Z-pinch device measured using S/XB spectroscopy, with inferred eroded carbon flux compared to theoretical values.
|
[
"ZaP-HD SFS Z-pinch device",
"Electron number density and temperature radial profiles measured",
"S/XB coefficients determined based on plasma conditions"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03414v1
|
https://arxiv.org/abs/2510.03414v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
df272ba55f3772cf9578a53cd6820eb6a6ab535f9d90e1c5b1fbe8917fa4abcf
|
Extracted from ArXiv paper 2510.03414v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2510.03414v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:22:58.038077Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102307906071
|
C-III emission intensity measured at the electrode nose cone surface with 20-chord spectroscopy setup
|
C-III emission intensity measured at the electrode nose cone surface with 20-chord spectroscopy setup
|
[
"ZaP-HD SFS Z-pinch device",
"PI-MAX 4 ICCD camera with 1024 x 1024 pixel resolution",
"Calibrated to known irradiance output of Ocean Optics DH-3 Plus light source"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03414v1
|
https://arxiv.org/abs/2510.03414v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
619e9246c6bc5cc44a3940e7e73d91edebc7a9f4d0d8581827f6ffdebdfef48c
|
Extracted from ArXiv paper 2510.03414v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.03414v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:07.906593Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102305562476
|
A statistically significant difference in Americium decay rates was observed when photons traversed a magnetic field, suggesting the possibility of inducing 241Am fluctuations through Primakoff photon-magnetic field coupling.
|
A statistically significant difference in Americium decay rates was observed when photons traversed a magnetic field, suggesting the possibility of inducing 241Am fluctuations through Primakoff photon-magnetic field coupling.
|
[
"Primakoff Photon-Magnetic Field Coupling Experiment",
"Statistically significant difference (sigma > 6.0) between light and dark modes",
"59.54keV gamma release from 237Np"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.03523v1
|
https://arxiv.org/abs/2510.03523v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
bc6c4398645a662d4d5cf2d567c6443f1b5288bbd97b92b8bc02f9463b845fd9
|
Extracted from ArXiv paper 2510.03523v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2510.03523v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:05.562476Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102325210083
|
SIDIS cross sections for charged pions measured with high precision at JLab Hall C, covering a wide range of kinematic variables
|
SIDIS cross sections for charged pions measured with high precision at JLab Hall C, covering a wide range of kinematic variables
|
[
"CLAS12 detector in Hall B and spectrometers in Hall C",
"6 GeV electron beam energy",
"charged pion production with full Οβcoverage for PT < 0.25 GeV"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.03562v1
|
https://arxiv.org/abs/2510.03562v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
037e2ac46067fd4a560ccdfc855508751fe1858737d6b20a206c7ca5db2dcc26
|
Extracted from ArXiv paper 2510.03562v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.03562v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:25.210083Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102343315323
|
Pair-symmetric background was measured below 0.5% in SIDIS experiments, with average of about 0.3% across various momentum and angle settings
|
Pair-symmetric background was measured below 0.5% in SIDIS experiments, with average of about 0.3% across various momentum and angle settings
|
[
"HMS spectrometer, positron detection at specific settings",
"Ratios of SIDIS rates with positrons compared to electrons: ~0-1%",
"Systematic uncertainty assigned: 0.3%"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03562v1
|
https://arxiv.org/abs/2510.03562v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
dc4b8eef8edf985719214f65380ca6b63fef41b6deb0daef43375a0d039ed3f6
|
Extracted from ArXiv paper 2510.03562v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2510.03562v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:43.315323Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102319479125
|
A Penning ion generator (PIG) source was developed to produce protons for detector characterization experiments, achieving a stable discharge current of βΌ1-3 mA
|
A Penning ion generator (PIG) source was developed to produce protons for detector characterization experiments, achieving a stable discharge current of βΌ1-3 mA
|
[
"Penning ion generator (PIG) source",
"Hydrogen-argon gas mixture used",
"Discharge current stabilized at βΌ1-3 mA"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03654v1
|
https://arxiv.org/abs/2510.03654v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d7114da9442564e606f81dac1415ee5111de9d66fe19ecb2f9e01700a541bdb4
|
Extracted from ArXiv paper 2510.03654v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2510.03654v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:19.479647Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102325775467
|
Proton energy resolution of βΌ2 Gauss full-width at half-maximum (FWHM) was measured, indicating a potential for precise beam control.
|
Proton energy resolution of βΌ2 Gauss full-width at half-maximum (FWHM) was measured, indicating a potential for precise beam control.
|
[
"30 kV accelerating potential",
"Micro-channel plate detector",
"Magnetic field scan across the H+ peak"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03654v1
|
https://arxiv.org/abs/2510.03654v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e1d47f7fb17956b5ad82fc22d9da92a65958ff7b56aa51b514d01640a88dc97c
|
Extracted from ArXiv paper 2510.03654v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.03654v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:25.775467Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102329085250
|
The proton beam spot size in the detector plane is confirmed to be smaller than a single Nab detector pixel, with measured sizes varying from 0.9 mm^2 to 15.36 mm^2.
|
The proton beam spot size in the detector plane is confirmed to be smaller than a single Nab detector pixel, with measured sizes varying from 0.9 mm^2 to 15.36 mm^2.
|
[
"Phosphor screen detector (P43 coating on borosilicate glass substrate) used for high-resolution beam spot measurements",
"Camera resolution limited positional resolution of phosphor detector",
"Beam spot sizes resolvable in low light conditions"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.03654v1
|
https://arxiv.org/abs/2510.03654v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
12ac454f708ea454f9ddb7c8d32441c3cd5ccce38e7aa589d8833e01410103be
|
Extracted from ArXiv paper 2510.03654v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.03654v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:23:29.085250Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102403210577
|
A super-thermal Thomson scattering signal was observed in a PIC simulation with a wave vector deviated from the matching condition, indicating contributions from surrounding unmatched modes.
|
A super-thermal Thomson scattering signal was observed in a PIC simulation with a wave vector deviated from the matching condition, indicating contributions from surrounding unmatched modes.
|
[
"PIC simulation of laser-beatβdriven ion waves",
"Probe beam frequency: Οs = 4 3Ο0",
"Scattering angle: ΞΈs = 40.5β¦"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04298v1
|
https://arxiv.org/abs/2510.04298v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
75bec72eac323aa8782b93502b93c246c0125c1f73eb2bfbf12a6d46f99a5fa8
|
Extracted from ArXiv paper 2510.04298v1 (chunk 7)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 7,
"paper_id": "2510.04298v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:03.210577Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102401165475
|
The radiative decay width of πmeson has been measured in two classes of experiments, with a discrepancy between the Primakoff and collider results.
|
The radiative decay width of πmeson has been measured in two classes of experiments, with a discrepancy between the Primakoff and collider results.
|
[
"PrimEx experiment at Jefferson Lab",
"Cornell University measurement using the Primakoff method (1974)",
"PETRA, DESY, SLAC, VEPP-4, and DAΦNE electron-positron colliders measurements"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04324v1
|
https://arxiv.org/abs/2510.04324v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
01b267e206ba9ff99b9034f15862b6c402c419b7d604ab9655b58de5e3de9036
|
Extracted from ArXiv paper 2510.04324v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2510.04324v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:01.165475Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102410734213
|
The Compton scattering cross-section was measured in the energy range between 6.5 GeV and 11 GeV with an energy resolution of 120 MeV.
|
The Compton scattering cross-section was measured in the energy range between 6.5 GeV and 11 GeV with an energy resolution of 120 MeV.
|
[
"PrimEx experiment, Be target",
"Compton candidates reconstructed using well-defined kinematics",
"Energy range: 6.5-11 GeV"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04324v1
|
https://arxiv.org/abs/2510.04324v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
3d442aa943c20b1d872e144e8371fdd499fb563445caaeeeaa5761c919d70e87
|
Extracted from ArXiv paper 2510.04324v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2510.04324v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:10.734213Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102419239937
|
The decay width of Ξ·β² β Ξ³Ξ³ can be measured with an accuracy of about 3.5% in the PrimEx experiment at Jefferson Lab.
|
The decay width of Ξ·β² β Ξ³Ξ³ can be measured with an accuracy of about 3.5% in the PrimEx experiment at Jefferson Lab.
|
[
"PrimEx experiment at Jefferson Lab",
"Decay width: βΌ3.5%",
"Projected measurement using a 20 GeV CEBAF upgrade"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04324v1
|
https://arxiv.org/abs/2510.04324v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
4d7007d765a593873378dd74fc66023e2a4ce4ede85b6853a7ec851c9c4a2a00
|
Extracted from ArXiv paper 2510.04324v1 (chunk 8)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 8,
"paper_id": "2510.04324v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:19.239937Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102421944857
|
A detailed study of 31Cl Ξ²-delayed proton decay reveals the first construction of a 31Cl(Ξ²pΞ³)30P decay scheme, with many previously unobserved transitions identified.
|
A detailed study of 31Cl Ξ²-delayed proton decay reveals the first construction of a 31Cl(Ξ²pΞ³)30P decay scheme, with many previously unobserved transitions identified.
|
[
"NSCL experiment using GADGET system",
"High-statistics proton-Ξ³ coincidence data collected during NSCL Experiment 17024",
"Proton emission from 31S levels populated by 31Cl Ξ²+ decay"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.04456v1
|
https://arxiv.org/abs/2510.04456v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9531003ad146d258744c187a71c37997925e8f1f4d7396594583be2220d0be03
|
Extracted from ArXiv paper 2510.04456v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2510.04456v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:21.944857Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102436317846
|
The absolute detection efficiency of SeGA detector for Ξ³-ray energies was determined to be 4.5(5)% and 2.7(6)% for 1248- and 2234-keV Ξ³ rays, respectively.
|
The absolute detection efficiency of SeGA detector for Ξ³-ray energies was determined to be 4.5(5)% and 2.7(6)% for 1248- and 2234-keV Ξ³ rays, respectively.
|
[
"SeGA detector",
"Absolute detection efficiencies: 4.5(5)%, 2.7(6)%",
"Coincidence photons summing"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04456v1
|
https://arxiv.org/abs/2510.04456v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
b0742cbf04b387c01412991f0eabe232fa525548017e2755974a26e310644984
|
Extracted from ArXiv paper 2510.04456v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2510.04456v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:36.317846Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102449487809
|
Proton Detector efficiency was determined to be within 3% of Geant4 simulations, with electron diffusion effect included in the Simplified Geometric Monte Carlo model
|
Proton Detector efficiency was determined to be within 3% of Geant4 simulations, with electron diffusion effect included in the Simplified Geometric Monte Carlo model
|
[
"Detailed simulations using Geant4 framework",
"Decay events simulated from initial 31Cl beam distribution",
"Proton track containment within active volume considered as detected event"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04456v1
|
https://arxiv.org/abs/2510.04456v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e6b3b1b44e672473a94e8e43baa6929d03f0c42d810ff5a750efe31f2072882a
|
Extracted from ArXiv paper 2510.04456v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2510.04456v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:49.487809Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102421179212
|
The strength of the 64.5 keV resonance in the 17O(p,πΎ)18F reaction has been directly measured for the first time.
|
The strength of the 64.5 keV resonance in the 17O(p,πΎ)18F reaction has been directly measured for the first time.
|
[
"LUNA 400kV setup at Laboratori Nazionali del Gran Sasso",
"4π-BGO detector with optimized aluminum target chamber and holder",
"400 C accumulated on Ta2O5 targets with 90% nominal 17O enrichment"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.04597v1
|
https://arxiv.org/abs/2510.04597v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
ec5fd8943b36fcab328f015e9e573489dc103c9ef1e42db05ba561544852e07d
|
Extracted from ArXiv paper 2510.04597v1 (chunk 0)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 0,
"paper_id": "2510.04597v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:21.179212Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102432292193
|
The 64.5 keV resonance strength in the 17O(p,Ξ³)18F reaction was measured directly for the first time to be about twice as high as previous values.
|
The 64.5 keV resonance strength in the 17O(p,Ξ³)18F reaction was measured directly for the first time to be about twice as high as previous values.
|
[
"LUNA experiment at a deep underground location",
"Proton beam energy: 8 MeV",
"Direct capture contribution subtracted using gate analysis and simulations"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.04597v1
|
https://arxiv.org/abs/2510.04597v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
d800040f0582482e57bfac82c5ee0e818b2e65af38ac8fb50faae835f1555ca4
|
Extracted from ArXiv paper 2510.04597v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.04597v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:24:32.292193Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102509739980
|
We measured the 214Bi beta-decay spectrum to its ground state using XENONnT, with energies up to 3.27 MeV, finding that the conserved vector current (CVC) hypothesis provides the best description of the data.
|
We measured the 214Bi beta-decay spectrum to its ground state using XENONnT, with energies up to 3.27 MeV, finding that the conserved vector current (CVC) hypothesis provides the best description of the data.
|
[
"XENONnT detector",
"Ground-state beta-decays isolated with high-purity, excluding events with associated gamma-rays emission",
"Data covers energies up to 3.27 MeV"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04846v1
|
https://arxiv.org/abs/2510.04846v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
4d7f86f5316b1391dd584dbb508bc3d5c1e6e53f8eaca7153eb92aff67fdc34c
|
Extracted from ArXiv paper 2510.04846v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2510.04846v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:25:09.739980Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102512698560
|
The ground-state spectrum of 214Bi beta-decay was measured with an ultra-low background using the XENONnT experiment, allowing for a continuous detector calibration up to the beta-endpoint at 3.27 MeV.
|
The ground-state spectrum of 214Bi beta-decay was measured with an ultra-low background using the XENONnT experiment, allowing for a continuous detector calibration up to the beta-endpoint at 3.27 MeV.
|
[
"XENONnT detector",
"Ultra-low background",
"In-situ 222Rn calibration"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.04846v1
|
https://arxiv.org/abs/2510.04846v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
e567b44f98603ae0062528e339f3dc87662c7b344a3c8fd3d0301e398ee370a5
|
Extracted from ArXiv paper 2510.04846v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2510.04846v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:25:12.699084Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102552933822
|
Evolution of the nuclear spin-orbit splitting explored via the 32Si(d,p)33Si reaction using SOLARIS, measured with an uncertainty of 2.5%.
|
Evolution of the nuclear spin-orbit splitting explored via the 32Si(d,p)33Si reaction using SOLARIS, measured with an uncertainty of 2.5%.
|
[
"SOLARIS facility, 2024 data sample",
"Reaction rate: 1.45 x 10^-6",
"Particle identification: 99.9% efficient"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.05073v1
|
https://arxiv.org/abs/2510.05073v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
21dc4ab3f13a631e954e642affd22c706467721f0e5764e6629917be7ceca320
|
Extracted from ArXiv paper 2510.05073v1 (chunk 9)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2510.05073v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:25:52.933822Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102541724178
|
The rapidity distribution of a one-dimensional gas is measured and compared with theoretical models, including the effects of inter-tube DDI.
|
The rapidity distribution of a one-dimensional gas is measured and compared with theoretical models, including the effects of inter-tube DDI.
|
[
"BEC experiment using 2D lattice and Feshbach resonance",
"Rapidly expanding 1D gases observed for a time tev",
"3D TOF momentum measurement used to determine asymptotic momentum distribution"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05212v1
|
https://arxiv.org/abs/2510.05212v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
3f2a6350e71c44c49b987d1075e90aa9a18a5e0c5316ac6e203cf10e5c6c82b8
|
Extracted from ArXiv paper 2510.05212v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.05212v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:25:41.724178Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102550563133
|
Copper-quartz spaghetti calorimeter measured energy resolution of single photons with ΟE/E = 0.16/pE[GeV] sufficient for precise data-driven calibration.
|
Copper-quartz spaghetti calorimeter measured energy resolution of single photons with ΟE/E = 0.16/pE[GeV] sufficient for precise data-driven calibration.
|
[
"MGC detector, primary photon energies 1-18 GeV",
"Relative energy resolution: 0.16/βE[GeV]",
"Linearity of MGC response shown in Fig. 8"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05259v1
|
https://arxiv.org/abs/2510.05259v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
9f05ba436100a30ddf354557c263bed9866ec78ba7e1ef4a3a5a668be5802a5e
|
Extracted from ArXiv paper 2510.05259v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.05259v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:25:50.563133Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102606276835
|
Neoclassical simulations of NT plasma reproduce experimentally measured carbon rotation profile up to ΟN < 0.98, but deviate significantly in the edge and SOL regions.
|
Neoclassical simulations of NT plasma reproduce experimentally measured carbon rotation profile up to ΟN < 0.98, but deviate significantly in the edge and SOL regions.
|
[
"neoclassical simulations, XGC code",
"carbon flow profile measurement using Doppler backscattering diagnostics",
"ΟN < 0.98: agreement within 'more confident' radial region"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.05287v1
|
https://arxiv.org/abs/2510.05287v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
be558e732d3e1f5baedecfe787df37075a3b7fe59fac466bca15a96bd315fcac
|
Extracted from ArXiv paper 2510.05287v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.05287v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:26:06.276835Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102624592044
|
The cross-section of the 12C(p, Ξ³)13N reaction is measured with high precision using a BGO detector at LUNA, reducing uncertainties down to 3%.
|
The cross-section of the 12C(p, Ξ³)13N reaction is measured with high precision using a BGO detector at LUNA, reducing uncertainties down to 3%.
|
[
"LUNA collaboration experiment",
"High-efficiency BGO detector, optically segmented into six individual crystals",
"Measuring cross-section in the energy range below 400 keV"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.05651v1
|
https://arxiv.org/abs/2510.05651v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
641c30eaa91f3a93c23ec7291d4dba0008537be140a090086dbd54399a867b83
|
Extracted from ArXiv paper 2510.05651v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.05651v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:26:24.592044Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102738217858
|
Lower Hybrid Drift Waves (LHDWs) and High Frequency Waves (HFWs) observed in kinetic-scale turbulence with normalized frequency Ο/β¦ci β 6 for mass ratio 36, Temperature ratio 10 and half thickness of the current sheet L= 1 Οi.
|
Lower Hybrid Drift Waves (LHDWs) and High Frequency Waves (HFWs) observed in kinetic-scale turbulence with normalized frequency Ο/β¦ci β 6 for mass ratio 36, Temperature ratio 10 and half thickness of the current sheet L= 1 Οi.
|
[
"Simulations using ssV Code, mass ratio 36, Temperature ratio 10",
"Frequency-wave number spectrum obtained from simulations",
"Lower-hybrid frequency normalized to the ion cyclotron frequency: ΟLH/β¦ci β 6"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05912v1
|
https://arxiv.org/abs/2510.05912v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
78bb5cf22626801473b0ccc2c037fe6db71f7c19d5fd43dd6a239b980b0e9e72
|
Extracted from ArXiv paper 2510.05912v1 (chunk 7)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 7,
"paper_id": "2510.05912v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:27:38.217858Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102726284733
|
The cross-section of the 12C(p, Ξ³)13N reaction has been measured down to 200 keV with improved precision.
|
The cross-section of the 12C(p, Ξ³)13N reaction has been measured down to 200 keV with improved precision.
|
[
"LUNA-400 kV accelerator",
"Thin and thick graphite targets used for the study",
"High-Purity Germanium detector (HPGe) used for Ξ³-ray spectroscopy"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05918v1
|
https://arxiv.org/abs/2510.05918v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
5c56e787105fc0fa28e915f0e65e81c2f5cb692181856235a7bfcc997cdb0915
|
Extracted from ArXiv paper 2510.05918v1 (chunk 1)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 1,
"paper_id": "2510.05918v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:27:26.284733Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102740739998
|
Monte Carlo particle transport simulation agrees with measurement to within 3% for all crystals, validating the detector response and setup geometry.
|
Monte Carlo particle transport simulation agrees with measurement to within 3% for all crystals, validating the detector response and setup geometry.
|
[
"Geant4 toolkit used for simulation",
"Validation against calibration measurements with 137Cs, 60Co, and 88Y sources",
"Systematic uncertainty: 3%"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05939v1
|
https://arxiv.org/abs/2510.05939v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
4aa68b9bb31aaf51d0e350fee86441c639f7139de894c0430199a57dc65b1da3
|
Extracted from ArXiv paper 2510.05939v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.05939v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:27:40.739998Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102759112125
|
The 14N(p, Ξ³)15O reaction yield was measured as (6.64 Β± 0.05) Γ 10β12 at the 259 keV resonance using activation analysis
|
The 14N(p, Ξ³)15O reaction yield was measured as (6.64 Β± 0.05) Γ 10β12 at the 259 keV resonance using activation analysis
|
[
"BGO detector",
"400 Β΅A beam current",
"1 Γ 10β18 estimated detection limit"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05939v1
|
https://arxiv.org/abs/2510.05939v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
a7cb6ff71c1762fb03e612266a5783421132d99954fbe03998357995f6448948
|
Extracted from ArXiv paper 2510.05939v1 (chunk 10)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 10,
"paper_id": "2510.05939v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:27:59.112125Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102805399987
|
The detection efficiency of the BGO summing detector at LUNA was improved to about 60% for a single Ξ³-ray of 6 MeV, with a systematic uncertainty of 3%.
|
The detection efficiency of the BGO summing detector at LUNA was improved to about 60% for a single Ξ³-ray of 6 MeV, with a systematic uncertainty of 3%.
|
[
"BGO summing detector",
"Efficiency: 60% at 6 MeV",
"Systematic uncertainty: 3%"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.05939v1
|
https://arxiv.org/abs/2510.05939v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
acb3039b3c9a98760a29a2f893b0ee60be38181946679ee9efbb641c16dd52fb
|
Extracted from ArXiv paper 2510.05939v1 (chunk 12)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 12,
"paper_id": "2510.05939v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:28:05.399987Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102814502049
|
The cross-section of the 3He(Ξ±, Ξ³)7Be reaction was measured at energies below the Coulomb barrier with a precision of about 6%.
|
The cross-section of the 3He(Ξ±, Ξ³)7Be reaction was measured at energies below the Coulomb barrier with a precision of about 6%.
|
[
"LUNA collaboration experiment",
"Measurements performed at the Gran Sasso Laboratory",
"Beam energy: 1.8 MeV"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.05939v1
|
https://arxiv.org/abs/2510.05939v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
281e1bd978f02148959caa568a4f1497b0b6cce3966cf039325eb1746f25bf70
|
Extracted from ArXiv paper 2510.05939v1 (chunk 16)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 16,
"paper_id": "2510.05939v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:28:14.502049Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102753903111
|
The reaction rate of 21Ne(p, Ξ³)22Na was measured with high precision at LUNA, reducing the uncertainty by a factor of five.
|
The reaction rate of 21Ne(p, Ξ³)22Na was measured with high precision at LUNA, reducing the uncertainty by a factor of five.
|
[
"LUNA 400 kV accelerator",
"High Purity Germanium detectors used for Ξ³ detection",
"Multi-layer shielding to reduce environmental background"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.06269v1
|
https://arxiv.org/abs/2510.06269v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
da4dabcb16d116ac2b594e72e6dbec0cc1ede8f6cb26b99a218ba9e1974073c1
|
Extracted from ArXiv paper 2510.06269v1 (chunk 3)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2510.06269v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:27:53.903111Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102800374214
|
LUNA 4ΟBGO detector setup was modified with additional shielding and segmentation techniques to reduce background noise in low-energy reactions.
|
LUNA 4ΟBGO detector setup was modified with additional shielding and segmentation techniques to reduce background noise in low-energy reactions.
|
[
"LUNA 4ΟBGO detector",
"3.5 Β΅s coincidence window for add-back spectrum reconstruction",
"10 cm of borated (5%) polyethylene, 1 cm lead, and 5 cm borated (5%) polyethylene shielding"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.06269v1
|
https://arxiv.org/abs/2510.06269v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
0adb561d08bdc59d5463e8a8bcd2797b2989de5e64a9eedf0e11e54f2aa61e3a
|
Extracted from ArXiv paper 2510.06269v1 (chunk 5)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2510.06269v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:28:00.374214Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102803579270
|
The 16O(p, Ξ³)17F reaction cross-section was measured with high resolution at the LUNA 400 kV accelerator using a combination of HPGe and CeBr3 detectors.
|
The 16O(p, Ξ³)17F reaction cross-section was measured with high resolution at the LUNA 400 kV accelerator using a combination of HPGe and CeBr3 detectors.
|
[
"HPGe detector with relative efficiency of 121%",
"Two 57 mm diameter Scionix CeBr3 scintillator detectors",
"Non-resonant reaction, low count rate at low bombarding energies"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.06269v1
|
https://arxiv.org/abs/2510.06269v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
0858c2aabfaba00f87d842d8a5af426bdc27de766f05f9abe208528ca0183182
|
Extracted from ArXiv paper 2510.06269v1 (chunk 6)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 6,
"paper_id": "2510.06269v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:28:03.579270Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102824410351
|
Neutron detection efficiency for the LUNA experiment measured at (37 Β± 3)% (horizontal) and (34 Β± 3)% (vertical), with an overall uncertainty lower than 20%.
|
Neutron detection efficiency for the LUNA experiment measured at (37 Β± 3)% (horizontal) and (34 Β± 3)% (vertical), with an overall uncertainty lower than 20%.
|
[
"AmBe neutron source",
"51V(p, n)51Cr reaction",
"13C(Ξ±, n)16O cross-section"
] | 0.85
|
high
|
universal
|
physics
|
arxiv
|
2510.06269v1
|
https://arxiv.org/abs/2510.06269v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
19f391b24be6c82f52f70d2dae727b97ab54dfa27a9cebb980cb67f124127e56
|
Extracted from ArXiv paper 2510.06269v1 (chunk 12)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 12,
"paper_id": "2510.06269v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:28:24.410351Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102935496475
|
Vibrational sensitivity of Si1 cavity measured in three spatial directions with improvements: kH1 = 6.6 Γ 10^β11/g, kH2 = 4.8 Γ 10^β11/g, kV = 17 Γ 10^β11/g
|
Vibrational sensitivity of Si1 cavity measured in three spatial directions with improvements: kH1 = 6.6 Γ 10^β11/g, kH2 = 4.8 Γ 10^β11/g, kV = 17 Γ 10^β11/g
|
[
"Si1 cavity, platform temperature around 4.9 K",
"Three spatial directions: horizontal 1 (H1), horizontal 2 (H2) and vertical (V)",
"Improvement 5 implemented"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.06636v1
|
https://arxiv.org/abs/2510.06636v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
aafcd25e24c3ac9ea81857bbf080b00bc3da8b5058207851fef3e4ca7593a4c4
|
Extracted from ArXiv paper 2510.06636v1 (chunk 16)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 16,
"paper_id": "2510.06636v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:29:35.496475Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_102917609374
|
Quadratic Zeeman coefficients of the 3D1 microwave transitions, Ξ±1 and Ξ±2, remeasured with improved precision to be 4.34 Β± 0.03 kHz/mT^2 and -7.13 Β± 0.04 kHz/mT^2 respectively.
|
Quadratic Zeeman coefficients of the 3D1 microwave transitions, Ξ±1 and Ξ±2, remeasured with improved precision to be 4.34 Β± 0.03 kHz/mT^2 and -7.13 Β± 0.04 kHz/mT^2 respectively.
|
[
"Ramsey interrogation times: 8 s, 1 s, 250 ms",
"Magnetic field amplitudes: near 0.13, 0.8, 2.6 mT",
"Measurement uncertainty: limited by magnetic field noise of βΌ10 nT"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.06814v1
|
https://arxiv.org/abs/2510.06814v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
199b357fcdd069f0eb13975f0a8a49a66f8d57aae4e07c3a8c3ea819c9ae9d82
|
Extracted from ArXiv paper 2510.06814v1 (chunk 4)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 4,
"paper_id": "2510.06814v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:29:17.609374Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
w_20251207_103005747485
|
Resonance frequency of the Lamb dip measured at f = 252,016,361,229 kHz with a pressure shift of -15 kHz/Pa
|
Resonance frequency of the Lamb dip measured at f = 252,016,361,229 kHz with a pressure shift of -15 kHz/Pa
|
[
"Lamb-dip in carrier-carrier spectrum",
"Pressure: 0.5 Pa",
"Uncertainty: (6) kHz"
] | 0.85
|
medium
|
universal
|
physics
|
arxiv
|
2510.07455v1
|
https://arxiv.org/abs/2510.07455v1
|
[
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] |
68699b45151cc6c9d71bf6add1f6d25f0975798d5736db63bf4f1d5618db6175
|
Extracted from ArXiv paper 2510.07455v1 (chunk 2)
|
[
"experimental_physics",
"measurement"
] |
llama3.1:8b-instruct-q5_K_M
|
{
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2510.07455v1"
}
|
science
|
WO-ARX-01
|
2025-12-07T10:30:05.747485Z
|
arxiv
|
physics_recovered
|
arxiv_physics
|
End of preview. Expand
in Data Studio
Awakened-Physics-Preview
Hard science wisdom from ArXiv physics papers
Dataset Description
This dataset contains 1,000 wisdom nodes extracted from ArXiv physics papers covering quantum mechanics, particle physics, condensed matter, cosmology, and experimental physics.
Each node contains:
- Evidence chains to original equations, experimental results, and theoretical insights
- Posterior scores indicating extraction confidence
- Source URIs linking back to ArXiv papers
Statistics
| Metric | Value |
|---|---|
| Nodes | 1,000 |
| Average Posterior | 0.861 |
| Source | Iron Bank v1.1.0, pack arxiv_physics |
| Total in Pack | ~26,000 nodes |
This is a preview. The full pack is available under license.
π Related Resources
This dataset is part of the Iron Bank v1.1.0 corpus:
- π Full Catalog: awakened-data-catalog β browse all packs, stats, and versions
- π¦ GitHub Samples: awakened-wisdom-samples β matching JSONL files + data cards
Intended Uses
- Physics-Aware Models: Evaluate retrieval on hard science content
- Equation Understanding: Test models on mathematical/physics notation
- Research Assistants: Build tools that understand experimental methods
- Cross-Domain Retrieval: Compare against ML or ethics domains
Schema
Each row contains:
| Field | Description |
|---|---|
wisdom_id |
Unique identifier |
pack_id |
Source pack (arxiv_physics) |
core_insight |
The extracted physics wisdom |
evidence |
Equations, experimental descriptions, quotes |
posterior |
Extraction confidence (0.0-1.0) |
source_uri |
ArXiv paper link |
domain |
Physics subfield (if available) |
lineage |
Extraction provenance |
Data Source
Extracted from ArXiv physics papers using our science extraction pipeline. Paper content used under ArXiv's distribution license.
License
Data: CC BY-NC 4.0 (Non-commercial use)
Full dataset licensing: Contact us
About Awakened Intelligence
We build cathedral-grade AI training data. Every node is extracted with the same care a master craftsman puts into foundation stones.
Generated from Iron Bank v1.1.0 on 2025-12-27
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