AwakenedIntelligence/Awakened-Physics-Preview

w_20251207_133224207605

The pion and kaon structure functions have systematic uncertainties estimated to be around 2% and 5%, respectively, due to detector acceptance effects, proton structure function, and background processes.

[ "EicC experiment", "Detector-resolution uncertainty: 2%", "Background process uncertainty: approximately 10%" ]

0.85

medium

universal

physics

arxiv

2512.01720v1

https://arxiv.org/abs/2512.01720v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

a554bf9a24054d6efd439e6ca6a8065302e2b969e6a006505d63361fdde3064b

Extracted from ArXiv paper 2512.01720v1 (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": "2512.01720v1" }

science

WO-ARX-01

2025-12-07T13:32:24.207605Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133221330523

Unscattered cross-section events contribute more than 75% of the full 1p1π−cross section around the Delta peak after applying cuts in missing energy and momentum.

[ "MAMI spectrometers, with acceptance from [29]", "Events with Em < 70 MeV and pm < 350 MeV selected", "Final electron energy chosen to be close to the Delta-resonance peak" ]

0.85

medium

universal

physics

arxiv

2512.01721v1

https://arxiv.org/abs/2512.01721v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

44066e0d582c4349314da04867c1eaad770218920a98fe97f509a1bc3882db66

Extracted from ArXiv paper 2512.01721v1 (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": "2512.01721v1" }

science

WO-ARX-01

2025-12-07T13:32:21.330523Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133234997150

The triple-coincidence interaction cross-section is measured for the reaction pπ− with a liquid argon target, achieving high statistics.

[ "Liquid argon target", "Triple-coincidence experiment with CLAS detector", "Kinematic conditions: Ei = 1159 MeV, θl = (30 ± 15) deg, kl < 400 MeV" ]

0.85

medium

universal

physics

arxiv

2512.01721v1

https://arxiv.org/abs/2512.01721v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d613d70689d58ff6281ef053028e3c074cc50bd72819bbe20114f5b5586928af

Extracted from ArXiv paper 2512.01721v1 (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": "2512.01721v1" }

science

WO-ARX-01

2025-12-07T13:32:34.997150Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133251185925

Pronounced nonthermal ion velocity distribution function modifications, including parallel heating and secondary ion beam formation, are observed in ultra-low-beta plasmas due to parametric decay instability.

[ "Hybrid particle-in-cell simulations", "Ultra-low-beta plasma conditions characteristic of the Earth's ionosphere", "Triggered PDI with a dispersive mother wave comparable to the ion inertial length" ]

0.85

high

universal

physics

arxiv

2512.01757v1

https://arxiv.org/abs/2512.01757v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

2c60439ed5bdc05072d6862c3268252ac309ae99f7cf5179c0c0f6bf49ec2df5

Extracted from ArXiv paper 2512.01757v1 (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": "2512.01757v1" }

science

WO-ARX-01

2025-12-07T13:32:51.185925Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133325709755

VDF modifications observed in runs F, G, and H, with varying magnitude of perpendicular magnetic field fluctuations.

[ "Runs F-G-H: simulations of Alfvén waves with modulated wave-packet", "kmin = 1.96 d−1 to kmax = 2.17 d−1, wmin = 19 to wmax = 21", "Left-handed and right-handed polarized spectra studied" ]

0.85

medium

universal

physics

arxiv

2512.01757v1

https://arxiv.org/abs/2512.01757v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

c50cd6a4e27d3badc1840a15f30760310fbeea92985e356b82c4fe5eda85cadf

Extracted from ArXiv paper 2512.01757v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.01757v1" }

science

WO-ARX-01

2025-12-07T13:33:25.709755Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133321989590

The ratio of the production cross-sections of χ_(c2) and χ_c1 mesons is measured in the 4-muon channel at LHCb.

[ "LHCb detector, Run 3 data", "Integrated luminosity: 5.1 fb^(-1)", "Muon momentum: 6-100 GeV" ]

0.85

medium

universal

physics

arxiv

2512.01780v1

https://arxiv.org/abs/2512.01780v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

510718b7df08d7b9f18479d2e0692d31134b0866ca94d6b103faf7e7c094f789

Extracted from ArXiv paper 2512.01780v1 (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": "2512.01780v1" }

science

WO-ARX-01

2025-12-07T13:33:21.989590Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133330657423

The ratio of beam-spin asymmetry to cross-section was measured in Deep Exclusive Meson Production reactions, with the Regge models better predicting this value.

[ "KaonLT experiment at Jefferson Lab Hall C", "Q2-dependent measurements from 2 < Q2 < 6 GeV^2", "Comparison with generalized parton distribution and Regge formalism" ]

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" ]

10f96045534b8732fd2a626696734ea6663ed1d7fe43aeae94fd8a6e095708ec

Extracted from ArXiv paper 2512.01928v1 (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": "2512.01928v1" }

science

WO-ARX-01

2025-12-07T13:33:30.657423Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133337306646

The ALU (Asymmetry of Longitudinal Uptake) was measured for the first time in p(⃗e, e′π+)n reactions at Jefferson Lab Hall C, with a result of 0.91 ± 0.03.

[ "KaonLT experiment in Hall C", "90 days of data taken with 10.585 GeV electron beam and 40 days used for analysis", "Beam helicity flipped at 30 Hz, with 89% longitudinal polarization" ]

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" ]

0b2de5f27a50d0c8752eaef4bacd2c37a750de4a63512778270ce87486c2aeb6

Extracted from ArXiv paper 2512.01928v1 (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": "2512.01928v1" }

science

WO-ARX-01

2025-12-07T13:33:37.306646Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133359899952

Pion electroproduction cross sections and charged pion form factor measured up to high Q^2 values, revealing scaling behavior

[ "CLAS detector, Jefferson Lab experiments E12-19-006 and others", "Multiple data points at Q^2 = [2.1, 3.0, 4.4, 5.5] GeV^2, x_B = [0.21, 0.25, 0.40]", "Cross-sections measured with systematic uncertainty of up to 10%" ]

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" ]

2d04629ac250149514094883c4d47a2b9269df744b5cc81cda8eaa593d3c24e0

Extracted from ArXiv paper 2512.01928v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.01928v1" }

science

WO-ARX-01

2025-12-07T13:33:59.899952Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133453692167

An extreme, short-lived optical flare in an elliptical galaxy was observed with luminosity and duration suggesting it may have originated from the tidal disruption of a star by an intermediate-mass black hole.

[ "AT2022zod transient event", "Elliptical galaxy at z = 0.11", "Galaxy centre SMBH mass: ∼108 M⊙" ]

0.85

medium

universal

physics

arxiv

2512.02136v1

https://arxiv.org/abs/2512.02136v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

1c2e2671894be3bb2793c36ce5c70ba35d8a19beda89be08464f0e504636eca3

Extracted from ArXiv paper 2512.02136v1 (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": "2512.02136v1" }

science

WO-ARX-01

2025-12-07T13:34:53.694132Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133603134080

The muon magnetic anomaly is measured to be aµ = 116 591 810(43) × 10−11, showing tension with the Standard Model prediction.

[ "Bunched beam experiment at Fermilab", "Muon decay measurements", "Theoretical SM value: 116 591 810(43) × 10−11" ]

0.85

high

universal

physics

arxiv

2512.02209v1

https://arxiv.org/abs/2512.02209v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

6f5b74dd6ae1c8864cbfb2224c5f6a2f4185c2ad34aa09d695d2d30f706b2320

Extracted from ArXiv paper 2512.02209v1 (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": "2512.02209v1" }

science

WO-ARX-01

2025-12-07T13:36:03.134080Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133647218240

Proton fusion cross-section measured for 20O(p,n) and 19O(p,n) reactions, with excitation functions showing broad peaks indicative of short-lived states.

[ "MuSIC@Indiana active target detector, CH4 gas, incident radioactive beams of 20O and 19O ions", "Cross-section measured over energy intervals 1.0 ≤Ecm ≤2.05 MeV (20O) and 1.48 ≤Ecm ≤1.94 MeV (19O)", "Statistical uncertainty associated with NER, systematic uncertainty of 5% for mis-identification of fusion events" ]

0.85

high

universal

physics

arxiv

2512.02277v1

https://arxiv.org/abs/2512.02277v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

3af0fbde66f9c57144bf84d3015907d161994ed7609576fb9ea7bc5a7beea5b6

Extracted from ArXiv paper 2512.02277v1 (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": "2512.02277v1" }

science

WO-ARX-01

2025-12-07T13:36:47.218240Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133640195376

LIGO/Virgo/KAGRA collaboration reports the detection of two binary neutron star systems, GW170817 and GW190425, with masses significantly different from those observed in the Milky Way.

[ "LIGO/Virgo/KAGRA detectors", "GW170817: total mass 2.66 ± 0.12 M⊙", "GW190425: total mass 3.4+0.03−0.01 M⊙" ]

0.85

high

universal

physics

arxiv

2512.02296v1

https://arxiv.org/abs/2512.02296v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

bda68f5c8e3bf818dc8c1d899be01807274cee7cb44e2e330fe9500d44f73c7e

Extracted from ArXiv paper 2512.02296v1 (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": "2512.02296v1" }

science

WO-ARX-01

2025-12-07T13:36:40.195376Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133700619255

HPGe detectors with p-type point-contact configuration achieve sub-keV energy thresholds, ultra-low impurity concentrations, and excellent pulse-shape discrimination.

[ "High-purity germanium (HPGe) detectors", "Capacitance of only 1–2 pF at full depletion", "Ultra-low impurity concentration: ∼10^8 atoms/cm^3" ]

0.85

high

universal

physics

arxiv

2512.02317v1

https://arxiv.org/abs/2512.02317v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

5ecb07998459948d7f8358200f715256301e66fe22f5993559db05655e63b639

Extracted from ArXiv paper 2512.02317v1 (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": "2512.02317v1" }

science

WO-ARX-01

2025-12-07T13:37:00.619255Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133713690469

Direct detection experiments measure the nuclear recoil spectrum expected from WIMP interactions, with cryogenic detectors particularly competitive in the low-mass regime.

[ "Cryogenic detectors (Al2O3 and LiAlO2 targets)", "Excellent energy resolution (O(10 eV) thresholds)", "World-leading sensitivity to sub-GeV WIMPs" ]

0.85

medium

universal

physics

arxiv

2512.02317v1

https://arxiv.org/abs/2512.02317v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

92d74607d3d8cef75b676a44770ce6398ed066484295428931e3e69ffc8206d3

Extracted from ArXiv paper 2512.02317v1 (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": "2512.02317v1" }

science

WO-ARX-01

2025-12-07T13:37:13.690469Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133815455016

Applied magnetic fields can facilitate volumetric heating in underdense plasma via direct laser acceleration, with the strongest acceleration observed when the magnetic field affects acceleration in a single half-cycle.

[ "Section IV of the paper", "Electrons need to be preheated prior to the laser pulse", "Low (but still relativistic) laser intensity is most efficient" ]

0.85

medium

universal

physics

arxiv

2512.02426v1

https://arxiv.org/abs/2512.02426v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

036930ee4b0e6a9eceb18c8af18fb1f61f008aa79a620fe1746444d04b9ec30f

Extracted from ArXiv paper 2512.02426v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.02426v1" }

science

WO-ARX-01

2025-12-07T13:38:15.455016Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133900998632

Intermolecular coupling strength strongly influences polarization dependence of harmonic yield, with flipping of yield-maximizing polarization angle observed for higher harmonic orders at weaker couplings.

[ "Four-level scheme analysis", "Laser pulse polarized parallel to molecular axes", "Harmonic intensities calculated as function of intermolecular coupling strength" ]

0.85

medium

universal

physics

arxiv

2512.02623v1

https://arxiv.org/abs/2512.02623v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

cc2b48532825e81b74274c943eedda76afe643228e1bb6b3214ba687155e06c5

Extracted from ArXiv paper 2512.02623v1 (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": "2512.02623v1" }

science

WO-ARX-01

2025-12-07T13:39:00.999166Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133919983942

The best fit value for the BBH merger rate parameter f_Y is found to be 0.55 with a χ^2 distribution, indicating a reasonable fit to the observed BBH merger rate at 1σ level.

[ "χ^2 test of mergers today's rate with SFRD and SMD from Eq. 2.1", "Observed BBH merger rate in observer reference frame (Eq. 5.2)", "30 linearly-spaced redshift bins" ]

0.85

high

universal

physics

arxiv

2512.02642v1

https://arxiv.org/abs/2512.02642v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

45007a14919b7eafd9b30b14ff4c300b552ebe05d257a192bbf2d08bdc986b20

Extracted from ArXiv paper 2512.02642v1 (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": "2512.02642v1" }

science

WO-ARX-01

2025-12-07T13:39:19.983942Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133923605479

Observed average stellar mass of FRB host galaxies is about 10^10 M⊙, with a normally distributed probability distribution in log M∗.

[ "Sample of 53 FRBs from Table 2", "Average stellar mass: 10^10 M⊙", "Standard deviation in log M∗: 0.6" ]

0.85

medium

universal

physics

arxiv

2512.02642v1

https://arxiv.org/abs/2512.02642v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

727d1030157c287e63fae158b7beed5ac677f17eefa386cb471e97ec6705103d

Extracted from ArXiv paper 2512.02642v1 (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": "2512.02642v1" }

science

WO-ARX-01

2025-12-07T13:39:23.605479Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133959269397

Fundamental quasinormal mode frequencies Mω in the electric sector (Qm = 0) measured for various values of β and Qe

[ "Table I, dimensionless frequencies for ℓ=2, M=1", "Chebyshev–Lobatto grids with N ∈{80, 100} and N ∈{120, 150}", "AdS boundary conditions" ]

0.85

medium

universal

physics

arxiv

2512.02714v1

https://arxiv.org/abs/2512.02714v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

1cb0a98cbbdc1868994ce04f4d1471847928f7c64cfe73c896ea69b74cb47aee

Extracted from ArXiv paper 2512.02714v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.02714v1" }

science

WO-ARX-01

2025-12-07T13:39:59.269397Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133941654294

Non-Hermitian many-body effects and PT-symmetric physics were observed in Rydberg atoms with a negligible interaction strength of about 2π × 5 kHz, separated by approximately 114 µm.

[ "Rydberg dressing and MW driving experiments", "Interaction strength: 2π × 5 kHz", "Atomic separation: 114 µm" ]

0.85

medium

universal

physics

arxiv

2512.02753v1

https://arxiv.org/abs/2512.02753v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

52bb9fbc686d2bd93ac46fef44ae7e7b96e36e8fbb9c4e76c607d6d7ca019bd7

Extracted from ArXiv paper 2512.02753v1 (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": "2512.02753v1" }

science

WO-ARX-01

2025-12-07T13:39:41.654294Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134010000124

Spin-exchange interaction strength between Rydberg atoms measured to be 2π × 5.75(4) MHz with a 1/e decay time of τ = 0.59(3) µs

[ "Rydberg atom experiment, arbitrary units", "Interaction strength: 2π × 5.75(4) MHz", "Decay time: 0.59(3) µs" ]

0.85

medium

universal

physics

arxiv

2512.02753v1

https://arxiv.org/abs/2512.02753v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

2b3c14c92f9562a2a8ad44d2b982a11139c05f0ce226fbd618f2ea7fb2f064bc

Extracted from ArXiv paper 2512.02753v1 (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": "2512.02753v1" }

science

WO-ARX-01

2025-12-07T13:40:10.000124Z

arxiv

physics_recovered

arxiv_physics

w_20251207_133945732532

Relative sensitivity of peak wavelength shift per degree measured as 0.02-0.023 % K-1 from ambient temperature to 160°C

[ "Measurement using Varshni equation", "Peak wavelength shift monitored with Raman spectroscopy", "Analysis of UPL mechanism and phonon mode energies" ]

0.85

medium

universal

physics

arxiv

2512.02754v1

https://arxiv.org/abs/2512.02754v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d7e11581b2259bb686ca62765e84c5b7045ce5e695518e089cfc3a5179946de7

Extracted from ArXiv paper 2512.02754v1 (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": "2512.02754v1" }

science

WO-ARX-01

2025-12-07T13:39:45.732532Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134035043459

Observed spectral changes in FSRQs may be due to varying energy density of BLR and IR photon fields, affecting MeV-GeV emission

[ "MAGIC Collaboration et al. (2018), KN disfavors IC-BLR for VHE", "IC-IR (or strong field with energy ≲IR) is relevant scenario for FSRQs", "Spectral parameters from Roy et al. (2021) used in SED modeling" ]

0.85

medium

universal

physics

arxiv

2512.02839v1

https://arxiv.org/abs/2512.02839v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

c77eeeccaf4f90a3ac992551ec7e578a0af2c4fcb2dd9846d346b838c397bf6b

Extracted from ArXiv paper 2512.02839v1 (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": "2512.02839v1" }

science

WO-ARX-01

2025-12-07T13:40:35.043995Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134107556601

A clear positive correlation is observed between injected current and longitudinal broadening, with higher currents leading to increased beam size.

[ "FIBRE experiment at FAST/IOTA", "RMS bunch length analysis from Fig. 12", "Observation of non-Gaussian features in longitudinal distribution" ]

0.85

high

universal

physics

arxiv

2512.03002v1

https://arxiv.org/abs/2512.03002v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

a6157c18252a1a893bfa84a10a78c11483f80ba59f5e96fbc9c67cc91941714c

Extracted from ArXiv paper 2512.03002v1 (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": "2512.03002v1" }

science

WO-ARX-01

2025-12-07T13:41:07.556601Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134109009877

The Rabi frequency for the transition between ground and first excited states in 23Na40K molecules was measured to be 71.1(3) MHz, with a RMS field strength of 6.9 kV/m.

[ "rectangular waveguide antenna", "100 W of power applied to each feed (amplifier output saturated)", "RMS field strength: 6.9 kV/m" ]

0.85

medium

universal

physics

arxiv

2512.03007v1

https://arxiv.org/abs/2512.03007v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

c4663ba3d23399e54550187cb14472256d4a831b0e793908c6e1a78a42123831

Extracted from ArXiv paper 2512.03007v1 (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": "2512.03007v1" }

science

WO-ARX-01

2025-12-07T13:41:09.009877Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134154631046

Production cross section for spin-0 mediators coupled to top quarks constrained by various LHC searches, with strongest limits from invisible decays and diphoton resonances.

[ "ATLAS data", "13 TeV LHC collisions", " Invisible decay channel and diphoton resonance search" ]

0.85

high

universal

physics

arxiv

2512.03133v1

https://arxiv.org/abs/2512.03133v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

25628f6bbded3dcaf2751f9d503edae5d51053c32e2084a44e6b8393e97c6c68

Extracted from ArXiv paper 2512.03133v1 (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": "2512.03133v1" }

science

WO-ARX-01

2025-12-07T13:41:54.631046Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134201973053

GRB 230204B's afterglow light curve and spectrum were observed with ZTF, VLT/X-shooter, and Fermi GBM, revealing a redshift of z = 2.142

[ "ZTF Fritz marshal, GROWTH collaboration", "VLT/X-shooter observations, redshift measurement", "Fermi GBM data, prompt emission analysis" ]

0.85

medium

universal

physics

arxiv

2512.03136v1

https://arxiv.org/abs/2512.03136v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

49fc93dbfe7571c09eebf3fbf953900e937077c950bb3a16d5430c6d24197480

Extracted from ArXiv paper 2512.03136v1 (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": "2512.03136v1" }

science

WO-ARX-01

2025-12-07T13:42:01.973053Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134256464964

The statistical model cross section for nuclear reactions is formulated using transmission coefficients and level densities in the compound nucleus and various nuclides.

[ "Equation (5)", "Nuclear properties entering the calculation of transmission coefficients", "Level density in the compound nucleus" ]

0.85

medium

universal

physics

arxiv

2512.03206v1

https://arxiv.org/abs/2512.03206v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

f0e82312a1edc79ca5809846556cd300178e68c7c976010b472c56e714a6e9ad

Extracted from ArXiv paper 2512.03206v1 (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": "2512.03206v1" }

science

WO-ARX-01

2025-12-07T13:42:56.464964Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134331925770

First proton-induced cross sections measured on a stored rare ion beam for explosive nucleosynthesis, specifically Te118(p,γ) reaction.

[ "Phys. Rev. Lett. 134(14), 142701 (2025)", "Stored rare ion beam: Te118", "Proton-induced cross-section measurement" ]

0.85

high

universal

physics

arxiv

2512.03206v1

https://arxiv.org/abs/2512.03206v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

7bc98a4a550f042be323414ede34a611faf5b627c6533df552b68a97c9dcce2b

Extracted from ArXiv paper 2512.03206v1 (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": "2512.03206v1" }

science

WO-ARX-01

2025-12-07T13:43:31.925770Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134313501412

Recent high-precision measurements by ATLAS and CMS reveal a robust enhancement in top-antitop production cross section near threshold, compatible with Standard Model predictions or additional contributions from pseudoscalar interactions.

[ "ATLAS and CMS collaborations", "LHC data samples", "Invariant mass of top-antitop pair approaches twice the top quark mass" ]

0.85

high

universal

physics

arxiv

2512.03220v1

https://arxiv.org/abs/2512.03220v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

f46fcb9b21753efba82962049f6bc1e45581788a63650447c3dd6b33d40e3617

Extracted from ArXiv paper 2512.03220v1 (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": "2512.03220v1" }

science

WO-ARX-01

2025-12-07T13:43:13.501412Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134347079266

The nearest source of low-energy cosmic-ray particles observed near the Solar system is constrained to be within 150-200 parsecs distant.

[ "Voyager 1 data taken in the local ISM", "GALPROP code used for modelling", "3D reconstructions of dust and gas" ]

0.85

high

universal

physics

arxiv

2512.03385v1

https://arxiv.org/abs/2512.03385v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

ae8b7e12d761d36a4e7d32e3cf5f8a27bef8a2b00175ea851897028fb50371df

Extracted from ArXiv paper 2512.03385v1 (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": "2512.03385v1" }

science

WO-ARX-01

2025-12-07T13:43:47.079266Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134415072952

Magnetic field amplification to several giga-gauss with a lifetime around hundreds of femtoseconds is observed in ultra-intense short laser pulses interacting with microtube plasmas.

[ "Particle-in-cell simulations by kinetic methods", "Peak intensity of 1021 W/cm2, pulse duration 100 fs, and wavelength 0.8 µm", "Seed magnetic field ranging from 10–60 MG" ]

0.85

high

universal

physics

arxiv

2512.03388v1

https://arxiv.org/abs/2512.03388v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d5463b0e0b11092471d266a94879835a446c84a122916e5a4c765edb4086da5a

Extracted from ArXiv paper 2512.03388v1 (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": "2512.03388v1" }

science

WO-ARX-01

2025-12-07T13:44:15.072952Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134436157459

The process γp →π0p →e+e−γp was measured at the Mainz Microtron, with energies of incident photons analyzed up to 750 MeV.

[ "Mainz Microtron (MAMI) facility", "energy-tagged bremsstrahlung photon beam", "incident photon energies: 0-750 MeV" ]

0.85

medium

universal

physics

arxiv

2512.03431v1

https://arxiv.org/abs/2512.03431v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

de85bd878b3ca696d25473619719ecd8161a8b1d4d2f31792f6c737e301d772a

Extracted from ArXiv paper 2512.03431v1 (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": "2512.03431v1" }

science

WO-ARX-01

2025-12-07T13:44:36.157459Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134458170520

The slope parameter aπ = 0.0315 ± 0.0026 was measured, with its uncertainty being close to 8%, using a fit to experimental data points from the present work.

[ "ATLAS detector, 2023 data sample", "362 million B-meson pairs analyzed", "Systematic uncertainty: 0.008" ]

0.85

high

universal

physics

arxiv

2512.03431v1

https://arxiv.org/abs/2512.03431v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

1f440a7ebc8b89b9cd830ea80f7a16f784cc5ab03b76aeda2aa0ad6691282d9c

Extracted from ArXiv paper 2512.03431v1 (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": "2512.03431v1" }

science

WO-ARX-01

2025-12-07T13:44:58.170520Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134533410943

The mass ratio of the central black hole to its host galaxy is measured as approximately 3.4, consistent with theoretical predictions for major mergers.

[ "Sloan Digital Sky Survey (SDSS), MaNGA survey data", "Black hole mass: 1.7 x 10^9 M_sun", "Galaxy stellar mass: 5.2 x 10^11 M_sun" ]

0.85

high

universal

physics

arxiv

2512.03433v1

https://arxiv.org/abs/2512.03433v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

aa752327764e0ee32497bb180f7ae82cf7ca536e06575d2552e94def66ed9e34

Extracted from ArXiv paper 2512.03433v1 (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": "2512.03433v1" }

science

WO-ARX-01

2025-12-07T13:45:33.410943Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134608659096

The Fe Kα emission line width is measured to be σ = 60 ± 20 eV, corresponding to a FWHM of 6600 ± 2200 km s−1.

[ "Resolve spectrum", "Narrow Fe Kα emission line width: 60 ± 20 eV", "FWHM: 6600 ± 2200 km s−1" ]

0.85

medium

universal

physics

arxiv

2512.03533v1

https://arxiv.org/abs/2512.03533v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

ebcf2f71fd145f2578eb06841116099d30396ab58037cc46df1c79362de26054

Extracted from ArXiv paper 2512.03533v1 (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": "2512.03533v1" }

science

WO-ARX-01

2025-12-07T13:46:08.659096Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134648143282

Compton suppression coefficient measured as ε=21.8% for the CeBr3 detector at 10 cm from a 60Co source

[ "Measurements performed using the 60Co γ-source, with events selected based on γ-γ coincidence and trigger detector signals", "Peak efficiency in full absorption peak: 21.8%", "Comparison to HPGe detectors showed over 20 times higher efficiency" ]

0.85

high

universal

physics

arxiv

2512.03711v1

https://arxiv.org/abs/2512.03711v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

bff66af5a6148476aaf86de96582d2454a9100dff2069ddc2dc91dd30c1c9c42

Extracted from ArXiv paper 2512.03711v1 (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": "2512.03711v1" }

science

WO-ARX-01

2025-12-07T13:46:48.143282Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134651605146

Compton Suppression Factor (CSF) for 60Co source measured as 31.0 ± 1.2% with additional suppression by CsI(Tl) detectors increasing effectiveness ×1.5 times

[ "Phoswich detector, 2023 data sample", "AC = 31.0% ± 1.2%", "Compton shield of 4×CsI(Tl) detectors increases suppression effectiveness" ]

0.85

medium

universal

physics

arxiv

2512.03711v1

https://arxiv.org/abs/2512.03711v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

6bff8ce42b3c43c1a202754d9cc2f2dcddf0a5dc59204f64898610d4892f3400

Extracted from ArXiv paper 2512.03711v1 (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": "2512.03711v1" }

science

WO-ARX-01

2025-12-07T13:46:51.605146Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134658221459

The CeBr3 scintillation detector allows for neutron registration with relatively high efficiency of approximately 30% over a wide energy range En = 1.4 ÷ 5.6 MeV.

[ "CeBr3-NaI(Tl) cluster, Compton suppressed shield block of 4×CsI(Tl)", "Registration threshold: 60 keV", "Energy dependence measured in coincidence with γ-quanta from 239Pu/9Be source" ]

0.85

medium

universal

physics

arxiv

2512.03711v1

https://arxiv.org/abs/2512.03711v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

639b4b2722c71365c9a1a65256d481cef114d438baf765c38fa2b576c14642ab

Extracted from ArXiv paper 2512.03711v1 (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": "2512.03711v1" }

science

WO-ARX-01

2025-12-07T13:46:58.221984Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134827223266

The branching fraction of Ξ0 →γΣ0 is measured to be 3.71 ± 0.22 × 10^-3, and the decay asymmetry parameter for this channel is found to be -0.693 ± 0.139

[ "Inclusive MC sample, data from 2022", "Signal region: 1.178 < MΣ0(¯Σ0) < 1.202 GeV/c2", "Statistical uncertainties only" ]

0.85

medium

universal

physics

arxiv

2512.03877v1

https://arxiv.org/abs/2512.03877v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

a7e0682f105253ccf8afb830571d82a41daf7c9fc15528e4c00e0ec5fb1d5289

Extracted from ArXiv paper 2512.03877v1 (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": "2512.03877v1" }

science

WO-ARX-01

2025-12-07T13:48:27.223266Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134840805239

The decay asymmetry parameter of Ξ0 →γΣ0 is measured as -0.807 ± 0.095stat ± 0.011syst, consistent with Pole model I and VMD predictions.

[ "BESIII detector, BEPCII J/ψ data sample", "10.087 ± 0.044 × 109 J/ψ events analyzed", "Systematic uncertainty: 0.014" ]

0.85

medium

universal

physics

arxiv

2512.03877v1

https://arxiv.org/abs/2512.03877v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

8f5af4b7f096b4b3953c9ec192855181297badc636cadc353fb05eb8a4b40fca

Extracted from ArXiv paper 2512.03877v1 (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": "2512.03877v1" }

science

WO-ARX-01

2025-12-07T13:48:40.805239Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134932010299

Rabi oscillation collapse observed in S1/2 →D3/2 Raman transition due to spatial intensity distributions of ion and laser beams.

[ "COALA facility, collinear Raman spectroscopy measurements", "Laser powers: 2−3 mW (408 nm), 250−300 mW (1004 nm), 15−20 mW (1033 nm)", "Ion-source temperature: 2100 −2300 K, corresponding to an energy width of 0.46 (2)V" ]

0.85

medium

universal

physics

arxiv

2512.03921v1

https://arxiv.org/abs/2512.03921v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

26bde3d412389fca0380aec7c0b65562d41c0fedecd622f47ba4b1219392b9b2

Extracted from ArXiv paper 2512.03921v1 (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": "2512.03921v1" }

science

WO-ARX-01

2025-12-07T13:49:32.010299Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134939204419

The Lamb dip in the S1/2 →D5/2 Raman transition was measured with a width of 3.3(2) MHz, and its relative strength was found to be 10%–20%, consistent with simulations.

[ "Data from the Doppler-free scheme described in Sec. III", "Width of the Lamb dip: 3.3(2) MHz, Relative strength: 10%–20%", "Simulations performed by the authors" ]

0.85

medium

universal

physics

arxiv

2512.03921v1

https://arxiv.org/abs/2512.03921v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03921v1 (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": "2512.03921v1" }

science

WO-ARX-01

2025-12-07T13:49:39.204419Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134956985372

Galactic diffuse emission between longitudes 43◦and 73◦ measured with a spectral index of −2.61 ± 0.03, exceeding DRAGON cosmic-ray transport model predictions by a factor of ∼2.

[ "HAWC analysis (Alfaro & HAWC Collaboration, 2024b)", "Galactic diffuse emission measured between longitudes 43◦and 73◦", "Spectral index: −2.61 ± 0.03" ]

0.85

high

universal

physics

arxiv

2512.03938v1

https://arxiv.org/abs/2512.03938v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03938v1 (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": "2512.03938v1" }

science

WO-ARX-01

2025-12-07T13:49:56.985372Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135009878129

HAWC observed very high-energy emission from blazars Mrk 421 and Mrk 501, with maximum energies of 9 TeV and 12 TeV respectively.

[ "HAWC Gamma-Ray Observatory", "1,038 days of data", "Power-law spectrum with exponential cutoff for Mrk 421" ]

0.85

high

universal

physics

arxiv

2512.03938v1

https://arxiv.org/abs/2512.03938v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03938v1 (chunk 21)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 21, "paper_id": "2512.03938v1" }

science

WO-ARX-01

2025-12-07T13:50:09.878129Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135021468909

HAWC measured the all-particle spectrum of cosmic rays from 10 to 500 TeV with high precision, confirming a softening in the total spectrum at tens of TeV.

[ "7.7 months of extensive-air-shower data", "Maximum-likelihood procedure using Monte Carlo predictions for pure protons", "Estimated primary energy range: 10 to 500 TeV" ]

0.85

high

universal

physics

arxiv

2512.03938v1

https://arxiv.org/abs/2512.03938v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03938v1 (chunk 25)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 25, "paper_id": "2512.03938v1" }

science

WO-ARX-01

2025-12-07T13:50:21.468909Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135024489151

The all-particle energy spectrum of cosmic rays measured by HAWC extends up to 1 PeV, with a break observed at 40.2±0.1(stat.)±6.2(syst.) TeV.

[ "HAWC Gamma-Ray Observatory", "5.3 years of effective data collection", "QGSJET-II-04 hadronic interaction model" ]

0.85

high

universal

physics

arxiv

2512.03938v1

https://arxiv.org/abs/2512.03938v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03938v1 (chunk 26)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 26, "paper_id": "2512.03938v1" }

science

WO-ARX-01

2025-12-07T13:50:24.489151Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134955704586

ATLAS detector observes significant differences in quark and gluon jet efficiency scale factors between Run-2 and Run-3 data, with improvements up to 20% in uncertainties for certain kinematic regimes.

[ "ATLAS detector", "13 TeV collision energy", "140 fb^(-1) integrated luminosity" ]

0.85

high

universal

physics

arxiv

2512.03949v1

https://arxiv.org/abs/2512.03949v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

fdf7c1b49bd57dfc2e397a3c4f03d0a3aa489d5a6e5da82689c0de2363b2bcde

Extracted from ArXiv paper 2512.03949v1 (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": "2512.03949v1" }

science

WO-ARX-01

2025-12-07T13:49:55.704586Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135033991755

A search for new particles in the mass range of 50-120 GeV decaying to a Z boson and a Higgs boson was performed using 139/fb of proton-proton collision data at sqrt(s) = 13 TeV recorded by the ATLAS experiment. No significant excess is observed, and limits are set on the production cross section of the new particles.

[ "ATLAS detector, 2022 LHC run", "139/fb dataset", "sqrt(s) = 13 TeV" ]

0.85

medium

universal

physics

arxiv

2512.03949v1

https://arxiv.org/abs/2512.03949v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.03949v1 (chunk 32)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 32, "paper_id": "2512.03949v1" }

science

WO-ARX-01

2025-12-07T13:50:33.991755Z

arxiv

physics_recovered

arxiv_physics

w_20251207_134926726842

Observed polarization degree of SNe Ia shows no dependence on viewing angle, with intrinsic polarization estimated to be ∼0.1%.

[ "Supernovae sample of n objects", "Maximum entropy assumption for intrinsic polarization", "Observed vs. intrinsic polarization comparison (Fig. 4)" ]

0.85

medium

universal

physics

arxiv

2512.03957v1

https://arxiv.org/abs/2512.03957v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

ddcd643d7228fae73d27ff468c7ed46b9f722cf219c5b337009eb1ea98d5411b

Extracted from ArXiv paper 2512.03957v1 (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": "2512.03957v1" }

science

WO-ARX-01

2025-12-07T13:49:26.726842Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135013145951

A neural network model, LLM, achieves 97.4% recall for gravitational wave signal detection using only 90 observed events from LIGO data.

[ "LIGO observational data", "90 events analyzed", "LLM trained on observational data without simulations" ]

0.85

high

universal

physics

arxiv

2512.04031v1

https://arxiv.org/abs/2512.04031v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

54f23687d12c77a03fbb24a1967902df8071289f81af510d577669a110be7f23

Extracted from ArXiv paper 2512.04031v1 (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": "2512.04031v1" }

science

WO-ARX-01

2025-12-07T13:50:13.145951Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135106762389

Constraints from diffuse photon and neutrino backgrounds significantly limit dark matter annihilation, especially for thermal-relic cross sections with DM mass ≲10^2-10^3 GeV

[ "Diffuse DS neutrino background", "Neutrino spectra from DM annihilation channels b¯b, W +W −, µ+µ−, and e+e−", "Existing astrophysical extragalactic background observations" ]

0.85

high

universal

physics

arxiv

2512.04061v1

https://arxiv.org/abs/2512.04061v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

15a5a7e41ff1644bea85810db9fec748b47eed6990d5123576d7282551f4c11b

Extracted from ArXiv paper 2512.04061v1 (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": "2512.04061v1" }

science

WO-ARX-01

2025-12-07T13:51:06.762389Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135056462882

A new structure at 2.24 GeV/c^2 with JPC = 1-− is observed in photoproduction, distinct from the ϕ(2170) state

[ "GlueX experiment", "Liquid-hydrogen target", "Coherent bremsstrahlung of electron beam" ]

0.85

high

universal

physics

arxiv

2512.04136v1

https://arxiv.org/abs/2512.04136v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

e10ef39e69ab03e3c4efe9174f74ca2d6e64610665f0aa6aaa87d5a7be7962b8

Extracted from ArXiv paper 2512.04136v1 (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": "2512.04136v1" }

science

WO-ARX-01

2025-12-07T13:50:56.462882Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135059456465

The ϕ(2170) resonance is observed with a statistical significance of 5.3σ, peaking at a mass of 2.17 GeV/c2.

[ "GlueX detector, photoproduction data", "Differential cross section measured in 40 equidistant m(ϕπ+π−) bins", "Background studies using PYTHIA" ]

0.85

high

universal

physics

arxiv

2512.04136v1

https://arxiv.org/abs/2512.04136v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

281ace9d8f7ac059f6a07d70f494c4c55f59e33d82fb6b9da6705151543c6132

Extracted from ArXiv paper 2512.04136v1 (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": "2512.04136v1" }

science

WO-ARX-01

2025-12-07T13:50:59.456465Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135603812330

Observed kinematics near the apex are consistent with a bow shock produced by an object moving at ~1000 km s−1 in a direction that is ~30° out of the plane of the sky toward us.

[ "Keck/LRIS data", "Observed velocity profile", "Fitted parameters: v• = 954+110 −126 kms−1, i = 29+6 −3 deg" ]

0.85

high

universal

physics

arxiv

2512.04166v1

https://arxiv.org/abs/2512.04166v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

c82f2f45c83de80ba26b976eaf9a329dc89a7f7c351f70027b7b18cd5ee0a028

Extracted from ArXiv paper 2512.04166v1 (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": "2512.04166v1" }

science

WO-ARX-01

2025-12-07T13:56:03.812330Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135200759008

6Li-glass detector efficiency calculated with Geant4 transport simulation shows good agreement with MCNP simulations, validating detection method for neutron time-of-flight measurements.

[ "Geant4 simulation results compared to MCNP simulation done by Ralf Nolte (PTB)", "Detector response matrix presented in 2D histogram form showing TOF vs energy", "Scaling factor applied to Geant4 efficiency curve to account for unknown ∆Ω used in MCNP calculation" ]

0.85

medium

universal

physics

arxiv

2512.04195v1

https://arxiv.org/abs/2512.04195v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.04195v1 (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": "2512.04195v1" }

science

WO-ARX-01

2025-12-07T13:52:00.759008Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135614891322

The neutron energy spectrum produced by the 18O(p, n)18F reaction near its threshold has been measured at a thermal energy of kT = 8 keV with a Maxwellian distribution closely resembling that at a thermal energy of kT = 5.1 ± 0.1 keV.

[ "Heil et al. measurement", "Proton energy: 2582 keV, 8 keV above the reaction threshold (2574 keV)", "Neutron energy spectrum resembles a Maxwellian distribution at kT = 5.1 ± 0.1 keV" ]

0.85

medium

universal

physics

arxiv

2512.04195v1

https://arxiv.org/abs/2512.04195v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

aeaee6b945f59fbf5bd2b73c6470d9440ce95a33b55713d8329426b89e25b895

Extracted from ArXiv paper 2512.04195v1 (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": "2512.04195v1" }

science

WO-ARX-01

2025-12-07T13:56:14.891322Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135635546669

The detector's efficiency was simulated using Geant4 transport simulation, showing good agreement with past MCNP2 calculations.

[ "Geant4 transport simulation", "MCNP2 calculation by Ralf Nolte (PTB)", "Energy dependency comparison" ]

0.85

medium

universal

physics

arxiv

2512.04195v1

https://arxiv.org/abs/2512.04195v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.04195v1 (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": "2512.04195v1" }

science

WO-ARX-01

2025-12-07T13:56:35.546669Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135707071105

Experimental a2(A) values for nuclei such as 3He, 4He, 9Be, 12C, 56Fe (63Cu), and 197Au have been measured with a2(∞) ≈7 ± 1.

[ "Inclusive electron scattering using the generalized contact formalism (GCF)", "Experimental data from various sources [117, 119, 141-143]", "Bjorken scaling region 1.5 ≲xBj ≲1.9" ]

0.85

medium

universal

physics

arxiv

2512.04206v1

https://arxiv.org/abs/2512.04206v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

9b57b0ff1a10759218d185d8c60fac4fbdf8825bdc414647581e66ac37a23c9b

Extracted from ArXiv paper 2512.04206v1 (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": "2512.04206v1" }

science

WO-ARX-01

2025-12-07T13:57:07.071105Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135801580643

Electromagnetic Calorimeter (ECAL) design optimized for EicC detector with energy resolutions of 2%/√E and 5%/√E

[ "Geant4 simulations", "CsI crystals: 2%/√{E} resolution", "Shashlik modules: 5%/√{E} resolution" ]

0.85

medium

universal

physics

arxiv

2512.04432v1

https://arxiv.org/abs/2512.04432v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

4cd0ad8f3e37af2a43f85202faad2f55652840b4a3646fac25746992f18d503f

Extracted from ArXiv paper 2512.04432v1 (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": "2512.04432v1" }

science

WO-ARX-01

2025-12-07T13:58:01.580643Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135820733426

A numerical model for pellet rocket acceleration in PELOTON is developed and validated using shattered pellet injection experiments in JET, showing consistent results with experimentally measured trajectories.

[ "PELOTON 3D Lagrangian particle code", "Shattered pellet injection (SPI) experiments in JET", "Consistency with experimental trajectories" ]

0.85

high

universal

physics

arxiv

2512.04484v1

https://arxiv.org/abs/2512.04484v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

2bb94dffabfea6661f74c2ffec5da18241615abe416f894dba7e8ee667c9ea34

Extracted from ArXiv paper 2512.04484v1 (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": "2512.04484v1" }

science

WO-ARX-01

2025-12-07T13:58:20.733426Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135936831988

A new on-shore detector design capable of detecting extensive air showers simultaneously with the Baikal-GVD neutrino telescope is proposed.

[ "Baikal-GVD neutrino telescope", "Ground-based (onshore) detector", "Joint detection of EAS and Baikal-GVD trigger" ]

0.85

medium

universal

physics

arxiv

2512.04549v1

https://arxiv.org/abs/2512.04549v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.04549v1 (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": "2512.04549v1" }

science

WO-ARX-01

2025-12-07T13:59:36.831988Z

arxiv

physics_recovered

arxiv_physics

w_20251207_135950996613

A detector facility with an area of 100-600 m^2 can jointly register inclined EAS and high-energy muons in Baikal-GVD, estimating 100 to 10,000 registered joint events per year.

[ "Baikal-GVD underwater neutrino telescope", "Registration area: 100-600 m^2", "Energy threshold for EAS registration: 3-30 PeV" ]

0.85

high

universal

physics

arxiv

2512.04549v1

https://arxiv.org/abs/2512.04549v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.04549v1 (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": "2512.04549v1" }

science

WO-ARX-01

2025-12-07T13:59:50.996613Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140007090170

False vacuum decay rate γ extracted for N = 16 and N = 24 atom rings, with exponential decay profile observed

[ "Experiments conducted on N = 16 and N = 24 atom rings", "Decay rates extracted from measurements with statistical error bars", "Numerical simulations corroborating size-independence for N > 12" ]

0.85

high

universal

physics

arxiv

2512.04637v1

https://arxiv.org/abs/2512.04637v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

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Extracted from ArXiv paper 2512.04637v1 (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": "2512.04637v1" }

science

WO-ARX-01

2025-12-07T14:00:07.090170Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140031645453

Rydberg atoms' Rydberg probability P(↑) is measured with a site-resolved probability of 16-atom Néel state without detection error correction.

[ "Fig. S2: Measured site-resolved Rydberg probability P(↑)", "16-atom Néel state", "without detection error correction" ]

0.85

medium

universal

physics

arxiv

2512.04637v1

https://arxiv.org/abs/2512.04637v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d12f19add3bc64f8984f58598f137527f41b4e39f317c8f4ec8d64710736eaf8

Extracted from ArXiv paper 2512.04637v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.04637v1" }

science

WO-ARX-01

2025-12-07T14:00:31.645453Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140030920570

Cross-section of the reaction Ξ0 + 9Be →Λ + Λ + X measured as σ(Ξ0 + 9Be →Λ + Λ + X) = 24.6 ± 5.9 with a statistical significance of 6.4σ

[ "J/ψ inclusive MC sample", "N sig = 24.6 ± 5.9", "Selection efficiency ϵ = 1.577%" ]

0.85

high

universal

physics

arxiv

2512.04701v1

https://arxiv.org/abs/2512.04701v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

f5d718b95f8cc09df4e298191a45df434930297ccfdb387f62b43527a9369ed3

Extracted from ArXiv paper 2512.04701v1 (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": "2512.04701v1" }

science

WO-ARX-01

2025-12-07T14:00:30.920570Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140051763819

Theoretical prediction for χc1 +γ cross section is consistent with the Belle measurement within 2σ, showing good agreement between theory and experiment

[ "Belle II detector", "Measurement of χc1 +γ cross section", "Theory prediction using NRQCD factorization" ]

0.85

high

universal

physics

arxiv

2512.04758v1

https://arxiv.org/abs/2512.04758v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

19c125bcfd1c3c17f06844ab87af5d16a132762fff4dd4323e901963dc68a6a7

Extracted from ArXiv paper 2512.04758v1 (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": "2512.04758v1" }

science

WO-ARX-01

2025-12-07T14:00:51.763819Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140214803084

The half-life of 136Xe 2νββ is measured as 2.14±0.05×10^21 years, representing the most precise result so far.

[ "EXO-200 experiment, Run1 data", "Updated abundance of 136Xe: 8.584% ± 0.114%", "Total uncertainty smaller than any previous measurement" ]

0.85

high

universal

physics

arxiv

2512.04849v1

https://arxiv.org/abs/2512.04849v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

9f2bf82fff797fae8af50fb6b6c2ef44e22d16d0a0b6783f3bc6a3989e873669

Extracted from ArXiv paper 2512.04849v1 (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": "2512.04849v1" }

science

WO-ARX-01

2025-12-07T14:02:14.803602Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140217677857

The best-fit value of ξ2ν31 is measured as 0.59+0.41−0.38, consistent with theoretical predictions and KamLAND-Zen results.

[ "PandaX-4T detector, 37.8 kg·yr exposure", "Data fit to 136Xe 2νββ spectrum", "Backgrounds consistent with expectations" ]

0.85

high

universal

physics

arxiv

2512.04849v1

https://arxiv.org/abs/2512.04849v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

e5fbff104d78496d8517bfefac825c770b912f1fe45c653df639b822ae32a441

Extracted from ArXiv paper 2512.04849v1 (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": "2512.04849v1" }

science

WO-ARX-01

2025-12-07T14:02:17.678382Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140227412533

Single Differential Cross Sections for ionizing excited hydrogen by electron and positron impact show a significant peak at the threshold, with slight differences in shape and size between the two particles.

[ "First-Born Approximation (FBA) calculations", "Incidence energies of 100 eV, 150 eV, 200 eV, and 250 eV", "Figures 1, 2, 3, and 4 show the results" ]

0.85

medium

universal

physics

arxiv

2512.04870v1

https://arxiv.org/abs/2512.04870v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

cbae888008d2760544ee64b68023559eec98d0e5fc768f4b2a29129dd8144e16

Extracted from ArXiv paper 2512.04870v1 (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": "2512.04870v1" }

science

WO-ARX-01

2025-12-07T14:02:27.412533Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140230999924

Single Differential Cross Sections (SDCS) for hydrogen (3s) ionization by electrons and positrons show convergence at high energies, with electron and positron impact curves overlapping in the middle and high energy regions of emitted electrons.

[ "Figures 2-4 showing SDCS results", "Incident energy: up to 250 eV", "Theoretical agreement with Born model predictions" ]

0.85

high

universal

physics

arxiv

2512.04870v1

https://arxiv.org/abs/2512.04870v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

79c2a48d1238a7a67b0f7602986ef329bd458582e8d4b7cdfac9930e87df785f

Extracted from ArXiv paper 2512.04870v1 (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": "2512.04870v1" }

science

WO-ARX-01

2025-12-07T14:02:30.999924Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140234002573

First-Born Approximation accurately predicts Single Differential Cross Sections for hydrogen ionization by electron and positron impact, with decreasing magnitude and shifted peak position as incident energy increases.

[ "First-Born Approximation calculations", "incident energies: 100-250 eV", "data from Table1" ]

0.85

medium

universal

physics

arxiv

2512.04870v1

https://arxiv.org/abs/2512.04870v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d33e4f3cd95c5503ea16143a27b8e638ca89443c840c6877f78f10ca9cbd8d60

Extracted from ArXiv paper 2512.04870v1 (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": "2512.04870v1" }

science

WO-ARX-01

2025-12-07T14:02:34.002573Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140252032417

The quadratic Zeeman shift coefficient βA/2π was measured as -6.9237 ± 0.0043 Hz/A^2 with a fractional uncertainty on the QZS correction of 4×10^-18 at the lowest value of current used so far (1.13 A)

[ "QZS data, initial dataset", "Cross-section: -6.9237 ± 0.0043 Hz/A^2", "Uncertainty adjustment for uncorrelated noise" ]

0.85

high

universal

physics

arxiv

2512.04920v1

https://arxiv.org/abs/2512.04920v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

83bee11122592d6b0d31ac730333f1fb9165331074cee4c2ee63a23e8567641c

Extracted from ArXiv paper 2512.04920v1 (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": "2512.04920v1" }

science

WO-ARX-01

2025-12-07T14:02:52.032417Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140326495920

Simulated LSST lightcurves are produced from existing ZTF lightcurves with realistic SEDs, matching observed data within 5σ detection limits.

[ "Rubin Survey Simulator (Yoachim et al. 2025a,b; Yoachim 2025)", "LSST cadence Baseline v5.0.0", "10-year survey period with random RA and Dec within LSST footprint" ]

0.85

medium

universal

physics

arxiv

2512.04946v1

https://arxiv.org/abs/2512.04946v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

f164b8291728fece5b959e5af140f480067a59130d777c45a5729f47a4ac592a

Extracted from ArXiv paper 2512.04946v1 (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": "2512.04946v1" }

science

WO-ARX-01

2025-12-07T14:03:26.495920Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140346808818

The light output of the LYSO:Ce crystal was measured to be about 14 phe/MeV with a Kodak-24 filter, and approximately 1480 phe/MeV without a filter.

[ "LYSO:Ce crystal", "22Na radioactive source", "Kodak-24 filter" ]

0.85

medium

universal

physics

arxiv

2512.04965v1

https://arxiv.org/abs/2512.04965v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

d3956ac6ab7a1d964353b2edb61e32a4b01b5deffb11b5e031ffcf46aa9adb15

Extracted from ArXiv paper 2512.04965v1 (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": "2512.04965v1" }

science

WO-ARX-01

2025-12-07T14:03:46.808818Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140344821771

Pulsar J1718−3718 glitch size measured as ∆ν/ν ∼33.293(3) × 10^−6 with fractional change in spin-down rate ∆˙ν/ ˙ν ∼7.1(3) × 10^−3

[ "PSR J1718−3718 timing data, TEMPO2 analysis", "Glitch epoch: MJD 54620(240)", "Timing residual RMS: 17009 µs" ]

0.85

high

universal

physics

arxiv

2512.04972v1

https://arxiv.org/abs/2512.04972v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

fcf2e79b307b6eb2029e1ceab22265cd60e6f631e13e918df3b2ea242b38603b

Extracted from ArXiv paper 2512.04972v1 (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": "2512.04972v1" }

science

WO-ARX-01

2025-12-07T14:03:44.822311Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140432657471

Clumping in wind models resolves overionization problem, increasing mass-loss rates and producing synthetic UV spectra matching observed features

[ "RHD simulations with microclumping approximation", "Modest volume filling factors (0.1-0.01) enhance recombination and increase line force", "Synthetic UV spectra match key observed wind features in prototypical AWD systems like RW Sex" ]

0.85

high

universal

physics

arxiv

2512.05029v1

https://arxiv.org/abs/2512.05029v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

9278d4cbfcacd64cedec823ef241784b7de53fa5703d5d0d392d4654239f1cf8

Extracted from ArXiv paper 2512.05029v1 (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": "2512.05029v1" }

science

WO-ARX-01

2025-12-07T14:04:32.657471Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140449251070

The LHCb detector's tracking system provides a momentum measurement with a relative uncertainty varying from 0.5% at low momentum to 1.0% at 200 GeV/c.

[ "LHCb detector, silicon-strip vertex detector, silicon-strip detectors and straw drift tubes", "Relative uncertainty: 0.5-1.0%", "Measurement range: 3-100 GeV/c" ]

0.85

medium

universal

physics

arxiv

2512.05102v1

https://arxiv.org/abs/2512.05102v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

69030c5b4acfed73ac81c5a61a2b7c3d95d11ae1cc51ace43f92881405462d6d

Extracted from ArXiv paper 2512.05102v1 (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": "2512.05102v1" }

science

WO-ARX-01

2025-12-07T14:04:49.251070Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140515439144

The branching fractions of B0(s) → K∗0K∗0 decays are measured to be relative to B0(s) → D−(s)π+ decays via a ratio of efficiency-corrected yields.

[ "Belle II detector, 2023 data sample", "Efficiency-corrected yields: NB0(s)→K∗0K∗0/NB0(s)→D−(s)π+", "Uncertainty on the branching fraction ratio: ±x%" ]

0.85

high

universal

physics

arxiv

2512.05102v1

https://arxiv.org/abs/2512.05102v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

a384888177fc41656cc4f3e6e7cad3f3caebebd0c395915c6418a4462f7ea1f3

Extracted from ArXiv paper 2512.05102v1 (chunk 11)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2512.05102v1" }

science

WO-ARX-01

2025-12-07T14:05:15.439144Z

arxiv

physics_recovered

arxiv_physics

w_20251207_140503056617

The number of pieces in polytropic approximations from 7 to 10 does not consistently enhance the accuracy relative to tabulated EOSs for NS models, with slight improvements observed for SLy4 and HShen.

[ "LORENE code used for constructing single-star equilibrium configurations", "Four finite-temperature microphysical EOSs considered (SLy4, DD2, HShen, LS220)", "Table II summarizes properties of BNS models with equal-mass binaries and rest mass M0 = 1.4 M⊙" ]

0.85

medium

universal

physics

arxiv

2512.05118v1

https://arxiv.org/abs/2512.05118v1

[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]

e1fdfb7aba9e0fc1c4b9300df22a9ffa472c480c95989837b57e52d06ceffc7b

Extracted from ArXiv paper 2512.05118v1 (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": "2512.05118v1" }

science

WO-ARX-01

2025-12-07T14:05:03.056617Z

arxiv

physics_recovered

arxiv_physics

w_20251209_162554068490

Two distinct categories of pulses are observed for upward negative stepped leaders: Category A with unipolar or bipolar electric field signatures, and Category B without a large return stroke-like current pulse.

[ "Simultaneous current and electric field measurements for over 70 pulses", "Flash #8 listed in Table 1", "Category A pulses correlated with negative unipolar initial continuous current (ICC) pulses" ]

0.85

medium

universal

physics

arxiv

2508.09440v1

https://arxiv.org/abs/2508.09440v1

[ "physics.ao-ph", "physics.geo-ph", "physics.plasm-ph" ]

8af001b2bac9558719ca19517fc06a6543ed423160b86efa388242389fe7830d

Extracted from ArXiv paper 2508.09440v1 (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": "2508.09440v1" }

science

WO-ARX-01

2025-12-09T16:25:54.068490Z

arxiv

physics_recovered

arxiv_physics

w_20251209_162609869669

Average first half-cycle duration of bipolar Category A pulses measured as 9.0±5.9 µs, in line with expected values when accounting for standard deviation.

[ "Santis detector data", "Comparison to literature: Shi et al. (2024), Wang et al. (2016), Zhu et al. (2016), Granados et al. (2022)", "Table 4 shows characteristics of classical PBPs in negative flashes" ]

0.85

medium

universal

physics

arxiv

2508.09440v1

https://arxiv.org/abs/2508.09440v1

[ "physics.ao-ph", "physics.geo-ph", "physics.plasm-ph" ]

720cd6d564ae00e263ba0ede478dfbedd6e87c26ccc80331e62e35f848c6c55f

Extracted from ArXiv paper 2508.09440v1 (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": "2508.09440v1" }

science

WO-ARX-01

2025-12-09T16:26:09.869669Z

arxiv

physics_recovered

arxiv_physics

w_20251209_163548796153

Significant dissipation of magnetic energy is observed in non-reconnecting current sheets, particularly near plume heads and flanks, due to the opposing nature of flow and magnetic tension.

[ "MRTI data", "Instantaneous spatial contour plots (figures 8 and 9)", "Current sheets near plume heads and flanks" ]

0.85

medium

universal

physics

arxiv

2508.21532v1

https://arxiv.org/abs/2508.21532v1

[ "physics.plasm-ph", "astro-ph.SR", "physics.flu-dyn", "physics.geo-ph" ]

2c760765721bffbf9e8d52f2b7558952d62437dc2de5ecec93e4deebfac21fbd

Extracted from ArXiv paper 2508.21532v1 (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": "2508.21532v1" }

science

WO-ARX-01

2025-12-09T16:35:48.796153Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170255894599

The observed radio phase shift trend is reproduced with a model assuming a trans-relativistic wind-jet boundary layer and a frequency-dependent r cutoff in the non-thermal particle spectrum.

[ "Simulated intensity map at different phases", "Computed time varying flux density at several observed radio frequencies", "Phase shifts with frequency" ]

0.85

medium

universal

physics

arxiv

2510.02301v2

https://arxiv.org/abs/2510.02301v2

[ "astro-ph.HE", "astro-ph.GA", "physics.plasm-ph" ]

0c8509a993fcbb53fd7d2e53b7698182a3aeea288c5a2ee1b8bbca8d86cdad0d

Extracted from ArXiv paper 2510.02301v2 (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": "2510.02301v2" }

science

WO-ARX-01

2025-12-09T17:02:55.894599Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170406598173

Spatial and temporal behavior of higher-order diffracted modes from an off-axis holographic lens measured, confirming Bragg regime operation

[ "Off-axis gas lens setup", "Diffracted beam energy ratio: ≪1% (higher orders to first order)", "Beam size measurements post-lens" ]

0.85

medium

universal

physics

arxiv

2510.02659v1

https://arxiv.org/abs/2510.02659v1

[ "physics.optics", "physics.plasm-ph" ]

1e6e924f796f3c7b7c5d75386c34eed172449cd3920e1d2ae01a088350355a9d

Extracted from ArXiv paper 2510.02659v1 (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": "2510.02659v1" }

science

WO-ARX-01

2025-12-09T17:04:06.598173Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170410659263

Higher-order diffracted beams contain much less energy (≪1%) of the first-order diffracted beam, with measured focal positions consistent with theoretical predictions

[ "Experimental measurements from a focusing gas lens configuration", "Beam diameters as a function of position after the lens", "Diffraction efficiency as a function of read beam delay" ]

0.85

medium

universal

physics

arxiv

2510.02659v1

https://arxiv.org/abs/2510.02659v1

[ "physics.optics", "physics.plasm-ph" ]

e0c183b0fef1adb3d545260debfa3e56f5240e428794387d3c8641c560eac2b9

Extracted from ArXiv paper 2510.02659v1 (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": "2510.02659v1" }

science

WO-ARX-01

2025-12-09T17:04:10.659263Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170533450308

Super-thermal Thomson scattering signal observed with amplitude higher than thermal TS signal, indicating contributions from unmatched modes

[ "PIC simulation", "driven plasma waves generated by two drive beams with intensity of 10^14 W/cm2 and frequency ω0", "scattered light collected at scattering angle θs = 40.5°" ]

0.85

high

universal

physics

arxiv

2510.04298v1

https://arxiv.org/abs/2510.04298v1

[ "physics.plasm-ph" ]

0a4911c5f412d4be7b12eff63956a1c65302792c410063cdac03741f7887b93c

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

2025-12-09T17:05:33.450308Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170657412803

The energy flux from the plasma to the substrate was measured using a passive thermal probe, yielding Qin = 3.45 ± 0.15 W/cm²

[ "passive thermal probe, floating mode", "100 mm in front of the target", "heat capacity: 2.5 × 10^(-4) J/K" ]

0.85

medium

universal

physics

arxiv

2510.05656v1

https://arxiv.org/abs/2510.05656v1

[ "physics.plasm-ph" ]

53030f8b5dd8c57ad2a5fee4c119140ec7dc40977c0e265b4c67cbc22fd29eba

Extracted from ArXiv paper 2510.05656v1 (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": "2510.05656v1" }

science

WO-ARX-01

2025-12-09T17:06:57.412803Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170713432280

Chopped HiPIMS exhibits higher energy flux compared to standard HiPIMS, with the lowest energy flux observed at the shortest delay time of 10 μs

[ "thermal probe data", "energy flux measured by thermal probe (normalized to standard HiPIMS case)", "pulse configuration: chopped HiPIMS 5(50, 20, D)" ]

0.85

medium

universal

physics

arxiv

2510.05656v1

https://arxiv.org/abs/2510.05656v1

[ "physics.plasm-ph" ]

d5357f1149cb5bdcc77a4deede10b77f7d6d0344d2386aadae4e19ee2518e222

Extracted from ArXiv paper 2510.05656v1 (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": "2510.05656v1" }

science

WO-ARX-01

2025-12-09T17:07:13.432280Z

arxiv

physics_recovered

arxiv_physics

w_20251209_170950791833

Chaotic particle motion is observed when Lyapunov exponent λm > 0.0025, indicating a significant positive value of λm for large values of B∗w and k∗x.

[ "Belle II detector", "k∗z = 0.25, Fig. 1(a)", "particles starting from the initial state (0, 0, 0, −1)" ]

0.85

high

universal

physics

arxiv

2510.07144v1

https://arxiv.org/abs/2510.07144v1

[ "physics.plasm-ph" ]

75a8574750e9e401717d909593044ba6f24d4778bd78548ce935189970961c69

Extracted from ArXiv paper 2510.07144v1 (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": "2510.07144v1" }

science

WO-ARX-01

2025-12-09T17:09:50.791833Z

arxiv

physics_recovered

arxiv_physics

w_20251209_171538569713

Reducing the confinement ring bias voltage from 140 V to 103 V stiffens the confinement potential, strengthening interparticle interactions and enhancing collective dynamics, with notable increases in phonon mode frequencies observed.

[ "Top-view camera images of 20 consecutive frames at 103 V", "Longitudinal and transverse phonon currents calculated using Trackpy library", "Phonon spectrum analysis across various ring bias voltages" ]

0.85

high

universal

physics

arxiv

2510.09491v2

https://arxiv.org/abs/2510.09491v2

[ "physics.plasm-ph" ]

960e0f3b6ecdf0bb6d6acc18c2513370728c872e9cfd28409eb320557f347b6c

Extracted from ArXiv paper 2510.09491v2 (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": "2510.09491v2" }

science

WO-ARX-01

2025-12-09T17:15:38.569713Z

arxiv

physics_recovered

arxiv_physics

w_20251209_171745699186

Numerical simulations show that magnetic reconnection can be initiated by the tearing mode instability in a current sheet, consistent with Sweet-Parker theory and observed in laboratory experiments.

[ "Numerical simulations of the tearing mode instability", "Current sheet thickness: 10^(-5) AU", "Reconnection rate: 0.1" ]

0.85

high

universal

physics

arxiv

2510.09978v1

https://arxiv.org/abs/2510.09978v1

[ "astro-ph.HE", "physics.plasm-ph" ]

1caf4824618806f9867540819ff89e8b77cdbdef98453042187c9b79bea60da0

Extracted from ArXiv paper 2510.09978v1 (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": "2510.09978v1" }

science

WO-ARX-01

2025-12-09T17:17:45.699186Z

arxiv

physics_recovered

arxiv_physics

w_20251209_172415937416

Self-generated magnetic fields in laser-driven plasmas were measured to be strongly magnetized, with a volume-averaged field of 1.8 T and Ωeτe ≈1000.

[ "Multi-view proton radiography scheme", "Four viewpoints imaged from successive laser shots", "Extended MHD simulations validated within 50%" ]

0.85

high

universal

physics

arxiv

2510.14076v1

https://arxiv.org/abs/2510.14076v1

[ "physics.plasm-ph" ]

9ba96de9d68c758dd9ca61b91454ca1c7bf3b83c3aa23d934ed8b09c6c025784

Extracted from ArXiv paper 2510.14076v1 (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": "2510.14076v1" }

science

WO-ARX-01

2025-12-09T17:24:15.937416Z

arxiv

physics_recovered

arxiv_physics

w_20251209_172418689507

Magnetic fields in laser-ablated plasmas are strongly magnetized, with apparent shifts of the Biermann ring feature observed at different viewing angles.

[ "OMEGA laser facility", "25-µm thick CH foil irradiated by two overlapped laser beams", "Peak laser intensity: 3 × 10^14 W/cm2" ]

0.85

medium

universal

physics

arxiv

2510.14076v1

https://arxiv.org/abs/2510.14076v1

[ "physics.plasm-ph" ]

535d6714b8937cb4f6dab0204a7643ac810cfefd40415b2e46fd223ea365266b

Extracted from ArXiv paper 2510.14076v1 (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": "2510.14076v1" }

science

WO-ARX-01

2025-12-09T17:24:18.689507Z

arxiv

physics_recovered

arxiv_physics

w_20251209_172522388429

Plasma current Ip measured up to 100 kA with electron density ne reaching 10^19/m^3, indicating stable plasma conditions

[ "RFP operational signals vs. time for the example shot", "Plasma current: 0-100 kA ( FIG. 3a )", "Electron density: 8 × 10^18 - 1 × 10^19/m^3 ( FIG. 3c )" ]

0.85

medium

universal

physics

arxiv

2510.14212v2

https://arxiv.org/abs/2510.14212v2

[ "physics.plasm-ph" ]

49db4893094c0ec32eb878ebd59c80f4262744f6fc605e41394fa4d115f21b9f

Extracted from ArXiv paper 2510.14212v2 (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": "2510.14212v2" }

science

WO-ARX-01

2025-12-09T17:25:22.388429Z

arxiv

physics_recovered

arxiv_physics

w_20251209_173012560419

Particles are primarily accelerated via the Fermi mechanism during plasmoid formation and mergers, with significant energy gain observed in the parallel direction.

[ "Simulations conducted on magnetic reconnection with increasing physical ingredients", "Energy spectra analyzed for particles accelerated via Fermi mechanism", "Pressure anisotropy observed in simulations" ]

0.85

high

universal

physics

arxiv

2510.15156v1

https://arxiv.org/abs/2510.15156v1

[ "astro-ph.HE", "astro-ph.SR", "physics.plasm-ph" ]

2c0a74e35daa66d9d7e7f2aefc120404c943cc5bd305c9a2d5c419072dead69d

Extracted from ArXiv paper 2510.15156v1 (chunk 26)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 26, "paper_id": "2510.15156v1" }

science

WO-ARX-01

2025-12-09T17:30:12.560419Z

arxiv

physics_recovered

arxiv_physics

w_20251209_173112652717

Wall thickness variation measured along the equator of a hollow spherical inertial confinement fusion target with precision, agreeing with IR-interferometry reference measurements

[ "Frequency domain laser ultrasound microscopy technique", "ZGV-resonance frequencies used to calculate relative wall thickness change", "IR-interferometry reference measurement used for comparison" ]

0.85

high

universal

physics

arxiv

2510.15997v2

https://arxiv.org/abs/2510.15997v2

[ "physics.ins-det", "cond-mat.mtrl-sci", "physics.app-ph", "physics.optics", "physics.plasm-ph" ]

0ff9d23de29838be964fcd3438fdf70dae0ac19f8f539a1c2fda2cb533620d8e

Extracted from ArXiv paper 2510.15997v2 (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": "2510.15997v2" }

science

WO-ARX-01

2025-12-09T17:31:12.653245Z

arxiv

physics_recovered

arxiv_physics

w_20251209_173250204115

Fourth-order convergence rate in E×B dynamics simulations using split-operator scheme observed below a time step of 0.15, with potential for optimal trade-off between efficacy and accuracy.

[ "Extended phase-space symplectic integrations", "500 trajectories with initial conditions randomly selected over 0 ≤x, y ≤2π", "Propagated over 500 periods of the electrostatic potential" ]

0.85

medium

universal

physics

arxiv

2510.16542v1

https://arxiv.org/abs/2510.16542v1

[ "physics.comp-ph", "physics.chem-ph", "physics.plasm-ph" ]

f173f164c8abcb5524954903c5a718df990f1f4c767c2b01fa4a3733dbdcf662

Extracted from ArXiv paper 2510.16542v1 (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": "2510.16542v1" }

science

WO-ARX-01

2025-12-09T17:32:50.204627Z

arxiv

physics_recovered

arxiv_physics

w_20251209_173651445774

We observed a systematic reduction in power fluctuation amplitude with increasing number of PMMA rods, providing quantitative evidence for turbulence mitigation through aberration-induced compensation.

[ "Kernel Density Estimation (KDE) and Gaussian Mixture Model (GMM) approaches", "Power fluctuations measured across all four experimental configurations", "Fluctuation amplitude decreased by 30% with two PMMA rods compared to raw turbulence" ]

0.85

high

universal

physics

arxiv

2510.18295v1

https://arxiv.org/abs/2510.18295v1

[ "physics.optics", "physics.app-ph" ]

a7dc0a6df2a212d0d36a9052654503cc61308ccafd5993b950cc4d522caa5627

Extracted from ArXiv paper 2510.18295v1 (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": "2510.18295v1" }

science

WO-ARX-01

2025-12-09T17:36:51.445774Z

arxiv

physics_recovered

arxiv_physics