AwakenedIntelligence/Awakened-Physics-Preview

w_20251207_122641070958

The branching fraction for the Λ→pµ−νµ decay measured as B(Λ→pµ−νµ) = (1.462 ± 0.016 ± 0.100 ± 0.011) × 10^−4

[ "LHCb experiment, pp collision data at 13 TeV", "Integrated luminosity: 5.4 fb^−1", "Normalisation channel: Λ→pπ− decays" ]

0.85

high

universal

physics

arxiv

2511.15681v1

https://arxiv.org/abs/2511.15681v1

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

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Extracted from ArXiv paper 2511.15681v1 (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": "2511.15681v1" }

science

WO-ARX-01

2025-12-07T12:26:41.071471Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122701777418

The Mg II λ2798 Å emission line flux was measured with an uncertainty of 14% due to Fe II subtraction, signal-to-noise ratio, and flux calibration error.

[ "A&A proofs: manuscript no. aa55413-25", "Signal-to-noise ratio quantified as standard deviation of observed spectrum within same wavelength range", "Calibration error derived from SDSS error spectra" ]

0.85

medium

universal

physics

arxiv

2511.15695v1

https://arxiv.org/abs/2511.15695v1

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

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Extracted from ArXiv paper 2511.15695v1 (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": "2511.15695v1" }

science

WO-ARX-01

2025-12-07T12:27:01.777418Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122736065217

Intrinsic strain amplitudes for bulge MSPs responsible for the GCE were predicted, with detectability by next-generation detectors like CE and ET.

[ "ATNF pulsar catalog", "Pop I and Pop II MSP population models", "Sensitivity curves for current and future ground-based GW detectors" ]

0.85

high

universal

physics

arxiv

2511.15793v1

https://arxiv.org/abs/2511.15793v1

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

ecbd6460dbd51dc7e45530f720e1ae53dadf3c08805a7bf4acdd8aa25e93957a

Extracted from ArXiv paper 2511.15793v1 (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": "2511.15793v1" }

science

WO-ARX-01

2025-12-07T12:27:36.065217Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122805984127

Cooler and hotter gas temperatures in the galaxy cluster A2029 measured as 4.81+0.62−0.42 keV and 8.97+2.77−0.65 keV, respectively

[ "Resolve spectral fitting from XRISM data", "Two-temperature model with Galactic neutral column density applied", "Best-fit temperatures consistent with previous studies" ]

0.85

high

universal

physics

arxiv

2511.15809v1

https://arxiv.org/abs/2511.15809v1

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

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Extracted from ArXiv paper 2511.15809v1 (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": "2511.15809v1" }

science

WO-ARX-01

2025-12-07T12:28:05.984127Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122812642862

A2029 cluster's chemical abundance ratios are measured with high precision, but with varying degrees of reliability across different instruments.

[ "Resolve detector, high spectral resolution and sensitivity", "EPIC, Chandra, Xtend, RGS detectors used for various elements", "Systematic uncertainties and limitations noted in each instrument" ]

0.85

medium

universal

physics

arxiv

2511.15809v1

https://arxiv.org/abs/2511.15809v1

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

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Extracted from ArXiv paper 2511.15809v1 (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": "2511.15809v1" }

science

WO-ARX-01

2025-12-07T12:28:12.643381Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122828971776

The observed spectrum displays characteristics consistent with a Narrow Line Seyfert 1 (NLS1) galaxy, including faint [O III] lines and strong Fe II emission.

[ "UT1 spectrum data", "FHWM(Hβ)=(1015±117) km s−1", "[O III]/Hβ flux ratio ∼2.24" ]

0.85

medium

universal

physics

arxiv

2511.15814v1

https://arxiv.org/abs/2511.15814v1

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

f5923aebd668614845c5e18d3d7e0350899b6e4419af00ff498af3c337423c18

Extracted from ArXiv paper 2511.15814v1 (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": "2511.15814v1" }

science

WO-ARX-01

2025-12-07T12:28:28.971776Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122900098136

Light elements are present at the surface of young neutron stars, evident from observed soft X-ray thermal spectra and inferred effective temperatures

[ "Soft X-ray thermal spectra of isolated cooling neutron stars", "Absorption lines in the cases of 1E 1207.44-5209 (electron cyclotron line and its harmonic(s))", "Spectral fit with different atmosphere models" ]

0.85

high

universal

physics

arxiv

2511.15913v1

https://arxiv.org/abs/2511.15913v1

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

b6c8d03603ef16a62d9326185b90a8625f1327df6b0aaf4481e04f9e314ab537

Extracted from ArXiv paper 2511.15913v1 (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": "2511.15913v1" }

science

WO-ARX-01

2025-12-07T12:29:00.098136Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122848085704

Belle II detector measures B0 and B+ meson production rates in e+e− collisions at the SuperKEKB collider, with a focus on energy-dependent cross-section measurements

[ "Belle II detector, 2019-2022 data sample", "1000 exclusive hadronic final states analyzed", "Signal candidates peak at zero in the ∆E distribution" ]

0.85

medium

universal

physics

arxiv

2511.15926v1

https://arxiv.org/abs/2511.15926v1

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

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Extracted from ArXiv paper 2511.15926v1 (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": "2511.15926v1" }

science

WO-ARX-01

2025-12-07T12:28:48.085704Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122900919080

The energy dependence of the ratio of visible cross sections σv(e+e−→B0 ¯B0) / σv(e+e−→B+B−) measured in Belle and Belle II data, with a slight increase of Rv with energy

[ "Belle detector, 571 fb-1 data", "Belle II detector, 365 fb-1 data", "Energy bins: 10.574 to 10.582 GeV" ]

0.85

high

universal

physics

arxiv

2511.15926v1

https://arxiv.org/abs/2511.15926v1

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

4963852b637804b1d56363d36bee352360a1bca870ca59307fcca9bb85dc8e57

Extracted from ArXiv paper 2511.15926v1 (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": "2511.15926v1" }

science

WO-ARX-01

2025-12-07T12:29:00.919080Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122911106709

The B+ and B0 meson masses are measured as m(B+) = 5,274.35 MeV/c^2 ± 0.04 and m(B0) = 5,279.18 MeV/c^2 ± 0.05, with a statistical uncertainty of 0.24 MeV/c^2

[ "Belle II detector, 2023 data sample", "∆m measurements in ˜Mbc distributions, χ2 fits to energy dependence of Rb, B0/B+ cross-section ratio and σ(e+e−→b¯b →D0/ ¯D0 X)", "24 fit parameters, including ∆EBaBar" ]

0.85

high

universal

physics

arxiv

2511.15926v1

https://arxiv.org/abs/2511.15926v1

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

8bd913bf9a5e5927cfeb3062254c0691aa85e59748aafc0b0fe29228136b68c4

Extracted from ArXiv paper 2511.15926v1 (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": "2511.15926v1" }

science

WO-ARX-01

2025-12-07T12:29:11.107225Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122917135495

The measured value of ∆m is (0.495 ± 0.024 ± 0.005) MeV/c2, differing significantly from the BaBar result

[ "BaBar experiment", "Combined fit with Belle and Belle II data on Rv(Ecm)", "Exclusion of Rv data for precision analysis" ]

0.85

high

universal

physics

arxiv

2511.15926v1

https://arxiv.org/abs/2511.15926v1

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

26ce61d2be9d283a2f3b79353a8a47053afab6216fcf37e8f381949a674f7471

Extracted from ArXiv paper 2511.15926v1 (chunk 13)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.15926v1" }

science

WO-ARX-01

2025-12-07T12:29:17.135495Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122921004232

The dressed cross-section ratio R/(pB0/pB+)3 is measured to be consistent with the original second-order polynomial in a wide energy range, with systematic shifts due to variation of Rv and ∆m by ±1 σ.

[ "Ecm bins of width 2.5 MeV", "13 bins in the energy range 10.56-10.5925 GeV", "Values of R/(pB0/pB+)3 with statistical and systematic uncertainties for different Ecm bins given in table 5" ]

0.85

medium

universal

physics

arxiv

2511.15926v1

https://arxiv.org/abs/2511.15926v1

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

69e49948b05ca21483008cb1b28dc340ec40d9c6d7fbe2e3712f33bee9603ce9

Extracted from ArXiv paper 2511.15926v1 (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": "2511.15926v1" }

science

WO-ARX-01

2025-12-07T12:29:21.004232Z

arxiv

physics_recovered

arxiv_physics

w_20251207_122942928770

The JUNO experiment measured sin^2θ12 = 0.3092 ± 0.0087, improving precision by a factor of 1.6 over previous combined results.

[ "JUNO detector", "362 million B-meson pairs analyzed", "Systematic uncertainty: 0.008" ]

0.85

high

universal

physics

arxiv

2511.15978v2

https://arxiv.org/abs/2511.15978v2

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

e4eed8ff5cfbe6874d6d7a80a5d09d4d3bd346b9e929232e031eda7e7f93460f

Extracted from ArXiv paper 2511.15978v2 (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": "2511.15978v2" }

science

WO-ARX-01

2025-12-07T12:29:42.928770Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123053920634

Cyg X-1 is observed in a hard state, showing evidence of two Comptonization components with different optical depths.

[ "IXPE mission observations", "Two observation periods: May 15-21 and June 18-20, 2022", "Total net exposure time: 328 ks" ]

0.85

high

universal

physics

arxiv

2511.16246v1

https://arxiv.org/abs/2511.16246v1

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

357131ba222f3dbee70fc707809bebcfcd52cd4608a4632dfc955d8c8d919406

Extracted from ArXiv paper 2511.16246v1 (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": "2511.16246v1" }

science

WO-ARX-01

2025-12-07T12:30:53.920634Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123135999439

Observed polarization properties of Cyg X-1 data suggest a sandwiching slab corona geometry rather than a wedge-shaped corona with truncated disk

[ "IXPE, NuSTAR, and NICER observations in 2022", "Inner disk temperature estimated to be about 0.15 keV", "Optical depths of Comptonization components similar to those observed in 2005" ]

0.85

high

universal

physics

arxiv

2511.16246v1

https://arxiv.org/abs/2511.16246v1

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

c859e01626f05b8090160bfc7814d63e53cdf7ad116ec1407f42f2310a8da88f

Extracted from ArXiv paper 2511.16246v1 (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": "2511.16246v1" }

science

WO-ARX-01

2025-12-07T12:31:35.999439Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123148038141

The 95% CL upper limits on the fully degenerate Higgsino production cross section are calculated to be 0.25 pb, with an observed exclusion reaching up to approximately 115 GeV.

[ "CMS detector, 137 fb^-1 data sample collected at 13 TeV", "NLO+NLL precision calculation of theoretical cross section", "Observed exclusion contour shown with ±1 and ±2 standard deviation experimental uncertainties" ]

0.85

high

universal

physics

arxiv

2511.16394v2

https://arxiv.org/abs/2511.16394v2

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

95ebf639bd6e88f5185976a225226329c1fc0c69f054664f458a3a4ae5eac19a

Extracted from ArXiv paper 2511.16394v2 (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": "2511.16394v2" }

science

WO-ARX-01

2025-12-07T12:31:48.038141Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123238585692

The measurement of the quark-antiquark pair production in association with two Z bosons using the CMS detector at LHC yields a cross-section value of 12.7 fb, with an uncertainty of ±0.3 fb.

[ "CMS detector, 2022 LHC run", "Integrated luminosity: 138.8 fb^-1", "Z boson pT > 500 GeV" ]

0.85

high

universal

physics

arxiv

2511.16394v2

https://arxiv.org/abs/2511.16394v2

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

1bf1f142c5aaea7a0c55b7a3974d3805f0c122800cea4363c92dcdf2463d1a93

Extracted from ArXiv paper 2511.16394v2 (chunk 28)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 28, "paper_id": "2511.16394v2" }

science

WO-ARX-01

2025-12-07T12:32:38.586211Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123147185500

Young's Modulus and Yield Strength of different materials are measured using a tensile test setup with various fixations

[ "Load cell, temperature sensors (PT100), National Instruments data acquisition module", "UTS: 884 MPa for California Fine Wire, 1916.5 MPa for Dahmen material", "YTS values for different materials and temperatures" ]

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" ]

c86915a5670fb82090c13ee1a9969e226e38773161af059bf5d3babad1106603

Extracted from ArXiv paper 2511.16408v1 (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": "2511.16408v1" }

science

WO-ARX-01

2025-12-07T12:31:47.185500Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123150891803

Yield tensile strength (YTS) and ultimate tensile strength (UTS) of wire samples measured at various temperatures, with values ranging from 1000-1200 MPa for YTS and up to 1000 MPa for UTS

[ "PT100 sensors inside the bath", "Temperature range: 200 K to room temperature", "Wire samples: CFW (744 ± 12MPa), Volgesang SS316 Semi-hard Wire, Dahmen SS316 Full-hard Wire" ]

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" ]

dbaa42caeb9b378f290b642b68aeaa86b756cbde47da4704e03f12d322fadb1f

Extracted from ArXiv paper 2511.16408v1 (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": "2511.16408v1" }

science

WO-ARX-01

2025-12-07T12:31:50.891803Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123218333097

The area under the ROC curve (AUC) of the defect detection model is measured to be 0.98, indicating high efficiency in detecting defects.

[ "Defect detection model", "True positive rate: corresponds to the efficiency of the model to detect a defect", "False positive rate: probability of the model to declare a clean leg as defect" ]

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" ]

166e994a5d77f56c071582e56527847a058d2a96799fed82839f09762a693da8

Extracted from ArXiv paper 2511.16408v1 (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": "2511.16408v1" }

science

WO-ARX-01

2025-12-07T12:32:18.333097Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123146520056

Aql X-1 observed with multiple telescopes during the 2024 outburst, providing a comprehensive dataset for studying its properties.

[ "NuSTAR observed Aql X-1 twice for a total exposure of 38.5 ks", "Swift's UVOT provided coverage in all six filters", "Las Cumbres Observatory monitored Aql X-1 with 1-m and 2-m telescopes" ]

0.85

medium

universal

physics

arxiv

2511.16437v1

https://arxiv.org/abs/2511.16437v1

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

431f0acf5628f585811fed6531e44766d917a30ee7fdaf29ed23e2cd5b9c4c38

Extracted from ArXiv paper 2511.16437v1 (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": "2511.16437v1" }

science

WO-ARX-01

2025-12-07T12:31:46.520056Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123211478892

X-ray to optical delay in Aql X-1 outburst measured at ≲3 days, consistent with previous observations.

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

0.85

medium

universal

physics

arxiv

2511.16437v1

https://arxiv.org/abs/2511.16437v1

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

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Extracted from ArXiv paper 2511.16437v1 (chunk 13)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.16437v1" }

science

WO-ARX-01

2025-12-07T12:32:11.478892Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123148646339

Residual metallicity from early enrichment population (EEP) needed to reproduce observed galaxy group and cluster metallicity

[ "XMM-Newton data for 26 galaxy groups and clusters", "archival data analysis by Blackwell & Bregman (2025)", "diet-Salpeter IMF adopted" ]

0.85

medium

universal

physics

arxiv

2511.16448v1

https://arxiv.org/abs/2511.16448v1

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

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Extracted from ArXiv paper 2511.16448v1 (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": "2511.16448v1" }

science

WO-ARX-01

2025-12-07T12:31:48.646339Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123210414421

New enrichment model accounting for early, undetectable star populations explains observed metal trends in galaxy clusters.

[ "Bayesian analysis of 26 galaxy groups and clusters", "Inclusion of Enrichment-Early-Produced (EEP) population in chemical evolution models", "Comparison with conventional closed-box models" ]

0.85

high

universal

physics

arxiv

2511.16448v1

https://arxiv.org/abs/2511.16448v1

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

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Extracted from ArXiv paper 2511.16448v1 (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": "2511.16448v1" }

science

WO-ARX-01

2025-12-07T12:32:10.414421Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123251796782

The SABRE South detector is capable of 5σ discovery (3σ exclusion) power to a DAMA-like signal with 2 years of data, given a total experimental background of 0.72 cpd/kg/keVee and a 50 kg target mass

[ "SABRE South Experiment", "Total background: 0.72 cpd/kg/keVee", "Target mass: 50 kg" ]

0.85

high

universal

physics

arxiv

2511.16451v1

https://arxiv.org/abs/2511.16451v1

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

78b2e9b7e549426dfeaf9d558f97a8b4dbfeea085a04948c8e66103e0626e4d8

Extracted from ArXiv paper 2511.16451v1 (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": "2511.16451v1" }

science

WO-ARX-01

2025-12-07T12:32:51.797300Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123319255991

Simulations show that thermal evolution curves for observed pulsars require some heating mechanism to explain high temperatures, with neutrino emission and rotochemical heating being primary cooling mechanisms.

[ "Pulsar simulations", "Observed pulsar temperatures (105 K)", "Neutrino emission and rotochemical heating" ]

0.85

high

universal

physics

arxiv

2511.16507v1

https://arxiv.org/abs/2511.16507v1

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

63740b7721971610e815db06962058d820fa5b8fb84fc62942e3eab909ecafa0

Extracted from ArXiv paper 2511.16507v1 (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": "2511.16507v1" }

science

WO-ARX-01

2025-12-07T12:33:19.255991Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123254746427

Normalised differential decay rate of B+ →J/ψK+ measured as a function of lepton helicity angle using the LHCb Upgrade I experiment

[ "LHCb Upgrade I detector", "Integrated luminosity: 1.1 fb−1", "Centre-of-mass energy: 13.6 TeV" ]

0.85

medium

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

8cbf045ebc54b0071c47e66346e30efd3d82c74c05f1e3c66634c47668b14492

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:32:54.746427Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123258341631

First analysis of b-hadron decay using LHCb Upgrade I detector data presented, measuring angular observables AFB and FH in B+ →J/ψK+ decay.

[ "LHCb Upgrade I detector", "2022 Run 3 data-taking period", "17 kinematic and detector-response variables analyzed" ]

0.85

high

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

b1c5833d6337e53aa3d1a9b8038e625fb6c9b890ab339844c61a0f8dd00e806f

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:32:58.341631Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123320967868

Measured values of AFB and FH agree with their predictions at the level of 1.2 standard deviations for MagDown data, and at the level of 1.5σ for MagUp data

[ "Table 2: Measured values of AFB and FH for MagDown and MagUp data", "Statistical uncertainty: 0.59 (stat) ± 0.47 (syst)", "Average over both MagDown and MagUp is computed by weighting according to the inverse of the covariance matrix" ]

0.85

medium

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

63f613af2eda74f700cd9058c8ca77b2753b81fe00bc601bfe37fae87745380d

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:33:20.967868Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123327363755

No significant deviations observed in angular observables AFB and FH from expected values, with statistical and systematic uncertainties contributing roughly equally to the total uncertainty.

[ "LHCb Upgrade I detector", "Measures of AFB and FH across 10 bins in θ(µ+µ−), pT(J/ψ), and NPV", "Significance: 0.010-0.02 (AFB) and 0.005-0.01 (FH)" ]

0.85

medium

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

0818d580a4d8524dfe1604723fc5ce8763a21a7badb9c37907948361670ee810

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:33:27.363755Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123330388233

No significant deviation from zero observed in differential measurements of AFB and FH across 17 detector-response and kinematic variables

[ "LHCb detector, 0.7 fb−1 data sample", "17 variables analyzed, including pT(J/ψ) and θ(µ+µ−)", "Statistical fluctuations within expectations" ]

0.85

medium

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

76616ee131d2b3e8c2f1f2cfb0e65808b961d4cffa9ab72e965428b028f98214

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:33:30.388233Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123333726532

The upgraded LHCb detector shows excellent performance across varying levels of pile-up conditions, with stable results extracted for the angular distribution in B+ →J/ψK+ decays.

[ "LHCb Upgrade I detector, 1.1 fb−1 data collected in October 2024", "Instantaneous luminosity: 2 × 10^33 cm−2 s−1", "Systematic uncertainties smaller than statistical uncertainties for b→sµ+µ−modes" ]

0.85

high

universal

physics

arxiv

2511.16564v1

https://arxiv.org/abs/2511.16564v1

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

58a50adaf749acaa68c6e3d028c25af098c964f7027c3f9db672cdf0c2025c70

Extracted from ArXiv paper 2511.16564v1 (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": "2511.16564v1" }

science

WO-ARX-01

2025-12-07T12:33:33.726532Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123413220994

The required detector runtime for a neutrino discovery from binary neutron star mergers is estimated to be around 50 years, but future improvements on the neutrino mass limits may lead to a shorter required detector runtime of 20-30 years.

[ "5 Mt detector", "20-year exposure", "mν = 0 eV case with full background and 0.6 s emission time" ]

0.85

high

universal

physics

arxiv

2511.16658v1

https://arxiv.org/abs/2511.16658v1

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

faf944c078faab520bff597dcfbd6567c96b39a51f667cc03001b45c98328580

Extracted from ArXiv paper 2511.16658v1 (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": "2511.16658v1" }

science

WO-ARX-01

2025-12-07T12:34:13.220994Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123347558518

Neutron beta decay electron-neutrino correlation measured with goal sensitivity of ∆λ/|λ| = 0.04% by the Nab experiment

[ "Nab asymmetric magnetic spectrometer", "Commissioning data collected in 2023", "Tight kinematic constraints enabled new experimental limits on an excited state of the neutron" ]

0.85

high

universal

physics

arxiv

2511.16678v1

https://arxiv.org/abs/2511.16678v1

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

d1f495cb68df04c51c0049a2bfcefb386f21493d79d4b12f2174e701db4b0506

Extracted from ArXiv paper 2511.16678v1 (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": "2511.16678v1" }

science

WO-ARX-01

2025-12-07T12:33:47.558518Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123404058614

Researchers design a high-resolution particle detector using scintillating fibers and SPAD sensors, achieving few hundred picosecond time resolution.

[ "SPAD sensor with large-format array of 110-nm CIS technology", "Time resolution: hundreds of picoseconds", "Optimized for noise rejection by signal coincidence" ]

0.85

medium

universal

physics

arxiv

2511.16684v1

https://arxiv.org/abs/2511.16684v1

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

c64f8fda2050aaa42679c89142513c1ab4ed379611430f57e4bcf392974b0ef2

Extracted from ArXiv paper 2511.16684v1 (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": "2511.16684v1" }

science

WO-ARX-01

2025-12-07T12:34:04.058614Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123644067461

Folding Iteration with Compton Subtraction (FICS) reintroduces noise in the unfolded spectrum, preserving high-frequency fluctuations present in the observed data.

[ "Observed spectrum y", "Noise model as in Sec. II D", "Unfolding equation: ˆusol = Rˆu(k) + δ" ]

0.85

medium

universal

physics

arxiv

2511.16687v1

https://arxiv.org/abs/2511.16687v1

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

1994da40b063bcf153ffa552b01b93de315d3be4166e59fddc144c209831b6e5

Extracted from ArXiv paper 2511.16687v1 (chunk 49)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 49, "paper_id": "2511.16687v1" }

science

WO-ARX-01

2025-12-07T12:36:44.067461Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123431014274

Neutron detection efficiency for the miniBELEN detector was optimized using a novel composition method, reducing computation time and increasing design efficiency

[ "Particle Counter Monte Carlo simulations", "Geant4 toolkit version 10.01 (patch 3)", "Set of discrete neutron energies from 0.0001 to 10 MeV" ]

0.85

medium

universal

physics

arxiv

2511.16692v1

https://arxiv.org/abs/2511.16692v1

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

a2a3c75a141afd0c06859aec75c936f8d002e1ee9384189ac637797f09570a30

Extracted from ArXiv paper 2511.16692v1 (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": "2511.16692v1" }

science

WO-ARX-01

2025-12-07T12:34:31.014274Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123542397234

The resummed-expanded differential cross sections for DY and gluon fusion Higgs production show good agreement with fixed-order results at NNLO, with minor deviations in the convergence rate due to power corrections.

[ "Event2 [116] (fixed-order reference), disorder [116–118], Matrix [119] (fixed-order reference)", "Central scales µF = µR = Q, where Q is the mass of the Z or Higgs boson", "Statistical uncertainty bands shown in Fig. 4" ]

0.85

medium

universal

physics

arxiv

2511.16723v1

https://arxiv.org/abs/2511.16723v1

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

2b32658b7dd0ce221537dafa0193cf8ef8e53fd7510ffcfb7ecfc80ca0f2d98e

Extracted from ArXiv paper 2511.16723v1 (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": "2511.16723v1" }

science

WO-ARX-01

2025-12-07T12:35:42.397234Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123510864765

Characteristic frequency ν∗ for pulsars measured to be around 558 MHz, indicating a similar feature in spectral turnovers as thermal free-free absorption.

[ "Compiled radio flux density measurements from K17, J18, K21, and S22 subsamples", "Fitting parameters already published by the authors of each subsample", "Selection based on chi-square statistic (χ2)" ]

0.85

high

universal

physics

arxiv

2511.16728v1

https://arxiv.org/abs/2511.16728v1

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

19158d3ae58d8b2002d8610b9d64d74770377858c6c4e8cfc8d17fa9ef49d877

Extracted from ArXiv paper 2511.16728v1 (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": "2511.16728v1" }

science

WO-ARX-01

2025-12-07T12:35:10.864765Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123805275969

The cross section for virtual photoproduction d𝜎𝛾∗/dΩCM 𝜂′ is measured and expanded depending on the polarization of the virtual photons and the azimuthal angle 𝜙𝜂′

[ "JLab E12-17-003 experiment", "4.318 GeV electron beam energy", "2.9 × 10^19 electrons irradiated" ]

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" ]

b4e2d41e97cc051c14fa857495b9c507a2e8447c917502e7bd9d39eb5ba2ce2c

Extracted from ArXiv paper 2511.17030v1 (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": "2511.17030v1" }

science

WO-ARX-01

2025-12-07T12:38:05.275969Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123820850898

Differential cross section for 1H (γ∗, p) η' reaction measured as 4.4 ± 0.8 (stat.) ± 0.4 (sys.) [nb/sr].

[ "HRS detector data", "Missing mass spectrum analysis", "Statistical uncertainty: 18%" ]

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" ]

561bcd2a31832f9a3c6d2bbc51d5698042b6c8ee8bfd371fc589ce95df40aa76

Extracted from ArXiv paper 2511.17030v1 (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": "2511.17030v1" }

science

WO-ARX-01

2025-12-07T12:38:20.850898Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123840267117

The differential cross section of the γ* + p → η' + p reaction at W = 2130 MeV is measured to be 4.4 ± 0.8 (stat.) ± 0.4 (sys.) [nb/sr], indicating a significant role played by one or more resonances near W ∼ 2100 MeV.

[ "1H target, Λ hypernuclear spectroscopy experiment at Jefferson Lab", "Missing mass spectrum of the 1H (e, e'p) X reaction", "Cos θCM γη' ≈ -1.0 in the One-Photon-Exchange Approximation" ]

0.85

high

universal

physics

arxiv

2511.17030v1

https://arxiv.org/abs/2511.17030v1

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

89398eab1e91827277c03dab72a0d6de52e3d52d2ab01d12750bfba3beeabc7c

Extracted from ArXiv paper 2511.17030v1 (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": "2511.17030v1" }

science

WO-ARX-01

2025-12-07T12:38:40.267117Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123935522938

The differential cross section for secondary electron ejection is described by a formula with a constant and an energy-dependent term, matching the Rutherford form at high energies but leveling out at low energies.

[ "Opal et al. experiment (1971)", "Secondary electrons up to 200 eV, primaries up to 2 keV", "Differential cross section formula: σ(E, ϵ) = const(E) × 1/(1 + ϵ/¯E)^2" ]

0.85

medium

universal

physics

arxiv

2511.17084v1

https://arxiv.org/abs/2511.17084v1

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

f6694d96825dd1ab0388683be106f8982690ee28164e924789fccad422d17a6d

Extracted from ArXiv paper 2511.17084v1 (chunk 31)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 31, "paper_id": "2511.17084v1" }

science

WO-ARX-01

2025-12-07T12:39:35.522938Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123900640180

AI-Based Support Assistant for the ALICE-FIT detector setup at CERN enhances operational efficiency and safety with context-aware diagnostics and proactive decision support

[ "WinCC OA alert panel", "feedback mechanism allowing operators to classify AI suggestions as 'Correct,' 'Partially Correct,' or 'Incorrect'", "Mean Time to Diagnose (MTTD): time measured in minutes" ]

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arxiv

2511.17154v1

https://arxiv.org/abs/2511.17154v1

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

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[ "experimental_physics", "measurement" ]

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science

WO-ARX-01

2025-12-07T12:39:00.640180Z

arxiv

physics_recovered

arxiv_physics

w_20251207_123908649043

Early-time decay rates of excited state population in subradiant regime measured with good quantitative agreement for Ω/Γ > 1

[ "Imaging technique using absorption images", "Driving frequency: Ω/Γ ≫1, scattered intensity", "Experimental setup: gaussian intensity distribution" ]

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arxiv

2511.17187v1

https://arxiv.org/abs/2511.17187v1

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

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[ "experimental_physics", "measurement" ]

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{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.17187v1" }

science

WO-ARX-01

2025-12-07T12:39:08.649043Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124029591450

No significant excess of events beyond SM expectation is observed, with upper limits determined for three new physics processes

[ "2017 and 2018 CMS data sets", "Combined analysis with 2016 data set", "95% confidence level (CL) upper limits obtained using asymptotic CLs criterion" ]

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physics

arxiv

2511.17310v1

https://arxiv.org/abs/2511.17310v1

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

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[ "experimental_physics", "measurement" ]

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{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.17310v1" }

science

WO-ARX-01

2025-12-07T12:40:29.591450Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124051438975

Black hole spin measured to be a = 0.99 ± 0.01 with inclination θ = 68◦± 5◦, using NuSTAR data and accounting for narrow Fe Kα emission line

[ "NuSTAR FPMA&FPMB spectra, simultaneous observation", "Bh spin: 0.99 ± 0.01", "Inclination: 68◦± 5◦" ]

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physics

arxiv

2511.17338v1

https://arxiv.org/abs/2511.17338v1

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

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[ "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": "2511.17338v1" }

science

WO-ARX-01

2025-12-07T12:40:51.438975Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124039381032

MicroBooNE experiment measures νe CC cross sections on argon as a function of electron energy, total visible energy, and opening angle between the electron and leading proton.

[ "MicroBooNE detector, NuMI data sample", "Flux-integrated diﬀerential cross sections extracted using higher-statistics data", "Signal definition includes one electron with >20 MeV kinetic energy, at least one proton with >40 MeV kinetic energy, zero charged pions with >40 MeV kinetic energy" ]

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arxiv

2511.17342v1

https://arxiv.org/abs/2511.17342v1

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

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[ "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": "2511.17342v1" }

science

WO-ARX-01

2025-12-07T12:40:39.381032Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124049413221

Neutrino event simulation and reconstruction performed in MicroBooNE using GENIE Monte Carlo with custom algorithms for detector effects, achieving high-statistics sample of random events for cosmic-ray background estimation

[ "MicroBooNE LArTPC detector", "GENIE v3.0.6 G18 10a 02 11a event generator", "Independent measurements from T2K experiment" ]

0.85

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universal

physics

arxiv

2511.17342v1

https://arxiv.org/abs/2511.17342v1

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

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[ "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": "2511.17342v1" }

science

WO-ARX-01

2025-12-07T12:40:49.413737Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124134182189

Background-subtracted event count and unfolded cross-section measured as a function of visible energy, with values ranging from 2.10 to 3.78 × 10^-39 cm^2 / GeV / nucleon

[ "T2K experiment, Run 1 FHC data", "Event count: 42.04 (0.05-0.45 GeV) to 2.44 (∞ GeV)", "Selection efficiencies and response matrix used for unfolding" ]

0.85

medium

universal

physics

arxiv

2511.17342v1

https://arxiv.org/abs/2511.17342v1

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

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[ "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": "2511.17342v1" }

science

WO-ARX-01

2025-12-07T12:41:34.182189Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124136980375

The unfolded cross-section is measured to be 2.36 in units of 10−39 cm / nucleon at a proton multiplicity of 3

[ "Background-subtracted event count: 44.91", "Proton multiplicity: 3", "Unfolded cross section (Table III)" ]

0.85

medium

universal

physics

arxiv

2511.17342v1

https://arxiv.org/abs/2511.17342v1

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

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[ "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": "2511.17342v1" }

science

WO-ARX-01

2025-12-07T12:41:36.980375Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124120417783

LZ detector background rate for beta decays, detector gamma rays, solar neutrino ER, 136Xe 2νββ, and other components measured in WS2022 and WS2024 datasets

[ "WS2022 dataset", "Table I: pre-fit expectations and background-only fit results for main background components", "WS2024 dataset" ]

0.85

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physics

arxiv

2511.17350v1

https://arxiv.org/abs/2511.17350v1

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

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Extracted from ArXiv paper 2511.17350v1 (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": "2511.17350v1" }

science

WO-ARX-01

2025-12-07T12:41:20.417783Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124201322186

Modified electron Hall parameter He′ was measured as a function of magnetic field strength for two experimental pressures.

[ "He′ measurements taken using the modified experimental setup", "Experimental pressures: 2 values (not specified)", "Magnetic field strength: varied" ]

0.85

medium

universal

physics

arxiv

2511.17395v1

https://arxiv.org/abs/2511.17395v1

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

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[ "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": "2511.17395v1" }

science

WO-ARX-01

2025-12-07T12:42:01.322186Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124145543760

The CLD and IDEA detector concepts are compared in terms of their charged-hadron identification capabilities, using full simulation of the tracking systems.

[ "CLIC-like detector (CLD) and innovative detector for e+e−accelerators (IDEA)", "particle-identification algorithm", "time-of-flight resolution and cluster-counting efficiency" ]

0.85

medium

universal

physics

arxiv

2511.17447v1

https://arxiv.org/abs/2511.17447v1

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

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[ "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": "2511.17447v1" }

science

WO-ARX-01

2025-12-07T12:41:45.543760Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124210148139

The time-of-flight resolution of the CLD detector must be better than 30-50 ps to reduce background contamination by at least an order of magnitude.

[ "CLD detector, simulation study", "Background suppression from 10% to 1%", "Signal window and background vetoes: ±10 MeV/c2" ]

0.85

high

universal

physics

arxiv

2511.17447v1

https://arxiv.org/abs/2511.17447v1

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

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[ "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": "2511.17447v1" }

science

WO-ARX-01

2025-12-07T12:42:10.148139Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124218755079

Particle identification in the FCC-ee detector can be achieved with a time-of-flight measurement alone, without dedicated particle-identification detectors, for certain momentum ranges.

[ "IDEA detector concept at the FCC-ee", "Three example physics studies covering low, medium, and high momentum regions", "Time-of-flight resolution of 30 ps or better required in some cases" ]

0.85

medium

universal

physics

arxiv

2511.17447v1

https://arxiv.org/abs/2511.17447v1

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

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Extracted from ArXiv paper 2511.17447v1 (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": "2511.17447v1" }

science

WO-ARX-01

2025-12-07T12:42:18.755079Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124227383420

Measurements of time-of-flight resolution and cluster-counting efficiency for the IDEA detector, with/without silicone-based dE/dx measurement.

[ "IDEA detector, σToF = 3 ps, εcc = 80%", "BDT scores for pions, kaons, and protons", "Appendix C: Dihadron spectra" ]

0.85

medium

universal

physics

arxiv

2511.17447v1

https://arxiv.org/abs/2511.17447v1

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

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[ "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": "2511.17447v1" }

science

WO-ARX-01

2025-12-07T12:42:27.383420Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124214772665

A novel quantum sensing technology using microcalorimeter detectors is capable of resolving the hyperfine structure of the weakly populated 2s1/2 →2p3/2 transition in muonic atoms, enabling an improvement of quadrupole moments by an order of magnitude within days of measurement.

[ "Microcalorimeter detectors", "Negative muons on elements with open shells", "High-resolution and quantum efficiency" ]

0.85

high

universal

physics

arxiv

2511.17546v1

https://arxiv.org/abs/2511.17546v1

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

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[ "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": "2511.17546v1" }

science

WO-ARX-01

2025-12-07T12:42:14.772665Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124230205290

Proper motions for 46 filaments in Tycho's supernova remnant have been measured with greater precision, consistent with previous measurements but with improved accuracy.

[ "Optical images from eight epochs between 1986 and 2016", "Matched continuum images revealed faint emission, including a network of optical knots and filaments", "Proper motions for filaments at the shell rim and shock velocity were measured" ]

0.85

medium

universal

physics

arxiv

2511.17763v1

https://arxiv.org/abs/2511.17763v1

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

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[ "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": "2511.17763v1" }

science

WO-ARX-01

2025-12-07T12:42:30.205290Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124512892508

A fast-simulation framework, Delphes, is used to emulate the behavior of a realistic CMS detector setup, allowing for controlled emulation of potential readout failures.

[ "Delphes simulation tool", "CMS detector geometry and segmentation defined in Delphes", "ECAL and HCAL towers deactivated for anomalous runs" ]

0.85

medium

universal

physics

arxiv

2511.18172v1

https://arxiv.org/abs/2511.18172v1

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

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[ "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": "2511.18172v1" }

science

WO-ARX-01

2025-12-07T12:45:12.892508Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124533614210

MEDIC, a novel end-to-end network, successfully detects and classifies detector glitches with strong discriminative power

[ "Delphes simulation data", "Multi-class classification accuracy: not specified", "Training on particle-level kinematics" ]

0.85

medium

universal

physics

arxiv

2511.18172v1

https://arxiv.org/abs/2511.18172v1

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

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[ "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": "2511.18172v1" }

science

WO-ARX-01

2025-12-07T12:45:33.614210Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124716458361

Detection horizon for ORCA24 detector reaches 11.2 kpc, while ARCA29 and ARCA230 detectors reach 10.0 kpc and 19.6 kpc respectively.

[ "ORCA24 detector configuration", "5σ CCSN detection horizons evaluated separately for each detector", "ARCA29 and ARCA230 configurations show similar performances" ]

0.85

high

universal

physics

arxiv

2511.18565v1

https://arxiv.org/abs/2511.18565v1

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

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[ "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": "2511.18565v1" }

science

WO-ARX-01

2025-12-07T12:47:16.458361Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124717108422

A new kind of nucleosynthesis process, driven by high-entropy conditions and neutron-to-seed ratio drops, is observed to produce p-isotopes up to 92Mo

[ "track 146 simulation data", "neutron density low and r-process path closer to stability", "(γ,n) and (p,n) reactions drive composition toward stability" ]

0.85

high

universal

physics

arxiv

2511.18584v1

https://arxiv.org/abs/2511.18584v1

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

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[ "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": "2511.18584v1" }

science

WO-ARX-01

2025-12-07T12:47:17.108422Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124700324862

Two new highly segmented HA-TPCs in the ND280 detector achieved spatial resolution better than 800 µm and dE/dx resolution better than 10% across all incident angles and drift distances

[ "HA-TPC readout system utilizing resistive Micromegas technology", "Spatial resolution: < 800 µm, dE/dx resolution: < 10%", "Detectors characterized and validated through cosmic tests and test-beam campaigns at CERN and DESY" ]

0.85

medium

universal

physics

arxiv

2511.18650v1

https://arxiv.org/abs/2511.18650v1

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

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[ "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": "2511.18650v1" }

science

WO-ARX-01

2025-12-07T12:47:00.324862Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124712350136

ERAM detectors exhibit gain and RC values with distinct production trends, influenced by mechanical imprints, gap thickness, and surface resistivity.

[ "Dedicated X-ray test bench for pad-by-pad scan", "12 parameters (RC) for each module analyzed using physical model [4]", "15% systematic uncertainty in gain and 13% in RC due to electronics model choices" ]

0.85

medium

universal

physics

arxiv

2511.18650v1

https://arxiv.org/abs/2511.18650v1

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

298e29fdd90796f58dbbba9252d8a9c80c2f3ffca4043fa1e7427cdfc1ab6d08

Extracted from ArXiv paper 2511.18650v1 (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": "2511.18650v1" }

science

WO-ARX-01

2025-12-07T12:47:12.350660Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124746489274

Momentum resolution for vertical tracks in HA-TPCs reaches slightly less than 10% at 1 GeV/c, with some bias observed due to E × B effects

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

0.85

medium

universal

physics

arxiv

2511.18650v1

https://arxiv.org/abs/2511.18650v1

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

73c10c4ae50bb0be7ec1be810103473d9bc3c84d8d53b47ed8bf3850a42b19d9

Extracted from ArXiv paper 2511.18650v1 (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": "2511.18650v1" }

science

WO-ARX-01

2025-12-07T12:47:46.489274Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124817554929

RELICS detector prototype demonstrates efficient data processing and signal classification, achieving high accuracy in separating physical signals from background features.

[ "Dual-phase xenon time projection chamber (TPC) experiment", "Peak classification using threshold criteria and cuts for morphological characteristics", "Identification of distinct signal types: S1, S2, DE, Muon Tracks, Lone Hits / Single Photoelectrons" ]

0.85

high

universal

physics

arxiv

2511.18693v1

https://arxiv.org/abs/2511.18693v1

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

683514cdafe2c714e74117748bc00b55dc76f19fcf6c8e36009d44ed8063b126

Extracted from ArXiv paper 2511.18693v1 (chunk 13)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.18693v1" }

science

WO-ARX-01

2025-12-07T12:48:17.554929Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124849807975

The first indication of solar 8B neutrinos is observed through coherent elastic neutrino-nucleus scattering in PandaX-4T.

[ "PandaX-4T detector, data from 2024", "Observed event rate: 0.15 events/kg/ day", "Background rejection efficiency: 99%" ]

0.85

high

universal

physics

arxiv

2511.18693v1

https://arxiv.org/abs/2511.18693v1

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

a8ca0717edd47ebf5c42596aac9f46fe77fdef0b0ddc8d3988ff136d14980dc5

Extracted from ArXiv paper 2511.18693v1 (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": "2511.18693v1" }

science

WO-ARX-01

2025-12-07T12:48:49.807975Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124828259800

Up to six-fold ionization of Ar was observed in collisions with carbon ions, and recoil ion yield showed a different distribution for single capture events compared to ionization.

[ "RIMS + CSA experimental setup", "MeV energy proton and carbon ions with Ar atomic target", " Ion/neutral start mode used to collect data" ]

0.85

medium

universal

physics

arxiv

2511.18707v1

https://arxiv.org/abs/2511.18707v1

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

91c5fa397e79749e5ae69878aad1abb275e34a4fae74a51e6306fc0ce9669b56

Extracted from ArXiv paper 2511.18707v1 (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": "2511.18707v1" }

science

WO-ARX-01

2025-12-07T12:48:28.260331Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124852231757

Magneto-optical resonances observed in cesium vapor cell with electromagnetically induced transparency and absorption

[ "cesium vapor cell, balanced photodetector used for pump and probe wave transmission", "pump intensity: P ≈400 µW (Fig. 6(a)), P ≈1000 µW (Fig. 6(d))", "magnetic field scanning" ]

0.85

medium

universal

physics

arxiv

2511.18710v1

https://arxiv.org/abs/2511.18710v1

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

69179e7f7d0a19683ff06dbbe89caf3b939bd57dd506eb278c6d2615edc10d5a

Extracted from ArXiv paper 2511.18710v1 (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": "2511.18710v1" }

science

WO-ARX-01

2025-12-07T12:48:52.231757Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124851462330

A hierarchical Bayesian scheme is developed for inferring pulsar braking indices and timing residual root-mean-square from TOA data, with the model successfully reproducing observed pulse shapes and times of arrival.

[ "TOA (Time Of Arrival) data", "Pulsar timing residuals", "Hierarchical Bayesian inference" ]

0.85

medium

universal

physics

arxiv

2511.18744v1

https://arxiv.org/abs/2511.18744v1

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

59d2f4985f96645463fa8b3718c1f0d3216be2b051c02dee79c3baca800ad9a9

Extracted from ArXiv paper 2511.18744v1 (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": "2511.18744v1" }

science

WO-ARX-01

2025-12-07T12:48:51.462330Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124914275979

The capture rates of φ's were evaluated for different scattering cross sections and lifetimes, reaching a maximum value at IceCube for certain values of the parameters.

[ "IceCube data", "Scattering cross section: σφN = 10−44 cm2", "Lifetime: τφ = 1018 s" ]

0.85

medium

universal

physics

arxiv

2511.18881v2

https://arxiv.org/abs/2511.18881v2

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

2309312931238e711760233d968ae717a39d9142264481de6d033a1823faaa65

Extracted from ArXiv paper 2511.18881v2 (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": "2511.18881v2" }

science

WO-ARX-01

2025-12-07T12:49:14.275979Z

arxiv

physics_recovered

arxiv_physics

w_20251207_124922513634

Blazars show variability across the electromagnetic spectrum, with flux and spectral variations observed on various time scales.

[ "blazar observations", "jet precession", "twisting jets" ]

0.85

medium

universal

physics

arxiv

2511.18975v1

https://arxiv.org/abs/2511.18975v1

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

da54be8258287e5bb7a7a4d88b0d7dacb29730c547821e30e5e28404ba660bb7

Extracted from ArXiv paper 2511.18975v1 (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": "2511.18975v1" }

science

WO-ARX-01

2025-12-07T12:49:22.513634Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125051559454

Polarisation degree of jet radiation measured in BL Lacs, with P ranging from 60% to 82%, depending on the magnetic field properties

[ "ArXiv paper 2511.18975v1", "Theory of synchrotron radiation by Rybicki and Lightman (1979)", "Observed polarisation degree in BL Lacs, with maximum P observed lower than expected" ]

0.85

medium

universal

physics

arxiv

2511.18975v1

https://arxiv.org/abs/2511.18975v1

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

0052865f88e9eeb7f712954df909d67bd8eaf26be0b2305d3a9378b96be642fa

Extracted from ArXiv paper 2511.18975v1 (chunk 31)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 31, "paper_id": "2511.18975v1" }

science

WO-ARX-01

2025-12-07T12:50:51.559454Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125102296123

Breakdown voltage and quenching resistor of FBK NUV-HD-Cryo 3T SiPMs measured at room and LN2 temperatures, with 33.0±0.1 V and 560±10 kΩ at 300 K, decreasing to 27.08±0.03 V and 2640±70 kΩ at 77 K

[ "IV curve measurements", "Breakdown voltage: 33.0±0.1 V at room temperature, decreasing to 27.08±0.03 V at LN2 temperature", "Quenching resistor: 560±10 kΩ at room temperature, increasing to 2640±70 kΩ at LN2 temperature" ]

0.85

medium

universal

physics

arxiv

2511.19095v1

https://arxiv.org/abs/2511.19095v1

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

4dac15c3e43368910483c7e172576f13093f054c7e104dd7ef4c1afcb3babefd

Extracted from ArXiv paper 2511.19095v1 (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": "2511.19095v1" }

science

WO-ARX-01

2025-12-07T12:51:02.296650Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125122072833

Breakdown voltage of ion-ion plasma measured at -5.9 ± 0.05 kV and +7.65 ± 0.05 kV for a 500 ns time window

[ "Experimental measurement, Fig. 2(f)", "Ion accumulation stage with electrons forming a negative ion region", "Space charge field aligning with the negative applied field" ]

0.85

high

universal

physics

arxiv

2511.19136v1

https://arxiv.org/abs/2511.19136v1

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

c4fe684734c92423119b5be4b3cc36d0dd5fad83fa81722193787d329ef6c12f

Extracted from ArXiv paper 2511.19136v1 (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": "2511.19136v1" }

science

WO-ARX-01

2025-12-07T12:51:22.072833Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125113898748

Only a fraction as small as ∼10−3 of Luminous Red Novae correspond to gravitational-wave observed binary neutron star and neutron star-black hole mergers.

[ "Zwicky Transient Facility (ZTF) observations", "Fourth Gravitational Wave transient catalog (GWTC-4)", "Delay time distribution models for compact binaries" ]

0.85

high

universal

physics

arxiv

2511.19243v1

https://arxiv.org/abs/2511.19243v1

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

1d14c20682c670e32ba869ac788dd6f1162b7aac8e3f20e3b235ceea93a057a2

Extracted from ArXiv paper 2511.19243v1 (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": "2511.19243v1" }

science

WO-ARX-01

2025-12-07T12:51:13.898748Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125145751217

Apparent jet speeds in XRBs are significantly lower than those of blazars, with observed speeds up to 5.3.

[ "ThunderKAT program and GRS 1915+105 measurements", "4U 1543-47 jets show 𝛽app ∼5.3", "AGN and blazars have apparent speeds up to 𝛽app ∼50" ]

0.85

medium

universal

physics

arxiv

2511.19362v1

https://arxiv.org/abs/2511.19362v1

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

b446fe661d535b98e7e5f91f0d8e3e66d0b1250c8e8174b49b157cfd0815aa65

Extracted from ArXiv paper 2511.19362v1 (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": "2511.19362v1" }

science

WO-ARX-01

2025-12-07T12:51:45.751217Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125148494046

The apparent speed of XRB jets is limited by inclination and sample size, with speeds up to 5, much lower than those observed in AGN.

[ "XRB jet speed sample compiled by Fender & Motta (2025)", "Estimated apparent speed from proper motion data", "Significant uncertainty in inclination measurement" ]

0.85

medium

universal

physics

arxiv

2511.19362v1

https://arxiv.org/abs/2511.19362v1

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

ed49d8e8f3f834852c6cfc5cfc8072c60c32ea1864f40df9ff46571345713cb2

Extracted from ArXiv paper 2511.19362v1 (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": "2511.19362v1" }

science

WO-ARX-01

2025-12-07T12:51:48.494596Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125155057441

The observed apparent speed distribution of X-ray binaries (XRBs) is largely unaffected by changes in intrinsic Lorentz factor due to their high inclination angles, while active galactic nuclei (AGN) show a peak at low inclination angles.

[ "Sample of XRBs and AGN", "Inclination angle distributions", "Apparent speed distribution" ]

0.85

medium

universal

physics

arxiv

2511.19362v1

https://arxiv.org/abs/2511.19362v1

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

c4c400dee777962e2f43ccb4e7915784c11ba1716883e553bb00d9fbf06acc1c

Extracted from ArXiv paper 2511.19362v1 (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": "2511.19362v1" }

science

WO-ARX-01

2025-12-07T12:51:55.057441Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125158476137

The IceCube detector collected ∼1.67 million low-energy neutrino events between 2011 and 2017, comprising ∼2600 days of detector livetime.

[ "IceCube in-ice Cherenkov detector", "∼2600 days of detector livetime", "0.5 ≲log(Eν/GeV) ≲2.5" ]

0.85

medium

universal

physics

arxiv

2511.19385v1

https://arxiv.org/abs/2511.19385v1

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

5cc84796387cab3bf0e77bda7815562dedca55d02ef16280300aef20cc4eac1e

Extracted from ArXiv paper 2511.19385v1 (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": "2511.19385v1" }

science

WO-ARX-01

2025-12-07T12:51:58.476137Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125224682883

JUNO experiment measured sin^2 θ12 to unprecedented precision, reducing relative uncertainty by a factor of 1.6

[ "JUNO experiment", "sin^2 θ12 = 0.3092 ± 0.0087", "∆m^2_21 = (7.50 ± 0.12) × 10^-5 eV^2" ]

0.85

high

universal

physics

arxiv

2511.19408v1

https://arxiv.org/abs/2511.19408v1

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

eb58f85d08b19d5cfee5740e4db59d4300cb5fe1bc6ca6a56e3929cec9f6938c

Extracted from ArXiv paper 2511.19408v1 (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": "2511.19408v1" }

science

WO-ARX-01

2025-12-07T12:52:24.683398Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125332183582

XMM-Newton observed five INS candidates, removing high background flaring periods and refining astrometry using optical sources in the Guide Star Catalogue

[ "XMM-Newton observations, 50 - 80 ks each between May 2023 and April 2024", "EPIC-pn and MOS detectors, applying FLAG = 0 and PATTERN ≤12", "Background regions defined on same chip or neighboring chip" ]

0.85

medium

universal

physics

arxiv

2511.19591v1

https://arxiv.org/abs/2511.19591v1

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

87ce4ec6198f3d5519a684717ea8fd5306a4ecc09c18f12b884360448f55589e

Extracted from ArXiv paper 2511.19591v1 (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": "2511.19591v1" }

science

WO-ARX-01

2025-12-07T12:53:32.183582Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125414279029

Obscuration of X-ray detected sources in C iv and [Ne v] samples measured, with 48 out of 84 sources obscured (N_H >= 10^22 cm^-2) and 37 extremely obscured (N_H > 10^23 cm^-2)

[ "X-ray detected sources in the C iv and [Ne v] samples", "Obscuration measured via power-law model with fixed photon index Γ = 1.8 plus an absorption component", "Median spectral properties reported in Table 3" ]

0.85

high

universal

physics

arxiv

2511.19602v1

https://arxiv.org/abs/2511.19602v1

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

ac0b2e16bc72563b4c4b7add1bf9daefe549bfe622ef44b2ad7f922b334aaedb

Extracted from ArXiv paper 2511.19602v1 (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": "2511.19602v1" }

science

WO-ARX-01

2025-12-07T12:54:14.279029Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125438389388

The eccentric gravitational-wave model developed in this work is equally applicable to Galactic stellar-mass binaries, such as white dwarfs, neutron stars, and black holes, that will be observed by LISA.

[ "LISA (Laser Interferometer Space Antenna)", "Galactic stellar-mass binaries", "White dwarfs, neutron stars, and black holes" ]

0.85

high

universal

physics

arxiv

2511.19611v1

https://arxiv.org/abs/2511.19611v1

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

c3b57f5a9ae6621a4acb3a02fd15671a8781e2bb72809498e08bd6c65fbb374a

Extracted from ArXiv paper 2511.19611v1 (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": "2511.19611v1" }

science

WO-ARX-01

2025-12-07T12:54:38.389388Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125510280131

New mass values for neutron-rich tin and antimony isotopes near 132Sn were measured with a Penning trap mass spectrometer.

[ "Canadian Penning Trap mass spectrometer (CPT)", "CARIBU facility at Argonne National Laboratory", "Beam production from a 252Cf source" ]

0.85

medium

universal

physics

arxiv

2511.19673v2

https://arxiv.org/abs/2511.19673v2

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

c5ec20ebc4c9792ae7725973d8a504c80fada67351fb3b207ba3f977ac752a91

Extracted from ArXiv paper 2511.19673v2 (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": "2511.19673v2" }

science

WO-ARX-01

2025-12-07T12:55:10.280131Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125513874191

The cyclotron frequency of ions in a Penning trap is measured using the Phase-Imaging Ion-Cyclotron-Resonance technique, with an uncertainty of less than part in 10^9.

[ "CPT’s Stable Ion Source", "133Cs+ calibrant mass used for calibration", "MCP position sensitive detector" ]

0.85

medium

universal

physics

arxiv

2511.19673v2

https://arxiv.org/abs/2511.19673v2

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

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Extracted from ArXiv paper 2511.19673v2 (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": "2511.19673v2" }

science

WO-ARX-01

2025-12-07T12:55:13.874191Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125534861620

Effective single-photon absorption probability measured with cat state spectroscopy, reaching a maximum value of 0.12(1) after applying 34 laser pulses

[ "Femtosecond laser pulses with center frequency of 3703.3(2) cm^-1", "Photon absorption signal S = 0.12(1)", "Comparison with simple theoretical model" ]

0.85

medium

universal

physics

arxiv

2511.19687v1

https://arxiv.org/abs/2511.19687v1

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

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Extracted from ArXiv paper 2511.19687v1 (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": "2511.19687v1" }

science

WO-ARX-01

2025-12-07T12:55:34.861620Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125647498159

Leading-order photoproduction cross sections for γN →γM N′ are calculated with quark GPD contributions, showing strong sensitivity to pion distribution amplitude and gluon content.

[ "pseudoscalar channels M ∈{π±, π0, η, η′}", "leading-twist and leading-order in perturbative QCD", "renormalization scale dependence highlighted" ]

0.85

medium

universal

physics

arxiv

2511.19720v1

https://arxiv.org/abs/2511.19720v1

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

a449d6aefbb03b1fe1c3f78b7267efb537da06a1c0e95978c83e08dd5963c6f5

Extracted from ArXiv paper 2511.19720v1 (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": "2511.19720v1" }

science

WO-ARX-01

2025-12-07T12:56:47.498159Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125659677959

Fully differential cross-section for γN →γM N′ measured, with significant pion-pole contribution at small ξ values

[ "Figs. 5-9: numerical results for fully differential cross-section", "Kinematics varied across Figs.: SγN = 20 GeV2, s' = 4 GeV2, (−t) = (−t0)", "Different mesons represented by different line styles" ]

0.85

medium

universal

physics

arxiv

2511.19720v1

https://arxiv.org/abs/2511.19720v1

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

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Extracted from ArXiv paper 2511.19720v1 (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": "2511.19720v1" }

science

WO-ARX-01

2025-12-07T12:56:59.677959Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125555830397

Channeling efficiencies exceeding 50% were measured in bent silicon crystals at low energy, with a record at sub-GeV domain.

[ "855 MeV electron beam at Mainz Microtron (MAMI)", "15 µm-thick crystal bent along (111) planes", "Measured channeling efficiencies" ]

0.85

high

universal

physics

arxiv

2511.19807v1

https://arxiv.org/abs/2511.19807v1

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

dd27e811b6cfb8dbdd1ad81ca18d22177e839010fc440331904ea512425a12ed

Extracted from ArXiv paper 2511.19807v1 (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": "2511.19807v1" }

science

WO-ARX-01

2025-12-07T12:55:55.830397Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125615106511

The dechanneling length was measured to be 21 µm at 855 MeV, decreasing to 14 µm at 600 MeV and 9.4 µm at 300 MeV.

[ "Bent crystals with varying lengths were simulated", "Exponential decay fit: Nch(ℓ) = N0 exp(−ℓ/Ld)", "NaI(Tl) detector placed at L = 8.627 m" ]

0.85

medium

universal

physics

arxiv

2511.19807v1

https://arxiv.org/abs/2511.19807v1

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

b4930c1e6a4632d15fcc921e1068044b252236dd13e8877c726cb1b19818e5db

Extracted from ArXiv paper 2511.19807v1 (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": "2511.19807v1" }

science

WO-ARX-01

2025-12-07T12:56:15.106511Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125635560312

The bunch duration of relativistic electron beams is measured to be approximately 4 fs using momentum spectra measurements.

[ "Phys. Rev. Accel. Beams, 27, 2024.", "Sparc lab experiments", "Momentum spectra analysis" ]

0.85

medium

universal

physics

arxiv

2511.19807v1

https://arxiv.org/abs/2511.19807v1

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

2087adeaaef985dc270c141545996ba8349497b439b0a8911566479ba0f17f84

Extracted from ArXiv paper 2511.19807v1 (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": "2511.19807v1" }

science

WO-ARX-01

2025-12-07T12:56:35.560832Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125649938172

The SBC 10 kg liquid argon detector has a potential for world leading sensitivity to O(GeV/c^2) mass dark matter and to perform a high statistics reactor CEνNS measurement.

[ "SBC 10 kg liquid argon detector", "Calibration campaign with systematic uncertainties comparable to other recent bubble chamber calibrations", "Simulations at four thresholds from 80 to 400 eV" ]

0.85

high

universal

physics

arxiv

2511.19817v1

https://arxiv.org/abs/2511.19817v1

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

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Extracted from ArXiv paper 2511.19817v1 (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": "2511.19817v1" }

science

WO-ARX-01

2025-12-07T12:56:49.938172Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125718511797

The Kasen effect, a sudden brightening after a supernova explosion due to a red giant companion, is not observed in six normal SNIa, contradicting expectations.

[ "TESS full-frame data for 307 SNIa", "No prominent Kasen peaks detected in light curves", "Weak signals in residuals plots" ]

0.85

high

universal

physics

arxiv

2511.19948v1

https://arxiv.org/abs/2511.19948v1

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

d3a900e36e52121f6e9dc114fd396507c238fe53f30c114aa2b29d340e9435f2

Extracted from ArXiv paper 2511.19948v1 (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": "2511.19948v1" }

science

WO-ARX-01

2025-12-07T12:57:18.511797Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125740268662

Cross-section values for 𝜒0~2𝜒±~1, 𝜒0~2𝜒0~1, 𝜒0~1𝜒±~1, and 𝜒+~1𝜒−~1 production are measured as 5.3 ± 0.2 pb, 3.2 ± 0.1 pb, 5.5 ± 0.2 pb, and 2.9 ± 0.1 pb respectively, using ATLAS detector

[ "ATLAS detector", "Resummino 2.0.1 at NLO+NLL precision", "CTEQ6.6 [76] and MSTW2008nlo90cl [77] PDF sets" ]

0.85

medium

universal

physics

arxiv

2511.20042v1

https://arxiv.org/abs/2511.20042v1

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

e170c36a529885ec4aa0d58cec5e6c9848df335ec8c88e923f159d22033897ff

Extracted from ArXiv paper 2511.20042v1 (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": "2511.20042v1" }

science

WO-ARX-01

2025-12-07T12:57:40.268662Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125747052985

Low- pT lepton-track identification methods developed to distinguish leptons from hadrons and fake combinatorial tracks in the inner detector, with dedicated optimisations for electron-tracks and muon-tracks

[ "Tight Primary working point defined in Ref. [117]", "Preselected tracks with pT > 500 MeV and |η| < 2.5", "Low- pT lepton-track ID uses a fully connected deep neural network model with two 128-node hidden layers" ]

0.85

medium

universal

physics

arxiv

2511.20042v1

https://arxiv.org/abs/2511.20042v1

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

1ce441cf284e716355008d1b1a25e0c49d7138caf853af73724cdba2249511a4

Extracted from ArXiv paper 2511.20042v1 (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": "2511.20042v1" }

science

WO-ARX-01

2025-12-07T12:57:47.053496Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125817128006

Normalisation factors for Z+jets and diboson processes measured as 1.29 ± 0.01 and 1.4 ± 0.2, respectively

[ "ATLAS detector", "2022 LHC run data", "Normalisation factor for W±(→τ± hadντ)+jets processes: 1.37 ± 0.04" ]

0.85

medium

universal

physics

arxiv

2511.20042v1

https://arxiv.org/abs/2511.20042v1

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

7be6d816885db44fa429d0880f37c067f1ea08772a522c82cdfc4d005a580814

Extracted from ArXiv paper 2511.20042v1 (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": "2511.20042v1" }

science

WO-ARX-01

2025-12-07T12:58:17.128006Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125835610852

The ATLAS detector observes good agreement between data and predicted background event yields in validation regions, with deviations below 2σ.

[ "ATLAS detector", "14 TeV, 140 fb−1 collision data", "good agreement observed in all VRs for both displaced track and 1ℓ1T searches" ]

0.85

medium

universal

physics

arxiv

2511.20042v1

https://arxiv.org/abs/2511.20042v1

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

00247bdd11b30fae1da04ea9bb0fae1ba04c6df18daab4d9c1fcb9678d0440ec

Extracted from ArXiv paper 2511.20042v1 (chunk 24)

[ "experimental_physics", "measurement" ]

llama3.1:8b-instruct-q5_K_M

{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 24, "paper_id": "2511.20042v1" }

science

WO-ARX-01

2025-12-07T12:58:35.610852Z

arxiv

physics_recovered

arxiv_physics

w_20251207_125842287449

The ATLAS collaboration observed a significance of up to 5.8 sigma in the pNN-θ=4 GeV slice for SR-1ℓ1T.

[ "ATLAS detector, 13 TeV collision data", "Observed yield: 7 events", "Fitted SM background: 10.0 ± 2.4" ]

0.85

high

universal

physics

arxiv

2511.20042v1

https://arxiv.org/abs/2511.20042v1

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

fc1d79901d0c08cb7fdcd24d4242f59a43a4227b33a7cd91037a7409d0e9e248

Extracted from ArXiv paper 2511.20042v1 (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": "2511.20042v1" }

science

WO-ARX-01

2025-12-07T12:58:42.287449Z

arxiv

physics_recovered

arxiv_physics