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Record W2052795885 · doi:10.1103/physrevc.91.015803

Discovery of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>34</mml:mn><mml:mi>g</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msup><mml:mi>Cl</mml:mi><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mn>35</mml:mn></mml:msup><mml:mi>Ar</mml:mi></mml:mrow></mml:math>resonances activated at classical nova temperatures

2015· article· lv· W2052795885 on OpenAlexafffund
C. Fry, C. Wrede, S. Bishop, B. A. Brown, A. A. Chen, T. Faestermann, R. Hertenberger, A. Parikh, D. Pérez–Loureiro, H.-F. Wirth, A. Garcı́a, R. Ortez

Bibliographic record

VenuePhysical Review C · 2015
Typearticle
Languagelv
FieldPhysics and Astronomy
TopicNuclear physics research studies
Canadian institutionsMcMaster University
FundersNatural Sciences and Engineering Research Council of CanadaDeutsche ForschungsgemeinschaftNational Science Foundation
KeywordsPhysicsNucleosynthesisNeonAtomic physicsDipoleThermonuclear fusionExcited stateNuclear reactionWhite dwarfQuadrupoleResonance (particle physics)Nuclear physicsExcitationNuclear astrophysicsAstrophysicsArgonPlasmaStars

Abstract

fetched live from OpenAlex

Background: The thermonuclear ${}^{34g,m}\mathrm{Cl}{(p,\ensuremath{\gamma})}^{35}\mathrm{Ar}$ reaction rates are unknown due to a lack of experimental nuclear physics data. Uncertainties in these rates translate to uncertainties in $^{34}\mathrm{S}$ production in models of classical novae on oxygen-neon white dwarfs. $^{34}\mathrm{S}$ abundances have the potential to aid in the classification of presolar grains.Purpose: Determine resonance energies for the ${}^{34g,m}\mathrm{Cl}{(p,\ensuremath{\gamma})}^{35}\mathrm{Ar}$ reactions within the region of astrophysical interest for classical novae to a precision of a few keV as an essential first step toward constraining their thermonuclear reaction rates.Method: $^{35}\mathrm{Ar}$ excited states were populated by the ${}^{36}\mathrm{Ar}{(d,t)}^{35}\mathrm{Ar}$ reaction at $E(d)=22\phantom{\rule{0.28em}{0ex}}\mathrm{MeV}$ and reaction products were momentum analyzed by a high resolution quadrupole-dipole-dipole-dipole (Q3D) magnetic spectrograph.Results: Seventeen new $^{35}\mathrm{Ar}$ levels have been detected at a statistically significant level in the region ${E}_{x}\ensuremath{\approx}\phantom{\rule{0.28em}{0ex}}5.9--6.7\phantom{\rule{0.28em}{0ex}}\mathrm{MeV}$ $({E}_{r}<800\phantom{\rule{0.28em}{0ex}}\mathrm{keV})$ and their excitation energies have been determined to typical uncertainties of 3 keV. The uncertainties for five previously known levels have also been reduced substantially. The measured level density was compared to those calculated using the WBMB Hamiltonian within the $sd\text{\ensuremath{-}}pf$ model space.Conclusions: Most of the resonances in the region of astrophysical interest have likely been discovered and their energies have been determined, but the resonance strengths are still unknown, and experimentally constraining the ${}^{34g,m}\mathrm{Cl}{(p,\ensuremath{\gamma})}^{35}\mathrm{Ar}$ reaction rates will require further experiments.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.047
Threshold uncertainty score0.158

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0020.002
Research integrity0.0020.002
Insufficient payload (model declined to judge)0.0470.024

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.026
GPT teacher head0.274
Teacher spread0.248 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations13
Published2015
Admission routes2
Has abstractyes

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