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A direct measurement of the 17O(α,γ)21Ne reaction in inverse kinematics and its impact on heavy element production

2019· article· en· W2970846207 on OpenAlexafffund
M.P. Taggart, C. Akers, A. M. Laird, U. Hager, C. Ruiz, D. A. Hutcheon, M. A. Bentley, James R. Brown, L. Buchmann, A. A. Chen, J. Chen, K. A. Chipps, A. Choplin, J.M. D’Auria, B. Davids, C. A. Davis, C. Aa. Diget, L. Erikson, J. Fallis, S. P. Fox, U. Frischknecht, Benjamin J. Fulton, N. Galinski, U. Greife, Raphaël Hirschi, Debra Howell, L. Martin, D. J. Mountford, A. St. J. Murphy, D. Ottewell, M. Pignatari, S. Reeve, G. Ruprecht, Sky Sjue, L. M. Veloce, M. Williams

Bibliographic record

VenuePhysics Letters B · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNuclear physics research studies
Canadian institutionsSimon Fraser UniversityMcMaster UniversityTRIUMF
FundersEuropean Research CouncilScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaMagyar Tudományos AkadémiaMinistry of Education, Culture, Sports, Science and TechnologyNational Science FoundationTRIUMFEuropean Cooperation in Science and TechnologyUniversity of HullColorado School of MinesSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of Energy
KeywordsNucleosynthesisPhysicsNuclear physicsNeutron captureNuclear reactionRecoilNuclear astrophysicsNeutronReaction rates-processr-processAtomic physicsChemistry

Abstract

fetched live from OpenAlex

During the slow neutron capture process in massive stars, reactions on light elements can both produce and absorb neutrons thereby influencing the final heavy element abundances. At low metallicities, the high neutron capture rate of 16O can inhibit s-process nucleosynthesis unless the neutrons are recycled via the 17O(α,n)20Ne reaction. The efficiency of this neutron recycling is determined by competition between the 17O(α,n)20Ne and 17O(α,γ)21Ne reactions. While some experimental data are available on the former reaction, no data exist for the radiative capture channel at the relevant astrophysical energies. The 17O(α,γ)21Ne reaction has been studied directly using the DRAGON recoil separator at the TRIUMF Laboratory. The reaction cross section has been determined at energies between 0.6 and 1.6 MeV Ecm, reaching into the Gamow window for core helium burning for the first time. Resonance strengths for resonances at 0.63, 0.721, 0.81 and 1.122 MeV Ecm have been extracted. The experimentally based reaction rate calculated represents a lower limit, but suggests that significant s-process nucleosynthesis occurs in low metallicity massive stars.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.143
Threshold uncertainty score0.422

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.025
GPT teacher head0.280
Teacher spread0.255 · 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 teacher head, 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".

Quick stats

Citations7
Published2019
Admission routes2
Has abstractyes

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