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Stellar neutron capture reactions at low and high temperature

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Thomas Rauscher

Nuclear Theory · Submitted 23 Sep 2022

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim The determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning.

how it is stated · asserted 1.00 read the record →

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arXiv ID2209.11480 (version 2)
Pith IDRGI7W5LT, Pith's permanent record of this paper and its review
CitationThomas Rauscher. "Stellar neutron capture reactions at low and high temperature." arXiv:2209.11480 (2022). https://pith.science/paper/RGI7W5LT
Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,222 input tokens.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.30 · human participants 0.01 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

The determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning. The focus here is on astrophysical reaction rates for radiative neutron capture reactions. Relevant nucleosynthesis processes not only involve the s-process but also the i-, r- and $\gamma$-processes, which from the nuclear perspective mainly differ in the relative interaction energies of neutrons and nuclei, and in the nuclear level densities of the involved nuclei. Emphasis is put on the difference between reactions at low and high temperature. Possible complications in the prediction and measurement of these reaction rates are illustrated and the connection between theory and experiment is addressed.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning. background 1.00 0.07 0.06 asserted 1.00
s1 The focus here is on astrophysical reaction rates for radiative neutron capture reactions. contribution 0.65 0.20 0.05 asserted 0.94
s2 Relevant nucleosynthesis processes not only involve the s-process but also the i-, r- and $\gamma$-processes, which from the nuclear perspective mainly differ in the relative interaction energies of neutrons and nuclei, and in the nuclear level densities of the involved nuclei. background 1.00 0.06 0.07 asserted 1.00
s3 Emphasis is put on the difference between reactions at low and high temperature. contribution 0.93 0.19 0.10 asserted 0.78
s4 Possible complications in the prediction and measurement of these reaction rates are illustrated and the connection between theory and experiment is addressed. contribution 0.94 0.30 0.07 asserted 0.57

What kind of paper the classifier reports this is: review 1.00 · evidence from argument 0.67.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

The determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning. The focus here is on astrophysical reaction rates for radiative neutron capture reactions. Relevant nucleosynthesis processes not only involve the s-process but also the i-, r- and $\gamma$-processes, which from the nuclear perspective mainly differ in the relative interaction energies of neutrons and nuclei, and in the nuclear level densities of the involved nuclei. Emphasis is put on the difference between reactions at low and high temperature. Possible complications in the prediction and measurement of these reaction rates are illustrated and the connection between theory and experiment is addressed.

Human review

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How the literature uses it

1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

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