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Approximate input physics for stellar modelling

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Pols, O. R., Tout, C. A., Eggleton, P. P., Han, Z.·1995·Monthly Notices of the Royal Astronomical Society

Abstract

We present a simple and efficient, yet reasonably accurate, equation of state, which at the moderately low temperatures and high densities found in the interiors of stars less massive than the Sun is substantially more accurate than its predecessor by Eggleton, Faulkner & Flannery. Along with the most recently available values in tabular form of opacities, neutrino loss rates, and nuclear reaction rates for a selection of the most important reactions, this provides a convenient package of input physics for stellar modelling. We briefly discuss a few results obtained with the updated stellar evolution code.

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Metadata

Authors
Pols, O. R., Tout, C. A., Eggleton, P. P., & Han, Z.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1995-06-01
Volume
274
Issue
3
Pages
964-974
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2000079703
Cited by
580
References
0
FWCI
2.45
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Approximate input physics for stellar modelling. https://app.cochat.ai/papers/10.1093/mnras/274.3.964
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Pols, O. R., Tout, C. A., Eggleton, P. P., & Han, Z. (1995). Approximate input physics for stellar modelling. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/274.3.964

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.