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Cited by 1,177

The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.

Equations of state for supernovae and compact stars

Open access
Oertel, M., Hempel, M., Klähn, T., Typel, S.·2017·Reviews of Modern Physics
DOI 10.1103/revmodphys.89.015007
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Abstract

What are the thermodynamic properties of matter at extreme densities, even exceeding nuclear matter density severely? How can we describe the composition of matter for such conditions, the resulting pressure, and the maximum mass of cold neutron stars? How is this affected by finite temperatures, as they occur in core collapse supernovae and in compact star mergers? This review addresses these points within the framework of constraints from experiments as well as astronomical observations.

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Metadata

Authors
Oertel, M., Hempel, M., Klähn, T., & Typel, S.
Venue
Reviews of Modern Physics
Publisher
American Physical Society (APS)
Published
2017-03-15
Volume
89
Issue
1
ISSN
  • 0034-6861 (ISSN-L)
  • 1539-0756
DOI
10.1103/revmodphys.89.015007
OpenAlex
W2531534365
Cited by
1,177
References
9
FWCI
53.10
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Equations of state for supernovae and compact stars. https://app.cochat.ai/papers/10.1103/revmodphys.89.015007
The paper
Oertel, M., Hempel, M., Klähn, T., & Typel, S. (2017). Equations of state for supernovae and compact stars. Reviews of Modern Physics. https://doi.org/10.1103/revmodphys.89.015007

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

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.