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Cited by 1,398

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

The Physics of Neutron Stars

Open access
Lattimer, J. M., Prakash, M.·2004·Science

Abstract

Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide connections among nuclear physics, particle physics, and astrophysics. Neutron stars may exhibit conditions and phenomena not observed elsewhere, such as hyperon-dominated matter, deconfined quark matter, superfluidity and superconductivity with critical temperatures near 10 10 kelvin, opaqueness to neutrinos, and magnetic fields in excess of 10 13 Gauss. Here, we describe the formation, structure, internal composition, and evolution of neutron stars. Observations that include studies of pulsars in binary systems, thermal emission from isolated neutron stars, glitches from pulsars, and quasi-periodic oscillations from accreting neutron stars provide information about neutron star masses, radii, temperatures, ages, and internal compositions.

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Crossref · 10.1126/science.1090720

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Metadata

Authors
Lattimer, J. M., & Prakash, M.
Venue
Science
Published
2004-04-23
Volume
304
Issue
5670
Pages
536-542
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2162076236
Cited by
1,398
References
1
FWCI
27.96
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Physics of Neutron Stars. https://app.cochat.ai/papers/10.1126/science.1090720
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Lattimer, J. M., & Prakash, M. (2004). The Physics of Neutron Stars. Science. https://doi.org/10.1126/science.1090720

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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.