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The Equation of State of Neutron Star Matter in Strong Magnetic Fields

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Broderick, A., Prakash, M., Lattimer, J. M.·2000·The Astrophysical Journal

Abstract

We study the effects of very strong magnetic fields on the equation of state (EOS) in multicomponent, interacting matter by developing a covariant description for the inclusion of the anomalous magnetic moments of nucleons. For the description of neutron star matter, we employ a field-theoretical approach, which permits the study of several models that differ in their behavior at high density. Effects of Landau quantization in ultrastrong magnetic fields ( B > 10 14 G) lead to a reduction in the electron chemical potential and a substantial increase in the proton fraction. We find the generic result for B > 10 18 G that the softening of the EOS caused by Landau quantization is overwhelmed by stiffening due to the incorporation of the anomalous magnetic moments of the nucleons. In addition, the neutrons become completely spin polarized. The inclusion of ultrastrong magnetic fields leads to a dramatic increase in the proton fraction, with consequences for the direct Urca process and neutron star cooling. The magnetization of the matter never appears to become very large, as the value of | H / B | never deviates from unity by more than a few percent. Our findings have implications for the structure of neutron stars in the presence of large frozen-in magnetic fields.

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Metadata

Authors
Broderick, A., Prakash, M., & Lattimer, J. M.
Venue
The Astrophysical Journal
Published
2000-07
Volume
537
Issue
1
Pages
351-367
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2039300833
Cited by
338
References
23
FWCI
4.94
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The Equation of State of Neutron Star Matter in Strong Magnetic Fields. https://app.cochat.ai/papers/10.1086/309010
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Broderick, A., Prakash, M., & Lattimer, J. M. (2000). The Equation of State of Neutron Star Matter in Strong Magnetic Fields. The Astrophysical Journal. https://doi.org/10.1086/309010

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