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Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 10 Dec 2006Embargo end date: 01 Jan 2006 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 653, pages 568-572 (issn: 0004-637X, eissn: 1538-4357,

Authors: Reisenegger, Andreas; Jofre, Paula; Fernandez, Rodrigo; Kantor, Elena;

doi: 10.1086/506601 , 10.48550/arxiv.astro-ph/0606322

arXiv: http://arxiv.org/abs/astro-ph/0606322

handle: 10533/178312 , 10533/178308

Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations

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Abstract

The electrostatic potential that keeps approximate charge neutrality in neutron star matter is self-consistently introduced into the formalism for rotochemical heating presented in a previous paper by Fernandez and Reisenegger. Although the new formalism is more rigorous, we show that its observable consequences are indistinguishable from those of the previous one, leaving the conclusions of the previous paper unchanged.

14 pages, including 4 eps figures. Accepted for publication in The Astrophysical Journal

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Keywords

Nuclear Theory (nucl-th), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology

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