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

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dc.creatorReisenegger, Andreas
dc.creatorJofre, Paula
dc.creatorFernandez, Rodrigo
dc.creatorKantor, Elena
dc.date2006-06-13
dc.date.accessioned2026-07-07T10:39:17Z
dc.date.available2026-07-07T10:39:17Z
dc.descriptionThe 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.
dc.description14 pages, including 4 eps figures. Accepted for publication in The Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0606322
dc.identifierhttp://arxiv.org/abs/astro-ph/0606322
dc.identifierAstrophys.J.653:568-572,2006
dc.identifierdoi:10.1086/506601
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180973
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectNuclear Theory
dc.titleRotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations
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