On neutron stars and gravitation

From the variational principle for the total internal energy of a neutron star and some restrictions on the form of the metric coefficients, we have found equations of structure which are valid for every metric theory of gravitation. We also present some simple solutions of the structure equations t...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Castagnino, M.A., Lousto, C.O.
Formato: JOUR
Materias:
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03693554_v99_n2_p123_Castagnino
Aporte de:
id todo:paper_03693554_v99_n2_p123_Castagnino
record_format dspace
spelling todo:paper_03693554_v99_n2_p123_Castagnino2023-10-03T15:28:29Z On neutron stars and gravitation Castagnino, M.A. Lousto, C.O. PACS. 97.60.Jd. Neutron stars From the variational principle for the total internal energy of a neutron star and some restrictions on the form of the metric coefficients, we have found equations of structure which are valid for every metric theory of gravitation. We also present some simple solutions of the structure equations to find the maximum mass of a neutron star. Finally we study this problem using a post post-Newtonian parametrization. © 1987 Società Italiana di Fisica. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03693554_v99_n2_p123_Castagnino
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic PACS. 97.60.Jd. Neutron stars
spellingShingle PACS. 97.60.Jd. Neutron stars
Castagnino, M.A.
Lousto, C.O.
On neutron stars and gravitation
topic_facet PACS. 97.60.Jd. Neutron stars
description From the variational principle for the total internal energy of a neutron star and some restrictions on the form of the metric coefficients, we have found equations of structure which are valid for every metric theory of gravitation. We also present some simple solutions of the structure equations to find the maximum mass of a neutron star. Finally we study this problem using a post post-Newtonian parametrization. © 1987 Società Italiana di Fisica.
format JOUR
author Castagnino, M.A.
Lousto, C.O.
author_facet Castagnino, M.A.
Lousto, C.O.
author_sort Castagnino, M.A.
title On neutron stars and gravitation
title_short On neutron stars and gravitation
title_full On neutron stars and gravitation
title_fullStr On neutron stars and gravitation
title_full_unstemmed On neutron stars and gravitation
title_sort on neutron stars and gravitation
url http://hdl.handle.net/20.500.12110/paper_03693554_v99_n2_p123_Castagnino
work_keys_str_mv AT castagninoma onneutronstarsandgravitation
AT loustoco onneutronstarsandgravitation
_version_ 1782030140014854144