Post-newtonian approximation of the spherical shell dynamics

Post-Newtonian approximation is used to find the motion equation of Spherically Symmetric radiating shell, moving in a central gravitational potential: the obtained equation coincides with the exact one, expanded up to the post-Newtonian order.

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Detalles Bibliográficos
Autores principales: Castagnino, M.A., Neira, L.P.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/141975
Aporte de:
id I19-R120-10915-141975
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Castagnino, M.A.
Neira, L.P.
Post-newtonian approximation of the spherical shell dynamics
topic_facet Astronomía
Galaxia
description Post-Newtonian approximation is used to find the motion equation of Spherically Symmetric radiating shell, moving in a central gravitational potential: the obtained equation coincides with the exact one, expanded up to the post-Newtonian order.
format Articulo
Comunicacion
author Castagnino, M.A.
Neira, L.P.
author_facet Castagnino, M.A.
Neira, L.P.
author_sort Castagnino, M.A.
title Post-newtonian approximation of the spherical shell dynamics
title_short Post-newtonian approximation of the spherical shell dynamics
title_full Post-newtonian approximation of the spherical shell dynamics
title_fullStr Post-newtonian approximation of the spherical shell dynamics
title_full_unstemmed Post-newtonian approximation of the spherical shell dynamics
title_sort post-newtonian approximation of the spherical shell dynamics
publishDate 1988
url http://sedici.unlp.edu.ar/handle/10915/141975
work_keys_str_mv AT castagninoma postnewtonianapproximationofthesphericalshelldynamics
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bdutipo_str Repositorios
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