ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC

The Hartle-Thorne metric defines a reliable spacetime for most astrophysical purposes, for instance simulations of slowly rotating stars. Solving the Einstein field equations, we added terms of second order in the quadrupole moment to its post-linear version in order to compare it with solutions fou...

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Main Authors: FRANCISCO FRUTOS ALFARO, MICHAEL SOFFEL
Format: Article
Language:English
Published: Universidad de Costa Rica 2017-07-01
Series:Revista de Matemática: Teoría y Aplicaciones
Subjects:
Online Access:https://revistas.ucr.ac.cr/index.php/matematica/article/view/29856
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author FRANCISCO FRUTOS ALFARO
MICHAEL SOFFEL
author_facet FRANCISCO FRUTOS ALFARO
MICHAEL SOFFEL
author_sort FRANCISCO FRUTOS ALFARO
collection DOAJ
description The Hartle-Thorne metric defines a reliable spacetime for most astrophysical purposes, for instance simulations of slowly rotating stars. Solving the Einstein field equations, we added terms of second order in the quadrupole moment to its post-linear version in order to compare it with solutions found by Blanchet in the multi-polar post-Minkowskian framework. We first derived the extended Hartle-Thorne metric in harmonic coordinates and then showed agreement with the corresponding post-linear metric from Blanchet. We also found a coordinate transformation from the post-linear Erez- Rosen metric to our extended Hartle-Thorne spacetime. It is well known that the Hartle-Thorne solution can be smoothly matched with an interior perfect fluid solution with appropriate physical properties. A comparison among these solutions provides a validation of them. It is clear that in order to represent realistic solutions of self-gravitating (axially symmetric) matter distributions of perfect fluid, the quadrupole moment has to be included as a physical parameter.
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spelling doaj.art-37d6427718a74dc18b8e674d0e650c402023-08-02T04:21:12ZengUniversidad de Costa RicaRevista de Matemática: Teoría y Aplicaciones2215-33732017-07-0124223925510.15517/rmta.v24i2.2985625661ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRICFRANCISCO FRUTOS ALFARO0MICHAEL SOFFEL1School of Physics and Space Research Center, University of Costa Rica, San José, Costa RicaTechnical University Dresden and Lohrmann Observatory, Dresden, GermanyThe Hartle-Thorne metric defines a reliable spacetime for most astrophysical purposes, for instance simulations of slowly rotating stars. Solving the Einstein field equations, we added terms of second order in the quadrupole moment to its post-linear version in order to compare it with solutions found by Blanchet in the multi-polar post-Minkowskian framework. We first derived the extended Hartle-Thorne metric in harmonic coordinates and then showed agreement with the corresponding post-linear metric from Blanchet. We also found a coordinate transformation from the post-linear Erez- Rosen metric to our extended Hartle-Thorne spacetime. It is well known that the Hartle-Thorne solution can be smoothly matched with an interior perfect fluid solution with appropriate physical properties. A comparison among these solutions provides a validation of them. It is clear that in order to represent realistic solutions of self-gravitating (axially symmetric) matter distributions of perfect fluid, the quadrupole moment has to be included as a physical parameter.https://revistas.ucr.ac.cr/index.php/matematica/article/view/29856general relativitysolutions of Einstein’s equationsapproximation proceduresweak fields
spellingShingle FRANCISCO FRUTOS ALFARO
MICHAEL SOFFEL
ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
Revista de Matemática: Teoría y Aplicaciones
general relativity
solutions of Einstein’s equations
approximation procedures
weak fields
title ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
title_full ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
title_fullStr ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
title_full_unstemmed ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
title_short ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
title_sort on the post linear quadrupole quadrupole metric
topic general relativity
solutions of Einstein’s equations
approximation procedures
weak fields
url https://revistas.ucr.ac.cr/index.php/matematica/article/view/29856
work_keys_str_mv AT franciscofrutosalfaro onthepostlinearquadrupolequadrupolemetric
AT michaelsoffel onthepostlinearquadrupolequadrupolemetric