On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars

ABSTRACT:Whether analytic exact vacuum(electrovacuum) solutions of the Einstein(Einstein-Maxwell) field equations can accurately describe or not the exterior spacetime of compact stars remains still an interesting open question in Relativistic Astrophysics. As an attempt to establish their level of...

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Autores:
Pachón Contreras, Leonardo Augusto
Rueda Hernández, Jorge Armando
Valenzuela Toledo, Cesar Alonso
Tipo de recurso:
Article of investigation
Fecha de publicación:
2012
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/35226
Acceso en línea:
https://hdl.handle.net/10495/35226
Palabra clave:
Cosmología cuántica
Quantum Cosmology
Astrofísica
Astrophysics
Ecuaciones de Maxwell
Maxwell equations
Agujeros negros (astronomía)
Black holes (astronomy)
Mecánica celeste
Mechanics, celestial
Estrrellas
Stars
Relatividad general (física)
General relativity (Physics)
http://id.loc.gov/authorities/subjects/sh2005001325
Rights
openAccess
License
http://creativecommons.org/licenses/by/2.5/co/
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dc.title.spa.fl_str_mv On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
title On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
spellingShingle On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
Cosmología cuántica
Quantum Cosmology
Astrofísica
Astrophysics
Ecuaciones de Maxwell
Maxwell equations
Agujeros negros (astronomía)
Black holes (astronomy)
Mecánica celeste
Mechanics, celestial
Estrrellas
Stars
Relatividad general (física)
General relativity (Physics)
http://id.loc.gov/authorities/subjects/sh2005001325
title_short On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
title_full On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
title_fullStr On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
title_full_unstemmed On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
title_sort On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
dc.creator.fl_str_mv Pachón Contreras, Leonardo Augusto
Rueda Hernández, Jorge Armando
Valenzuela Toledo, Cesar Alonso
dc.contributor.author.none.fl_str_mv Pachón Contreras, Leonardo Augusto
Rueda Hernández, Jorge Armando
Valenzuela Toledo, Cesar Alonso
dc.contributor.researchgroup.spa.fl_str_mv Grupo de Física Atómica y Molecular
dc.subject.lcsh.none.fl_str_mv Cosmología cuántica
Quantum Cosmology
topic Cosmología cuántica
Quantum Cosmology
Astrofísica
Astrophysics
Ecuaciones de Maxwell
Maxwell equations
Agujeros negros (astronomía)
Black holes (astronomy)
Mecánica celeste
Mechanics, celestial
Estrrellas
Stars
Relatividad general (física)
General relativity (Physics)
http://id.loc.gov/authorities/subjects/sh2005001325
dc.subject.lemb.none.fl_str_mv Astrofísica
Astrophysics
Ecuaciones de Maxwell
Maxwell equations
Agujeros negros (astronomía)
Black holes (astronomy)
Mecánica celeste
Mechanics, celestial
Estrrellas
Stars
Relatividad general (física)
General relativity (Physics)
dc.subject.lcshuri.none.fl_str_mv http://id.loc.gov/authorities/subjects/sh2005001325
description ABSTRACT:Whether analytic exact vacuum(electrovacuum) solutions of the Einstein(Einstein-Maxwell) field equations can accurately describe or not the exterior spacetime of compact stars remains still an interesting open question in Relativistic Astrophysics. As an attempt to establish their level of accuracy, the radii of the Innermost Stable Circular Orbits (ISCOs) of test particles given by analytic exterior spacetime geometries have been compared with the ones given by numerical solutions for neutron stars (NSs) obeying a realistic equation of state (EoS). It has been so shown that the six-parametric solution of Pach´on, Rueda, and Sanabria (2006) (hereafter PRS) is more accurate to describe the NS ISCO radii than other analytic models. We propose here an additional test of accuracy for analytic exterior geometries based on the comparison of orbital frequencies of neutral test particles. We compute the Keplerian, frame-dragging, as well as the precession and oscillation frequencies of the radial and vertical motions of neutral test particles for the Kerr and PRS geometries; then we compare them with the numerical values obtained by Morsink and Stella (1999) for realistic NSs. We identify the role of highorder multipole moments such as the mass quadrupole and current octupole in the determination of the orbital frequencies especially in the rapid rotation regime. The results of this work are relevant to cast a separatrix between black hole (BH) and NS signatures as well as probe the nuclear matter EoS and NS parameters from the Quasi-Periodic Oscillations (QPOs) observed in Low Mass X-Ray Binaries.
publishDate 2012
dc.date.issued.none.fl_str_mv 2012
dc.date.accessioned.none.fl_str_mv 2023-06-01T15:01:18Z
dc.date.available.none.fl_str_mv 2023-06-01T15:01:18Z
dc.type.spa.fl_str_mv Artículo de investigación
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dc.identifier.issn.none.fl_str_mv 0004-637X
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10495/35226
dc.identifier.doi.none.fl_str_mv 10.1088/0004-637X/756/1/82
dc.identifier.eissn.none.fl_str_mv 1538-4357
identifier_str_mv 0004-637X
10.1088/0004-637X/756/1/82
1538-4357
url https://hdl.handle.net/10495/35226
dc.language.iso.spa.fl_str_mv eng
language eng
dc.relation.ispartofjournalabbrev.spa.fl_str_mv Astrophys. J.
dc.relation.citationendpage.spa.fl_str_mv 14
dc.relation.citationissue.spa.fl_str_mv 1
dc.relation.citationstartpage.spa.fl_str_mv 1
dc.relation.citationvolume.spa.fl_str_mv 756
dc.relation.ispartofjournal.spa.fl_str_mv Astrophysical Journal
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dc.format.extent.spa.fl_str_mv 14
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dc.publisher.spa.fl_str_mv Institute of Physics Publishing (IOP)
American Astronomical Society
dc.publisher.place.spa.fl_str_mv Chicago, Estados Unidos
institution Universidad de Antioquia
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spelling Pachón Contreras, Leonardo AugustoRueda Hernández, Jorge ArmandoValenzuela Toledo, Cesar AlonsoGrupo de Física Atómica y Molecular2023-06-01T15:01:18Z2023-06-01T15:01:18Z20120004-637Xhttps://hdl.handle.net/10495/3522610.1088/0004-637X/756/1/821538-4357ABSTRACT:Whether analytic exact vacuum(electrovacuum) solutions of the Einstein(Einstein-Maxwell) field equations can accurately describe or not the exterior spacetime of compact stars remains still an interesting open question in Relativistic Astrophysics. As an attempt to establish their level of accuracy, the radii of the Innermost Stable Circular Orbits (ISCOs) of test particles given by analytic exterior spacetime geometries have been compared with the ones given by numerical solutions for neutron stars (NSs) obeying a realistic equation of state (EoS). It has been so shown that the six-parametric solution of Pach´on, Rueda, and Sanabria (2006) (hereafter PRS) is more accurate to describe the NS ISCO radii than other analytic models. We propose here an additional test of accuracy for analytic exterior geometries based on the comparison of orbital frequencies of neutral test particles. We compute the Keplerian, frame-dragging, as well as the precession and oscillation frequencies of the radial and vertical motions of neutral test particles for the Kerr and PRS geometries; then we compare them with the numerical values obtained by Morsink and Stella (1999) for realistic NSs. We identify the role of highorder multipole moments such as the mass quadrupole and current octupole in the determination of the orbital frequencies especially in the rapid rotation regime. The results of this work are relevant to cast a separatrix between black hole (BH) and NS signatures as well as probe the nuclear matter EoS and NS parameters from the Quasi-Periodic Oscillations (QPOs) observed in Low Mass X-Ray Binaries.COL000844114application/pdfengInstitute of Physics Publishing (IOP)American Astronomical SocietyChicago, Estados Unidoshttp://creativecommons.org/licenses/by/2.5/co/https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Cosmología cuánticaQuantum CosmologyAstrofísicaAstrophysicsEcuaciones de MaxwellMaxwell equationsAgujeros negros (astronomía)Black holes (astronomy)Mecánica celesteMechanics, celestialEstrrellasStarsRelatividad general (física)General relativity (Physics)http://id.loc.gov/authorities/subjects/sh2005001325On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact starsArtículo de investigaciónhttp://purl.org/coar/resource_type/c_2df8fbb1https://purl.org/redcol/resource_type/ARThttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionAstrophys. 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