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...
- 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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http://purl.org/coar/resource_type/c_2df8fbb1 |
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http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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info:eu-repo/semantics/article |
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info:eu-repo/semantics/publishedVersion |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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publishedVersion |
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0004-637X |
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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. |
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14 |
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1 |
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1 |
| dc.relation.citationvolume.spa.fl_str_mv |
756 |
| dc.relation.ispartofjournal.spa.fl_str_mv |
Astrophysical Journal |
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http://creativecommons.org/licenses/by/2.5/co/ |
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14 |
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application/pdf |
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Institute of Physics Publishing (IOP) American Astronomical Society |
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Chicago, Estados Unidos |
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Universidad de Antioquia |
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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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