Innermost stable circular orbits and epicyclic frequencies around a magnetized neutron star

A full-relativistic approach is used to compute the radius of the innermost stable circular orbit (ISCO), the Keplerian, frame-dragging, precession and oscillation frequencies of the radial and vertical motions of neutral test particles orbiting the equatorial plane of a magnetized neutron star. The...

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Autores:
Tipo de recurso:
article
Fecha de publicación:
2013
Institución:
Pontificia Universidad Javeriana
Repositorio:
Repositorio Universidad Javeriana
Idioma:
eng
OAI Identifier:
oai:repository.javeriana.edu.co:10554/31274
Acceso en línea:
http://revistas.javeriana.edu.co/index.php/scientarium/article/view/5582
http://hdl.handle.net/10554/31274
Palabra clave:
Physics
Relativistic precession frequencies; Innermost stable circular orbits; Neutron stars.
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