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...
- 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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- Rights
- openAccess
- License
- Atribución-NoComercial-SinDerivadas 4.0 Internacional