Rotating compact objects with magnetic fields
arXiv:astro-ph/9805146 · doi:10.1088/0264-9381/15/10/016
Abstract
We consider here the structure of rotating compact objects endowed with a magnetic field in general relativity as models of pulsars. We discuss first the structure of rotating stars in the framework of Hartle taking different realistic equations of state and study their effects on bulk properties of the star. We consider the possibilty of rotating stars with a quark matter core. We further analyse the structure of the magnetic field in the interior of the star as affected by different equations of state as well as due to rotation.
Latex file, 27pages including 10 figures
References in corpus (1)
Cited by in corpus (11)
- Rotating Stars in Relativity
- General Relativistic Electromagnetic Fields of a Slowly Rotating Magnetized Neutron Star. I. Formulation of the equations
- Torsional Oscillations of Magnetized Relativistic Stars
- Magnetic Fields of Spherical Compact Stars in Braneworld
- On attributes of a Rotating Neutron star with a Hyperon core
- Bulk viscosity in hyperonic star and r-mode instability
- General Relativistic Electromagnetic Fields of a Slowly Rotating Magnetized Neutron Star. II. Solution of the Induction Equations
- Electromagnetic Fields of Slowly Rotating Compact Magnetized Stars in Braneworld
- Magnetic Field of a Compact Spherical Star under f(R,T) Gravity
- Gravitomagnetic Effects on Collective Plasma Oscillations in Compact Stars
- Thermal field theories coupled to curved spacetime