General Relativistic effects on the conversion of nuclear to two-flavour quark matter in compact stars
arXiv:0707.3677 · doi:10.1103/PhysRevC.76.052801
Abstract
We investigate the General Relativistic (GR) effects on the conversion from nuclear to two-flavour quark matter in compact stars, both static as well as rotating. We find that GR effects lead to qualitative differences in rotating stars, indicating the inadequacy of non-relativistic (NR) or even Special Relativistic (SR) treatments for these cases.
arXiv comment4 pages, 4 figures
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- Effects of Onset of Phase Transition on Binary Neutron Star Mergers
- Spin-down induced quark-hadron phase transition in cold isolated neutron stars
- General Relativistic effect on the energy deposition rate for neutrino pair annihilation above the equatorial plane along the symmetry axis near a rotating neutron star
- Multimessenger signal from phase transition of neutron star to quark star
- Maximum mass of hybrid star formed via shock induced phase transition in cold neutron stars
- Solving relativistic hydrodynamic equation in presence of magnetic field for phase transition in a neutron star
- Formation of a magnetized hybrid star with a purely toroidal field from phase-transition-induced collapse
- Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
- Magnetic field inhibits the conversion of neutron stars to quark stars
- Converting Neutron Stars into Strange Stars: Instanton Model