Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity
arXiv:1110.6586 · doi:10.1007/s10509-011-0912-6
Abstract
We find that in general relativity slow down of the pulsar rotation due to the magnetodipolar radiation is more faster for the strange star with comparison to that for the neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evidence for the strange star existence and, thus, serve as a test for distinguishing it from the neutron star.
6 pages; Accepted for publication in Astrophysics and Space Science
References in corpus (8)
- Physics of Strongly Magnetized Neutron Stars
- Anisotropic Hydrodynamics, Bulk Viscosities and R-Modes of Strange Quark Stars with Strong Magnetic Fields
- The physics of neutron stars
- Sensitivity of the Moment of Inertia of Neutron Stars to the Equation of State of Neutron-Rich Matter
- Properties of Bare Strange Stars Associated with Surface Electric Fields
- General Relativistic Effect of Gravitomagnetic Charge on Pulsar Magnetosphere and Particle Acceleration in a Polar Cap
- Rotational parameters of strange stars in comparison with neutron stars
- Cold quark matter in astrophysics of compact stars
Cited by in corpus (5)
- Fast spinning strange stars: possible ways to constrain interacting quark matter parameters
- Strange quark matter in strong magnetic fields within a confining model
- Electromagnetic fields of slowly rotating magnetized compact stars in conformal gravity
- Nonlinear magnetic response of the magnetized vacuum to applied electric field
- Spindown of magnetars: Quantum Vacuum Friction?