Critical mass, moment of inertia and universal relations of rapidly rotating neutron stars with exotic matter
arXiv:1704.07113 · doi:10.1142/S0218271817501279
Abstract
We calculate moment of inertia of neutron star with different exotic constituents such as hyperons and (anti)kaon condensates and study its variation with mass and spin frequency. The sets of equation of state, generated within the framework of relativistic mean field model with density-dependent couplings are adopted for the purpose. We follow the quasi-stationary evolution of rotating stars along the constant rest mass sequences, that varies considerably with different constituents in the equation of state. We also explore the universal relations associated with some of the normalised properties, such as critical mass and moment of inertia for specific EoS or as a matter of fact constituents of the dense matter. Deviations in the universal relations for moment of inertia are observed at higher compactness. This study presents important results concerning the properties of neutron stars, that could be observationally verified in the near future using Square Kilometer Array telescope.
16 figures
References in corpus (12)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Equations of state for supernovae and compact stars
- Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
- Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
- Relativistic model for nuclear matter and atomic nuclei with momentum-dependent self-energies
- Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
- Constraining hypernuclear density functional with -hypernuclei and compact stars
- Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
- Rotating proto-neutron stars: spin evolution, maximum mass and I-Love-Q relations
- Phase transitions in rotating neutron stars cores: back bending, stability, corequakes and pulsar timing
- Massive Neutron Stars with Antikaon Condensates in a Density Dependent Hadron Field Theory
Cited by in corpus (9)
- Heavy Baryons in Compact Stars
- Inferring neutron star properties from GW170817 with universal relations
- Universal relations for differentially rotating relativistic stars at the threshold to collapse
- Universal relations for rapidly rotating cold and hot hybrid star
- Moment of inertia, quadrupole moment, Love number of neutron star and their relations with strange matter equations of state
- Effects of hadron-quark phase transition on properties of Neutron Stars
- Universal Relations For Generic Family Of Neutron Star Equations Of State
- Properties of rapidly rotating hot neutron stars with antikaon condensates at constant entropy per baryon
- Insights Into Neutron Stars From Gravitational Redshifts and Universal Relations