Hot Spin Polarized Strange Quark Stars in the Presence of Magnetic Field using a density dependent bag constant

Abstract

The effect of magnetic field on the structure properties of hot spin polarized strange quark stars has been investigated. For this purpose, we use the MIT bag model with a density dependent bag constant to calculate the thermodynamic properties of spin polarized strange quark matter such as energy and equation of state. We see that the energy and equation of state of strange quark matter changes significantly in a strong magnetic field. Finally, using our equation of state, we compute the structure of spin polarized strange quark star at different temperatures and magnetic fields.

Astrophysics 57 (2014) in press. 24 pages, 3 tables, 10 figures

References in corpus (4)

• Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method
• Lowest Order Constrained Variational Calculation of the Polarized Nuclear Matter with the Modern $A{V}_{18}$ Potential
• Lowest order constrained variational calculation of polarized neutron matter at finite temperature
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Cited by in corpus (6)

• Constraints on Density Dependent MIT Bag Model Parameters for Quark and Hybrid Stars
• Influence of strong magnetic field on the structure properties of strange quark stars
• Proto-Strange Quark Star Structure
• The structure of cold neutron star with a quark core within the MIT and NJL models
• Gravitational Lensing in a Model of Nonlinear Electrodynamics: The case for electrically and magnetically charged compact objects
• Structure of hot strange quark stars: an NJL model approach at finite temperature