Computation of the structure of magnetized strange quark star
G. H. Bordbar, A. Peivand
TL;DR
This paper investigates the effects of strong magnetic fields on the properties and structure of strange quark stars, revealing that magnetic polarization results in a stiffer equation of state and more stable star configurations.
Contribution
It introduces a detailed calculation of spin polarized strange quark matter and star structure under magnetic fields using the MIT bag model, highlighting the impact of polarization.
Findings
Magnetic fields make the equation of state of SQM stiffer.
Spin polarization enhances the stability of strange quark stars.
Magnetic effects lead to observable differences in star structure.
Abstract
In this work, we have calculated some properties of the spin polarized strange quark matter (SQM) in a strong magnetic field at zero temperature using the MIT bag model. We have shown that the equation of state of spin polarized SQM is stiffer than that of the unpolarized case. We have also computed the structure properties of the spin polarized strange quark star (SQS) and have found that the presence of magnetic field leads to a more stable SQS compared to the unpolarized SQS.
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