G. H. Bordbar, A. Peivand
Published 2011-03-07Version 1
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.
Comments: 23 pages, 13 figures, 2 tables Res. Astron. Astrophys. (2011) in press
Journal: Research in Astron. Astrophys. 11 (2011) 851
Hot Spin Polarized Strange Quark Stars in the Presence of Magnetic Field using a density dependent bag constant
B fields in OB stars (BOB): Detection of a strong magnetic field in the O9.7 V star HD54879
Effect of a strong magnetic field on gravity-mode period spacings in red giant stars
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