http://arxiv.org/abs/1808.01086
We solve the Taub adiabat equation to study the phase transition of a neutron star to quark star. We show that the PT from NS to QS is not always possible and sometimes the PT could lead to a Qs which is much smaller than the original NS. We derive the magnetized Taub adiabat equation from the magnetic field induced RH equations and solved it to show that the magnetic field of the resultant QS after the PT depends strongly on the tilt of the magnetic axis of the original NS.
R. Mallick and M. Irfan
Mon, 6 Aug 18
10/33
Comments: 5 pages, 5 figures
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