On the Low Surface Magnetic Field Structure of Quark Stars

Details On the Low Surface Magnetic Field Structure of Quark Stars On the Low Surface Magnetic Field Structure of Quark Stars

2008-10-27

arxiv.org/abs/0810.4793v1

Astronomy and Astrophysics

Astrophysics

24 pages REVTEX, one .eps figure, psfig.sty is included

Scientific paper

Following some of the recent articles on hole super-conductivity and related phenomena by Hirsch \cite{H1,H2,H3}, a simple model is proposed to explain the observed low surface magnetic field of the expected quark stars. It is argued that the diamagnetic moments of the electrons circulating in the electro-sphere induce a magnetic field, which forces the existing quark star magnetic flux density to become dilute. We have also analysed the instability of normal-superconducting interface due to excess accumulation of magnetic flux lines, assuming an extremely slow growth of superconducting phase through a first order bubble nucleation type transition.

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