Expulsion of Magnetic Flux Lines from the Growing Superconducting Core of a Magnetized Quark Star
arXiv:hep-ph/9508384 · doi:10.1007/s10509-008-9745-3
Abstract
The expulsion of magnetic flux lines from a growing superconducting core of a quark star has been investigated. The idea of impurity diffusion in molten alloys and an identical mechanism of baryon number transport from hot quark-gluon-plasma phase to hadronic phase during quark-hadron phase transition in the early universe, micro-second after big bang has been used. The possibility of Mullins-Sekerka normal-superconducting interface instability has also been studied.
Thoroughly revised version. Accepted for Astrophysics & Space Science
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