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.
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Chakrabarty, S. Expulsion of magnetic flux lines from the growing superconducting core of a magnetised quark star. Astrophys Space Sci 314, 105–112 (2008). https://doi.org/10.1007/s10509-008-9745-3
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DOI: https://doi.org/10.1007/s10509-008-9745-3