Expulsion of Magnetic Flux Lines from the Growing Superconducting Core of a Magnetized Quark Star

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dc.creatorChakrabarty, Somenath
dc.date1995-08-25
dc.date2008-01-22
dc.date.accessioned2026-07-07T11:35:11Z
dc.date.available2026-07-07T11:35:11Z
dc.descriptionThe 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.
dc.descriptionThoroughly revised version. Accepted for Astrophysics & Space Science
dc.identifierhttps://arxiv.org/abs/hep-ph/9508384
dc.identifierhttp://arxiv.org/abs/hep-ph/9508384
dc.identifierAstrophys.SpaceSci.314:105-112,2008
dc.identifierdoi:10.1007/s10509-008-9745-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198508
dc.subjectHigh Energy Physics - Phenomenology
dc.titleExpulsion of Magnetic Flux Lines from the Growing Superconducting Core of a Magnetized Quark Star
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