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

نویسنده

  • Somenath Chakrabarty
چکیده

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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Expulsion of Magnetic Flux Lines from Growing Superconducting Core of a Quark Star and The Possibility of Mullins-Sekerka Interface Instability

The expulsion of magnetic flux lines from a growing superconducting core of a quark star has been investigated using the idea of impurity diffusion in molten alloys. The possibility of Mullins-Sekerka normal-superconducting interface instability has also been studied. PACS NO.:24.85+p, 97.60Jd, 74.20Hi, 64.70-p † Permanent Address

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تاریخ انتشار 2008