Generation and Distribution of a Magnetic Field in Superconducting Strange Stars View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2015-12

AUTHORS

D. M. Sedrakian, M. V. Hayrapetyan, D. S. Baghdasaryan

ABSTRACT

Generation of a magnetic field and its distribution are considered within a rotating strange quark star with a crust. It is shown how, over time, a differential rotation is established between the superfluid and superconducting quark core and normal electron plasma, which leads to the generation of magnetic field. The magnetic field at the surface of a strange star may attain values of 1011–1015 G, depending on the star model. It is suggested that magnetars may be manifestations of strange stars, the cores of which rotate much faster than the observable part, i.e., the crust. More... »

PAGES

536-549

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10511-015-9406-5

DOI

http://dx.doi.org/10.1007/s10511-015-9406-5

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1002581460


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