Magnetic Field of Neutron Stars with a Quark Core View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2018-12

AUTHORS

D. M. Sedrakian, M. V. Hayrapetyan

ABSTRACT

The mechanism for magnetic field generation by hybrid neutron stars containing a 2SC quark phase is examined. It is assumed that S-vortices with quantized angular momentum develop in the superconducting quark fluid. Entrainment of the charged quark fluid in a superfluid motion around the S-vortex leads to the development of currents that generate a magnetic field. It is shown that S-vortices have a magnetic structure in the form of a cluster of Abrikosov magnetic vortices with quantized magnetic flux. The distribution of the magnetic induction in the quark core of neutron stars is also studied. More... »

PAGES

499-510

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10511-018-9554-5

DOI

http://dx.doi.org/10.1007/s10511-018-9554-5

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1107989268


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