Speakers
Prof.
David Sedrakian
(Yerevan State Unniversity)
Mekhak Hayrapetyan
(Yerevan State University)
Description
The generation of a magnetic field and its distribution inside a rotating strange star
are discussed. The difference between the angular velocities of the superfluid and
superconducting quark core and of the normal electron plasma increases because of
spin-down of the star and this leads to the generation of a magnetic field. The magnetic field distribution in a star is found for a stationary value of difference of angular velocities of these components. In all parts of the star this field is determined entirely by the total magnetic moment M of the star which can vary from 10^31-10^34 G·cm^3 for some models of compact stars.
Primary author
Prof.
David Sedrakian
(Yerevan State Unniversity)
Co-authors
Mr
Daniel Baghdasaryan
(Yerevan State University)
Mekhak Hayrapetyan
(Yerevan State University)
