Magnetic domain in magnetar-matters and soft gamma repeaters

Details Magnetic domain in magnetar-matters and soft gamma repeaters Magnetic domain in magnetar-matters and soft gamma repeaters

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..569s&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 569-571 (2001).

Astronomy and Astrophysics

Astrophysics

1

Magnetic And Electric Fields, Polarization Of Starlight, Neutron Stars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

Magnetars have been suggested as the site for the origin of observed soft gamma repeaters (SGRs). In this work we discuss the possibility that SGRs might be observational evidence for a magnetic phase separation in magnetars. We study magnetic domain formation as a new mechanism for SGRs in which magnetar-matter separates into two phases containing different flux densities. We use relativistic Hartree theory to estimate the densities at which there is an instability in magnetic domain formation for a given magnetic field. .

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