Bulletin of Taras Shevchenko National University of Kyiv. Astronomy, no. 51, p. 16-18 (2014)

SGR bursts due to magnetar crust magnetoemission

V. Kondratyev, Ph.D. in Phys. and Math. Science
Iu. Korovina, Associate Prof.
Taras Shevchenko National University of Kyiv
MIOE, Moscow, Russia

Abstract
Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultranamagnetized neutron stars). It isshown that all the observations of such bursts can be described and systematized within randomly jumping interacting moments model includingthe quantum fluctuations and the internuclear interaction in an inhomogeneous medium.

Keywords
Gamma-ray bursts, neutron stars, magnetars.

References
Kondratyev, V.N. 2002,JAERI Research-Series 2001-057 (JAERI-Prtss, Japan, 2002), 88, 221101
Mazets, E.P., Golentskii, S.V., Ilinskii, V.N.1979, Observations of a flaring X-ray pulsar in Dorado Nature (London), 282,587
Kondratyev, V.N. 2010, Bull.Univ.Kiev,SPM, 3, 31
Kondratyev, V.N.2012, Creation and transmutation of magnetized nuclei at explosively dense matter Eur. Phys. WC., 38, 17008
Kondratyev, V.N.2014, Explosivenucleosynthesis at strong magnetic field Eur. Phys. J. A, 50, 7
Kondratyev, V.N. 2010, Dynamics of magnetic nanoparticle assembly J. Phys. CS, 248, 012027
Gogus E.1999, Astrophys. J. Letters, 526, 93
Gogus E.2000, Astrophys. J. Letters, 532, 121

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