Magnetoemission of magnetar crust

Magnetoemission of magnetar crust

The magnetoemission of crusts of magnetars (ultramagnetized neutron stars) is considered as an origin of repeated soft gamma-ray bursts. It is shown that all observations of such bursts can be described and systematized on the basis of amodel of randomly jumping interacting moments that includes qua...

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Veröffentlicht in:Physics of atomic nuclei 2017-05, Vol.80 (3), p.558-561
Hauptverfasser: Kondratyev, V. N., Korovina, Yu. V.
Format: Artikel
Sprache:eng
Schlagworte:
Analysis
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Bursting
COSMIC GAMMA BURSTS
Crusts
DYNAMIC MAGNETIC FIELDS
Elementary Particles and Fields Theory
FLUCTUATIONS
Gamma ray bursts
Gamma rays
Magnetars
MAGNETIC MOMENTS
NEUTRON STARS
Neutrons
NUCLEAR MATTER
NUCLEAR PHYSICS AND RADIATION PHYSICS
Particle and Nuclear Physics
Physics
Physics and Astronomy
PULSARS
Telecommunications equipment
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Beschreibung
Zusammenfassung:The magnetoemission of crusts of magnetars (ultramagnetized neutron stars) is considered as an origin of repeated soft gamma-ray bursts. It is shown that all observations of such bursts can be described and systematized on the basis of amodel of randomly jumping interacting moments that includes quantum fluctuations and internuclear magnetic interaction in inhomogeneous crusty nuclear matter.
ISSN:1063-7788
1562-692X
DOI:10.1134/S1063778817030139