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Physics of Particles and Nuclei, 2019
Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultramagnetized neutron stars). It is shown that all the observations of such bursts can be described and systematized within a randomly jumping interacting moments model including quantum fluctuations and internuclear interaction in an inhomogeneous medium.
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Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultramagnetized neutron stars). It is shown that all the observations of such bursts can be described and systematized within a randomly jumping interacting moments model including quantum fluctuations and internuclear interaction in an inhomogeneous medium.
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Rotating vector model for magnetars
Monthly Notices of the Royal Astronomical Society, 2021Hao Tong
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Modelling spin evolution of magnetars
Monthly Notices of the Royal Astronomical Society, 2021Thomas M Tauris
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Precession of magnetars: dynamical evolutions and modulations on polarized electromagnetic waves
Monthly Notices of the Royal Astronomical Society, 2022Yong Gao, Lijing Shao, Gregory Desvignes
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Testing the fossil field hypothesis: could strongly magnetized OB stars produce all known magnetars?
Monthly Notices of the Royal Astronomical Society, 2021Ekaterina I Makarenko, Andrei Igoshev
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Periodicity in recurrent fast radio bursts and the origin of ultralong period magnetars
Monthly Notices of the Royal Astronomical Society, 2020Paz Beniamini +2 more
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