Young neutron stars with soft gamma ray emission and anomalous X-ray pulsar [HEAP]

http://arxiv.org/abs/1702.08353


The observational properties of Soft Gamma Repeaters and Ano\-malous X-ray Pulsars (SGR/AXP) indicate to necessity of the energy source different from a rotational energy of a neutron star. The model, where the source of the energy is connected with a magnetic field dissipation in a highly magnetized neutron star (magnetar) is analyzed. Some observational inconsistencies are indicated for this interpretation. The alternative energy source, connected with the nuclear energy of superheavy nuclei stored in the nonequilibrium layer of low mass neutron star is discussed.

Read this paper on arXiv…

G. Bisnovatyi-Kogan
Tue, 28 Feb 17
47/69

Comments: 29 pages, 13 figures, Springer International Publishing Switzerland 2016 A.W. Alsabti, P. Murdin (eds.), Handbook of Supernovae

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