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- W2589577059 abstract "The observational properties of soft gamma repeaters and anomalous X-ray pulsars (SGR/AXP) indicate that an energy source is necessary additional to the rotational energy of a neutron star. A current model involving magnetic field dissipation in a highly magnetised neutron star (magnetar) is analysed. Some observational inconsistencies are indicated for this interpretation. Slow rotating neutron stars with very high magnetic fields have been discovered, which do not show any features of SGR, and behave as normal radio pulsars. There are SGR/AXP in which estimates of magnetic field strength, made in the same way as in other SGR, give an upper limit consistent with the average magnetic field of radio pulsars. An alternative energy source, connected with the nuclear energy of superheavy nuclei stored in the nonequilibrium layer of a low-mass neutron stars is discussed. The losses of rotational energy, observed in SGR/AXP are connected with a magnetised stellar wind, induced by bursting events near the neutron star surface." @default.
- W2589577059 created "2017-03-03" @default.
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- W2589577059 date "2017-01-01" @default.
- W2589577059 modified "2023-09-27" @default.
- W2589577059 title "Young Neutron Stars with Soft Gamma Ray Emission and Anomalous X-Ray Pulsars" @default.
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- W2589577059 doi "https://doi.org/10.1007/978-3-319-21846-5_70" @default.
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