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- W3105255714 abstract "Fast radio bursts (FRBs) at cosmological distances still hold concealed physical origins. Previously Liu (2018) proposes a scenario that the collision between a neutron star (NS) and a white dwarf (WD) can be one of the progenitors of non-repeating FRBs and notices that the repeating FRBs can also be explained if a magnetar formed after such NS-WD merger. In this paper, we investigate this channel of magnetar formation in more detail. We propose that the NS-WD post-merger, after cooling and angular momentum redistribution, may collapse to either a black hole or a new NS or even remains as a hybrid WDNS, depending on the total mass of the NS and WD. In particular, the newly formed NS can be a magnetar if the core of the WD collapsed into the NS while large quantities of degenerate electrons of the WD compressed to the outer layers of the new NS. A strong magnetic field can be formed by the electrons and positive charges with different angular velocities induced by the differential rotation of the newborn magnetar. Such a magnetar can power the repeating FRBs by the magnetic reconnections due to the crustal movements or starquakes." @default.
- W3105255714 created "2020-11-23" @default.
- W3105255714 creator A5038789356 @default.
- W3105255714 date "2020-01-01" @default.
- W3105255714 modified "2023-09-25" @default.
- W3105255714 title "The Remnant of Neutron Star-White Dwarf Merger and the Repeating Fast Radio Bursts" @default.
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- W3105255714 doi "https://doi.org/10.4236/ijaa.2020.101003" @default.
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