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- W3086487019 abstract "ABSTRACT Pulsars undergoing crustquake release strain energy, which can be absorbed in a small region inside the inner crust of the star and excite the free superfluid neutrons therein. The scattering of these neutrons with the surrounding pinned vortices may unpin a large number of vortices and effectively reduce the pinning force on vortex lines. Such unpinning by neutron scattering can produce glitches for Crab-like pulsars and Vela pulsar of size in the range of ∼10−8–10−7 and ∼10−9–10−8, respectively. Although we discuss here the crustquake-initiated excitation, the proposal is very generic and equally applicable for any other sources, which can excite the free superfluid neutrons, or can be responsible for superfluid – normal phase transition of neutron superfluid in the inner crust of a pulsar." @default.
- W3086487019 created "2020-09-21" @default.
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- W3086487019 date "2020-09-21" @default.
- W3086487019 modified "2023-10-16" @default.
- W3086487019 title "Vortex unpinning due to crustquake-initiated neutron excitation and pulsar glitches" @default.
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- W3086487019 doi "https://doi.org/10.1093/mnras/staa2880" @default.
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