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2018MNRAS.473..621A - Mon. Not. R. Astron. Soc., 473, 621-624 (2018/January-1)

Minimum glitch of the Crab pulsar and the crustquake as a trigger mechanism.


Abstract (from CDS):

We discuss the minimum glitch size of Crab observed by Espinoza et al. (2014). Modelling the crustquake as a trigger mechanism, we estimate the size of the broken plate. The plate size obtained, D ∼ 100 m is comparable to plate size estimates for PSR J1119-6127. The plate size naturally leads to an estimate of the number of unpinned vortices involved in the glitch, N ∼ 1013. This number is of the same order in all Crab and Vela pulsar glitches. The minimum glitch relates the constancy of all these numbers among different pulsars to the basic plate size involved in crust breaking. This in turn depends on the critical strain angle θcr of the Coulomb lattice in the neutron star crust. The minimum glitch size implies θcr ∼ 10–1 in agreement with theoretical and computational estimates.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): dense matter - stars: neutron - pulsars: general - pulsars: individual: Crab - pulsars: individual: Crab

Simbad objects: 6

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