Autocorrelations In Pulsar Glitch Waiting Times And Sizes

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Autocorrelations in pulsar glitch waiting times and sizes

MNRAS 000,1{8(2019) Preprint 26 March 2021 Compiled using MNRAS LATEX style le v3.0 Autocorrelations in pulsar glitch waiting times and sizes J. B. Carlin,1 A. Melatos1;2 1School of Physics, University of Melbourne, Parkville, VIC 3010, Australia

1 2 arXiv:2105.13588v1 [astro-ph.HE] 28 May 2021

1 day ago correlations between glitch sizes and subsequent waiting times (ˆ+ & 0:8), which are largely absent from obser-vational data. It also predicts that either(i)the system stagnates, for Xth;max Xc, or(ii)there is an excess of the largest waiting times and sizes, corresponding to events which completely reset the system by unpinning all vortices.