On torque reversal during delayed spin up glitch of SGR 1935+2154
Wei-Hua Wang, Ming-Yu Ge, Xi Huang, Xiao-Ping Zheng

TL;DR
This paper reports the first observed torque reversal during a delayed spin-up glitch in the magnetar SGR 1935+2154, suggesting a common physical origin with similar phenomena in other pulsars and implications for neutron star physics.
Contribution
It presents the first detection of a delayed spin-up and torque reversal in SGR 1935+2154, linking it to similar phenomena in the Crab pulsar and proposing a unified physical origin.
Findings
First unambiguous detection of delayed spin-up in a magnetar
Torque reversal observed within 8 days of glitch
Similar positive torque values as in Crab pulsar
Abstract
Ge et al. reported a peculiar large glitch observed from SGR 1935 recently~\citep{2022arXiv221103246G}. % Interestingly, this glitch occurred about before FRB 200428, accompanied by a delayed spin up (DSU) process with a timescale of . % This DSU is the first one detected from magnetars unambiguously, previously, DSU has only been detected from large glitches of the young Crab pulsar. % Strikingly, this DSU even resulted in torque reversal, i.e., the spin down state of SGR 1935 was turned into a spin up one within , the first case observed from isolated neutron stars as far as we know. % What's more, the average positive torque is consistent in value and order of magnitude with those deduced from DSUs observed from the Crab pulsar. % The coincidences of DSU appearance and consistent positive torque in the Crab pulsar and SGR…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Geophysics and Gravity Measurements
