2022/11/15 by Wang, Wei-Hua, Ge, Ming-Yu, Huang, Xi +1
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Phenomenology (hep-ph)
paper · doi:10.48550/arxiv.2211.08151
Ge et al. reported a peculiar large glitch observed from SGR 1935 recently~\citep2022arXiv221103246G. % Interestingly, this glitch occurred about 3.1± 2.5~\rmdays before FRB 200428, accompanied by a delayed spin up (DSU) process with a timescale of 8± 1~\rmdays. % 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 8± 1~\rmdays, 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 1935 suggest that, these DSUs have the same physical origin and should be analyzed simultaneously. % Joint analysis on DSUs from the Crab pulsar and SGR 1935 suggests a physical origin independent of (at least not directly dependent on) rotational parameters. % If this new DSU and torque reversal phenomena be further confirmed and accretion be excluded convincingly, nearly all models regarding DSU phenomenon under the framework of vortex motion should be reconsidered, new physics will be required. % We stress that, joint analysis on DSUs from different pulsars with different rotational parameters may provide pivotal clue to reveal their physical origin, even neutron star equation of state and the triggering mechanism(s) of (galactic) fast radio bursts ultimately.