Quakes of Compact Stars
Ruipeng Lu (PKU), Han Yue (PKU), Xiaoyu Lai (HUE), Weihua Wang (WU),, Shenjian Zhang (SUST), Renxin Xu (PKU)

TL;DR
This paper develops a theoretical model incorporating elastic deformation theories to explain pulsar glitches via starquakes, comparing neutron and strangeon star models, and finds that strangeon starquakes can account for observed glitch amplitudes.
Contribution
It introduces a quantitative elastic deformation model for starquakes in pulsars, analyzing stress loading and quake types in neutron and strangeon star models, which is rarely addressed.
Findings
Strangeon starquakes can explain observed glitch amplitudes.
The required starquake magnitude is larger than Earthquakes.
Differences between neutron and strangeon star models are significant.
Abstract
Glitches are commonly observed for pulsars, which are explained by various mechanisms. One hypothesis attributes the glitch effect to the instantaneous moment of inertia change of the whole star caused by a starquake, which is similar to earthquakes caused by fast dislocation occurring on planar faults for the static stress, though the quake-induced dynamics responsible for glitch (superfluid vortex vs. pure starquake) remains still unknown. However, a theoretical model to quantitatively explain the stress loading, types of starquakes, and co-seismic change of moment of inertia is rarely discussed. In this study, we incorporate elastic deformation theories of earthquakes into the starquake problems. We compute the field of stress loading associated with rotation deceleration and determine the optimal type of starquakes at various locations. Two types of pulsar structure models, i.e.…
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Taxonomy
Topicsearthquake and tectonic studies · Pulsars and Gravitational Waves Research · High-pressure geophysics and materials
