New pulse profile variability associated with a glitch of PSR J0738-4042
S. Q. Zhou, E. G\"ugercino\u{g}lu, J. P. Yuan, M. Y. Ge, C. Yu, C. M., Zhang, J. Zhang, Z. W. Feng, C. Q. Ye

TL;DR
This study reports the first observed glitch in pulsar PSR J0738-4042, revealing a unique correlation between emission profile changes and spin-down rate, linked to internal neutron star processes and magnetospheric state changes.
Contribution
It identifies a new glitch event in PSR J0738-4042 and links it to emission profile variability, proposing a combined crustquake and vortex creep model for the observed phenomena.
Findings
First glitch observed in PSR J0738-4042
Post-glitch increase in braking torque over 1380 days
Significant change in pulse profile components after glitch
Abstract
The close correlation observed between emission state and spin-down rate change of pulsars has many implications both for the magnetospheric physics and the neutron star interior. The middle-aged pulsar PSR J07384042, which had been observed to display variations in the pulse profile associated with its spin-down rate change due to external effects, is a remarkable example. In this study, based on the 12.5-yr combined public timing data from UTMOST and Parkes, we have detected a new emission-rotation correlation in PSR J07384042 concurrent with a glitch. A glitch that occurred at MJD 57359(5) (December 3, 2015) with is the first glitch event observed in this pulsar and is probably the underlying cause of the emission-rotation correlation. Unlike the usual post-glitch behaviours, the braking torque on the pulsar has continued to increase…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · High-pressure geophysics and materials
