M Millhouse, A Melatos, G Howitt… - Monthly Notices of …, 2022 - academic.oup.com
Radio pulsar glitches probe far-from-equilibrium processes involving stress accumulation and relaxation in neutron star interiors. Previous studies of glitch rates have focused on …
There are two types of timing irregularities seen in pulsars: glitches and timing noise. Both of these phenomena can help us to probe the interior of such exotic objects. This paper …
A Melatos, M Millhouse - The Astrophysical Journal, 2023 - iopscience.iop.org
Measuring the Vortex−Nucleus Pinning Force from Pulsar Glitch Rates - IOPscience Skip to content IOP Science home Accessibility Help Search Journals Journals list Browse more than …
WH Wang, XY Lai, EP Zhou, JG Lu… - Monthly Notices of the …, 2021 - academic.oup.com
Glitch is supposed to be a useful probe into pulsar's interior, but the underlying physics remains puzzling. The glitch activity may reflect a lower limit of the crustal moment of inertia …
S Arumugam, S Desai - Journal of High Energy Astrophysics, 2023 - Elsevier
We carry out a classification of the glitch amplitudes of radio pulsars using Extreme Deconvolution technique based on the Gaussian Mixture Model, where the observed …
QH Peng, JJ Liu, CK Chou - New Astronomy, 2022 - Elsevier
Based on the oscillation between the B phase and A phase of 3 P 2 neutron superfluid in neutron stars, we propose a new glitch model for young pulsars. According to our model, the …
PX Zhu, XP Zheng - The Astrophysical Journal, 2024 - iopscience.iop.org
The study of pulsar glitch phenomena serves as a valuable probe into the dynamic properties of matter under extreme high-density conditions, offering insights into the physics …
The number of sudden spin-ups in radio pulsars known as pulsar glitches has increased over the years. Though a consensus has not been reached with regards to the actual cause …
IO Eya, EU Iyida - Research in Astronomy and Astrophysics, 2024 - iopscience.iop.org
Glitch activity refers to the mean increase in pulsar spin frequency per year due to rotational glitches. It is an important tool for studying super-nuclear matter using neutron star interiors …