Glitch Statistics of Radio Pulsars : Multiple populations
Sushan Konar (NCRA-TIFR), Mihir Arjunwadkar (CMS, UoP)

TL;DR
This paper investigates the energy distribution of pulsar glitches and finds evidence for multiple distinct populations, suggesting different underlying mechanisms.
Contribution
It identifies multiple statistically distinct glitch populations, indicating varied mechanisms behind pulsar glitches.
Findings
Multiple glitch populations with different energy distributions
Evidence for different mechanisms causing glitches
Statistical analysis supports multiple underlying processes
Abstract
There appears to be more than one statistically different populations in the energy distribution of glitches, strongly indicative of different mechanisms accessing different energy ranges responsible for them.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRadio Astronomy Observations and Technology · Pulsars and Gravitational Waves Research · Particle Accelerators and Free-Electron Lasers
