# Statistical characterization of pulsar glitches and their potential   impact on searches for continuous gravitational waves

**Authors:** Gregory Ashton, Reinhard Prix, David Ian Jones

arXiv: 1704.00742 · 2017-09-26

## TL;DR

This paper statistically analyzes pulsar glitches to assess their impact on continuous gravitational wave searches, revealing that glitches can significantly reduce detection sensitivity and cause missed signals.

## Contribution

It introduces a statistical framework to estimate glitch occurrence and their effects on gravitational wave search mismatch, highlighting potential detection challenges.

## Key findings

- Glitches increase the likelihood of signal mismatch in searches.
- Many pulsars have a high probability of experiencing glitches during searches.
- Glitches can cause substantial loss of signal-to-noise ratio, risking missed detections.

## Abstract

Continuous gravitational waves from neutron stars could provide an invaluable resource to learn about their interior physics. A common search method involves matched filtering a modeled template against the noisy gravitational-wave data to find signals. This method suffers a mismatch (i.e., relative loss of the signal-to-noise ratio) if the signal deviates from the template. One possible instance in which this may occur is if the neutron star undergoes a glitch, a sudden rapid increase in the rotation frequency seen in the timing of many radio pulsars. In this work, we use a statistical characterization of the glitch rate and size in radio pulsars to estimate how often neutron star glitches would occur within the parameter space of continuous gravitational-wave searches and how much mismatch putative signals would suffer in the search due to these glitches. We find that for many previous and potential future searches continuous-wave signals have an elevated probability of undergoing one or more glitches and that these glitches will often lead to a substantial fraction of the signal-to-noise ratio being lost. This could lead to a failure to identify candidate gravitational-wave signals in the initial stages of a search and also to the false dismissal of candidates in subsequent follow-up stages.

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Source: https://tomesphere.com/paper/1704.00742