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Autor principal: Marcel, Miracle Chibuzor
Formato: Preprint
Publicado: 2024
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Acceso en línea:https://arxiv.org/abs/2411.12139
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author Marcel, Miracle Chibuzor
author_facet Marcel, Miracle Chibuzor
contents An updated analysis of pulsar glitch parameters was conducted using a sample of 215 pulsars, encompassing 677 recorded glitch events, each glitch at least once between 1968 and 2024. The glitch rates were estimated and plotted against various pulsar parameters, including rotational frequency, spin-down rate, and characteristic age. These relationships were analyzed using Pearson's correlation coefficient. The results indicate linear and weak relationships between glitch rate and the pulsar parameters. However, the relationship between glitch rate and characteristic age is inversely weak.
format Preprint
id arxiv_https___arxiv_org_abs_2411_12139
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Investigation into Pulsar Glitch Parameters
Marcel, Miracle Chibuzor
High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
An updated analysis of pulsar glitch parameters was conducted using a sample of 215 pulsars, encompassing 677 recorded glitch events, each glitch at least once between 1968 and 2024. The glitch rates were estimated and plotted against various pulsar parameters, including rotational frequency, spin-down rate, and characteristic age. These relationships were analyzed using Pearson's correlation coefficient. The results indicate linear and weak relationships between glitch rate and the pulsar parameters. However, the relationship between glitch rate and characteristic age is inversely weak.
title Investigation into Pulsar Glitch Parameters
topic High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2411.12139