Investigation into Pulsar Glitch Parameters
Fuente:
arXiv
Enregistré dans:
| Auteur principal: | |
|---|---|
| Format: | Preprint |
| Publié: |
2024
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1866915024840163328 |
|---|---|
| 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 |