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| Main Authors: | , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2507.18187 |
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| _version_ | 1866912499621691392 |
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| author | Yu, Zhi-xiang Dang, Shi-jun Wang, Wei-hua Li, Lin Li, Wei Yuan, Jian-ping Kou, Fei-fei Bai, Jun-tao Ge, Mingyu Zhou, Xia Shang, Lun-hua Zhou, Zu-rong Wang, Yu-bin Cai, Yan-qing Zhao, Ru-shuang Li, Qing-ying Zeng, Xiang-dong Wang, Na |
| author_facet | Yu, Zhi-xiang Dang, Shi-jun Wang, Wei-hua Li, Lin Li, Wei Yuan, Jian-ping Kou, Fei-fei Bai, Jun-tao Ge, Mingyu Zhou, Xia Shang, Lun-hua Zhou, Zu-rong Wang, Yu-bin Cai, Yan-qing Zhao, Ru-shuang Li, Qing-ying Zeng, Xiang-dong Wang, Na |
| contents | The study of pulsar glitches provides a unique window into the internal structure and dynamic processes of neutron stars. PSR J0007+7303, a very bright gamma-ray pulsar, is the first pulsar discovered by the Fermi-LAT telescope. In this paper, we present the 15 years of timing results of this pulsar using the Fermi-LAT data. We identified nine glitches, five of which are newly discovered. Among these, two are small glitches, occurring between the three previously reported ones, while the other four are large glitches. The glitches exhibit fractional frequency changes ranging from 15 x 10^-9 to 1238 x 10^-9, with intervals of approximately 1-2 years between events. Uniquely, this pulsar shows no exponential recovery behavior following any glitch, setting it apart from most glitching pulsars. Furthermore, no significant changes were observed in the gamma-ray pulse profile, flux, or phase-averaged spectra before and after glitches, indicating the stability of the pulsar's emission properties despite internal changes. A parametric analysis of the glitches yielded a fractional moment of inertia of the crustal superfluid involved in glitches as 1.06 percent, which matches extremely well with previous statistical work if the non-dissipative entrainment effect is not considered and strongly supports the internal origin of these glitches. These results highlight the distinct glitch behavior of PSR J0007+7303 and offer valuable insights into the crust-superfluid interaction in neutron stars. The physical origin of no exponential recovery is also discussed. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_18187 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Results of 15-Year Pulsar Timing of PSR J0007+7303 with Fermi-LAT Yu, Zhi-xiang Dang, Shi-jun Wang, Wei-hua Li, Lin Li, Wei Yuan, Jian-ping Kou, Fei-fei Bai, Jun-tao Ge, Mingyu Zhou, Xia Shang, Lun-hua Zhou, Zu-rong Wang, Yu-bin Cai, Yan-qing Zhao, Ru-shuang Li, Qing-ying Zeng, Xiang-dong Wang, Na High Energy Astrophysical Phenomena The study of pulsar glitches provides a unique window into the internal structure and dynamic processes of neutron stars. PSR J0007+7303, a very bright gamma-ray pulsar, is the first pulsar discovered by the Fermi-LAT telescope. In this paper, we present the 15 years of timing results of this pulsar using the Fermi-LAT data. We identified nine glitches, five of which are newly discovered. Among these, two are small glitches, occurring between the three previously reported ones, while the other four are large glitches. The glitches exhibit fractional frequency changes ranging from 15 x 10^-9 to 1238 x 10^-9, with intervals of approximately 1-2 years between events. Uniquely, this pulsar shows no exponential recovery behavior following any glitch, setting it apart from most glitching pulsars. Furthermore, no significant changes were observed in the gamma-ray pulse profile, flux, or phase-averaged spectra before and after glitches, indicating the stability of the pulsar's emission properties despite internal changes. A parametric analysis of the glitches yielded a fractional moment of inertia of the crustal superfluid involved in glitches as 1.06 percent, which matches extremely well with previous statistical work if the non-dissipative entrainment effect is not considered and strongly supports the internal origin of these glitches. These results highlight the distinct glitch behavior of PSR J0007+7303 and offer valuable insights into the crust-superfluid interaction in neutron stars. The physical origin of no exponential recovery is also discussed. |
| title | Results of 15-Year Pulsar Timing of PSR J0007+7303 with Fermi-LAT |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2507.18187 |