Investigating the neutron star physics through observations of several young pulsars in the dipole-field re-emergence scenario

The observed timing data, magnetic tilt angle \(\chi\), and age of young pulsars could be used to probe some important issues about neutron star (NS) physics, e.g., the NS internal magnetic field configuration, and the number of precession cycles \(\xi\). \textbf{Both} quantities are critical in stu...

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Veröffentlicht in:	arXiv.org 2024-10
Hauptverfasser:	Yu-Long, Yan, Cheng, Quan, Xiao-Ping, Zheng
Format:	Artikel
Sprache:	eng
Schlagworte:	Chronology Dipoles Emission Fluids Gravitational waves Magnetars Magnetic field configurations Neutron stars Neutrons Particle decay Physics - High Energy Astrophysical Phenomena Pulsars Superfluidity
Online-Zugang:	Volltext
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