Código QR (código de barras bidimensional)

Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque

The evolutions of a neutron star’s rotation and magnetic field (B-field) have remained unsolved puzzles for over half a century. We ascribe the rotational braking torques of pulsar to both components, the standard magnetic dipole radiation (MDR) and particle wind flow (MDR + Wind, hereafter named MD...

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Principais autores: Cheng-Min Zhang, Xiang-Han Cui, Di Li, De-Hua Wang, Shuang-Qiang Wang, Na Wang, Jian-Wei Zhang, Bo Peng, Wei-Wei Zhu, Yi-Yan Yang, Yuan-Yue Pan
Format: Artigo
Sprog:Inglês
Udgivet: MDPI AG 2022-11-01
Serier:Universe
Fag:
pulsars
general pulsars
individual
PSR B0531 + 21 (the Crab pulsar)
stars
neutron
Online adgang:https://www.mdpi.com/2218-1997/8/12/628
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