29 citations · 92 across the 7 of their papers we have counts for
9 papers
Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque
Cheng-Min Zhang, Xiang-Han Cui, Di Li +8
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…
Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation
Xiang-Han Cui, Cheng-Min Zhang, Di Li +9
Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are on…
Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars
Xiang-Han Cui, Cheng-Min Zhang, Di Li +11
The properties of the young pulsars and their relations to the supernova remnants (SNRs) have been the interesting topics. At present, 383 SNRs in the Milky Way galaxy have been pu…
Statistical properties of fast radio bursts elucidate their origins: magnetars are favoured over gamma-ray bursts
Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +11
Fast radio bursts (FRBs) are extremely strong radio flares lasting several milliseconds, most of which come from unidentified objects at a cosmological distance. They can be appare…
Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles
Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +9
Fast Radio Bursts (FRBs) are the short, strong radio pulses lasting several milliseconds. They are subsequently identified, for the most part, as emanating from unknown objects at…
Evolution implications of neutron star magnetic fields: inferred from pulsars and cyclotron lines of HMXBs
Chang-Qing Ye, De-Hua Wang, Cheng-Min Zhang +1
The evolution of neutron star (NS) magnetic field (B-field) has long been an important topic, which is still not yet settled down. Here, we analyze the NS B-fields inferred by the…