4 papers
Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?
Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng +1
Newborn magnetars are important gravitational wave sources due to their ultra-strong magnetic fields and fast spins, and the entire population in the Universe may significantly con…
Investigating the neutron star physics through observations of several young pulsars in the dipole-field re-emergence scenario
Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng
The observed timing data, magnetic tilt angle , and age of young pulsars could be used to probe some important issues about neutron star (NS) physics, e.g., the NS internal mag…
Constraints on the internal physics of neutron stars from the observational data of several young pulsars: the role of a power-law decaying dipole magnetic field
Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng
The observational data (e.g., the timing data and magnetic tilt angles ) of young pulsars can be used to probe some critical issues about the internal physics of neutron stars…
On the initial spin periods of magnetars born in weak supernova explosions and their gravitational wave radiation
Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng +1
The initial spin periods of newborn magnetars are \textbf{strongly associated with the origin of their strong magnetic fields, both of which can affect the electromagnetic radiatio…