2 citations · 6 across the 6 of their papers we have counts for
6 papers
Gravitational-wave bursts from spin-precessing black holes in binary systems
Cheng Zhang, Wen-Biao Han, Shu-Cheng Yang
Gravitational waves from precessing binary black holes exhibit new features that are absent in non-precessionary systems. All current waveform models take into account only the mod…
Minimum Accretion Rate for Millisecond Pulsar Formation in Binary System
Yuanyue Pan, Chengmin Zhang, Na Wang
186 binary pulsars are shown in the magnetic field versus spin period (B-P) dia- gram, and their relations to the millisecond pulsars can be clearly seen. We declaim a minimum accr…
The meaning inferred from the spin period distribution of normal pulsars
Ying-Chun Wei, Cheng-Min Zhang, Yong-Heng Zhao +2
We make statistics about the number distribution of normal radio pulsars according to the pulsar spin period. And find the physical meaning of the traditional statistical method ab…
A TFD model for the Electrospheres of Bare Strange Quark Stars
Hai-Chuan Guo, Ren-Xin Xu, Cheng-Min Zhang
We study the layer of electrons on bare strange star surfaces, taking the Dirac exchange-energy into account. Because electrons are fermions, the electron wave function must be of…
Rms-flux relation of Cyg X-1 with RXTE: dipping and nondipping cases
Y. J. Lei, L. M. Song, J. L. Qu +1
The rms (root mean square) variability is the parameter for understanding the emission temporal properties of X-ray binaries (XRBs) and active galactic nuclei (AGN). The rms-flux r…
On the Bottom Magnetic Fields of the Millisecond Pulsars
Chengmin Zhang
The magnetic field strengths of most millisecond pulsars(MSP) are about Gauss. The accretion induced magnetic field evolution scenario here concludes that the field deca…