更新时间：2023-10-02 13:28
张承民，男，中国科学院国家天文台研究员。研究领域为高能天体物理和广义相对论：中子星自旋和磁场演化等。
大连理工大学学士、硕士，香港大学博士；
天津河北工业大学，巴西圣保罗州大学，台湾清华大学，澳大利亚悉尼大学，中科院 国家天文台。
高能天体物理和广义相对论：中子星自旋和磁场演化，中子星准周期振（QPO），脉冲星射电闪烁，白矮星磁场和QPO研究，中子星天体物理和极端环境，引力场时空性质和天体物理应用。
Is there evidence for field restructuring or decay in accreting magnetic white dwarfs? C.M. Zhang, D. Wickramasinghe & L. Ferrario，MNRAS，2009，397，2208
The Neutron star mass and radius by three measurements C. M. Zhang, H. X. Yin, Y. Kojima, et al, MNRAS，2007, 374, 232
Correlation between Neutron Star spin and kHz QPOs in LMXBs H. X. Yin, C. M. Zhang, Y.H. Zhao, LM Song，F Zhang， AA, 2007, 471, 381
On the low-high frequency mechanism for white dwarf, neutron star and black hole Zhang, C.M., Yin, H.X. & Zhao, Y.H.， PASP, 2007, 119, 393
The correlations between the twin kHz QPO frequencies of LMXBs Zhang, C.M., Yin H.X., Zhao, Y.H., Song, L.M., Zhang, F.， MNRAS, 2006, 366, 1373
Neutron star magnetic field and magnetosphere evolution in low mass X-ray binary Zhang, C.M. and Kojima, Y.， MNRAS, 2006, 366, 137
The kHz QPO mechanism of MHD Alfven wave oscillation Zhang, C.M. AA， 2004, 423, 401
Interpretation of parabolic arcs in pulsar secondary spectra D.B. Melrose, M.W. Walker, D.R. Stinebring, and Zhang, C.M.，MNRAS, 354, 43, 2004
The general treatment of neutrino and thermal neutron interference phase in a gravitational field Zhang, C.M. and A. Beesham，Gen. Rel. Grav., 2001，33, 1101
The axial torsion vector in Kerr spacetime Pereira, J.G., T. Vargas, and Zhang, C.M.， Class. Quant. Grav. 2001，18，833