张承民

中国科学院国家天文台

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  • 张承民
  • 研究员
  • 北京市朝阳区大屯路甲20号 中国科学院国家天文台B231

简历:

教育经历:

大连理工大学学士、硕士,香港大学博士;

工作经历:

天津河北工业大学,巴西圣保罗州大学,台湾国立清华大学,澳大利亚悉尼大学,中科院 国家天文台。

研究领域:

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。

承担科研项目情况:

社会任职:

获奖及荣誉:

代表论著:

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, 232Correlation 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, 1373Neutron star magnetic field and magnetosphere evolution in low mass X-ray binary Zhang, C.M. and Kojima, Y., MNRAS, 2006, 366, 137The kHz QPO mechanism of MHD Alfven wave oscillation Zhang, C.M. AA, 2004, 423, 401Interpretation of parabolic arcs in pulsar secondary spectra D.B. Melrose, M.W. Walker, D.R. Stinebring, and Zhang, C.M.,MNRAS, 354, 43, 2004The general treatment of neutrino and thermal neutron interference phase in a gravitational field Zhang, C.M. and A. Beesham,Gen. Rel. Grav., 2001,33, 1101The axial torsion vector in Kerr spacetime Pereira, J.G., T. Vargas, and Zhang, C.M., Class. Quant. Grav. 2001,18,833