基本信息
张承民  男  博导  中国科学院国家天文台
电子邮件: zhangcm@bao.ac.cn
通信地址: 中科院国家天文台
邮政编码: 100101

研究领域

脉冲星, 中子星,致密星体,引力波辐射与广义相对论 ,快速射电暴, FAST科学

招生信息

1 M.S.  1 Ph.D.

招生专业
070401-天体物理
招生方向
脉冲星; 中子星;天体物理
中子星和黑洞准周期振荡
毫秒脉冲星和引力波

教育背景

1995-09--1998-07   香港大学   博士生
1983-09--1986-07   大连理工大学   硕士生
1979-09--1983-07   大连理工大学   大学生
学历
-- 研究生
学位
-- 博士

工作经历

工作经历
2004-03~现在, 中科院国家天文台, 副研、研究员
2001-11~2004-03,澳大利亚悉尼大学, 研究助理
2001-07~2001-11,台湾国立清华大学,  研究助理
2001-01~2001-07,南非祖鲁兰大学,德国马普爱因斯坦引力研究所, 客座
1998-09~2001-01,巴西圣保罗州大学, 研究助理
1986-07~1995-09,天津河北工业大学, 讲师、副教授、教授
社会兼职
2014-07-01-今,北京市科学促进会理事, 理事
2008-07-01-2012-08-01,中国引力与相对论天体物理学会理事, 理事

教授课程

高能天体物理(1)
学术道德与学术写作规范-分论
英语学术论文写作
高能天体物理I
高能天体物理
现代天体物理II
现代天体物理I

专利与奖励

   
奖励信息
(1) 中国科学院大学朱李月华优秀教师奖, 研究所(学校), 2020
(2) 中国科学院大学优秀课程奖, 研究所(学校), 2014
(3) 国家教委科技进步奖, 二等奖, 部委级, 1995

出版信息

著作:

论文集1: Timing Neutron Stars: Pulsations, Oscillations and Explosions,  eds.    Belloni T. ,Mendez M., Zhang C.M.  (斯普林格出版社, ISSN:0067-0057, 2021

论文集2: Proceedings of IAU-Symposium 290,Feeding compact objects,  Accretions at all scales, eds.  Zhang C.M. , Belloni T. ,Mendez M.,  &Zhang S.N. (剑桥大学出版社 ISBN-13: 978-1107033795,2013) 


书1:奇妙的太空探秘:随神舟进入太空课堂,张承民 ( 北京师范大学出版社,ISSN: 9787303233540, 2020)

书2:中子星与脉冲星天体物理,张承民等(科学出版社, ISBN: 9787030492821,2018)

书3:中国天眼科普-神秘的脉冲星,张承民(清华大学出版社, ISBN:9787302535539,2019)


Publications: recent articles in 2022

2022, Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque,  Zhang Cheng-Min; Cui Xiang-Han; Li Di et al, Universe 2022, 8, 628. https://doi.org/10.3390/universe8120628


2022,Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1  by means of the updated Macquart relation, Cui Xiang-Han; Zhang Cheng-Min; Li Di et al, Ap&SS,367,66 

2022, Study on the magnetic field strength of NGC 300 ULX,Pan Y. Y.; Li Z. S.; Zhang C. M., MNRAS.513.6219 




发表论文
[1] Cui, XiangHan, Zhang, ChengMin, Li, Di, Zhang, JianWei, Peng, Bo, Zhu, WeiWei, Strom, Richard, Wang, ShuangQiang, Wang, Na, Wu, QingDong, Wang, DeHua, Yang, YiYan. Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation. ASTROPHYSICS AND SPACE SCIENCE[J]. 2022, 367(7): http://dx.doi.org/10.1007/s10509-022-04093-y.
[2] Zhang Chengmin. Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque. Universe[J]. 2022, [3] Zhang, Jianwei, Zhang, Chengmin, Li, Di, Yang, Wuming, Cui, Xianghan, Wang, Dehua, Yang, Yiyan, Bi, Shaolan, Zhang, Xianfei. Gaussian mixture models of the total mass distribution of stellar black holes from LIGO-Virgo GWTC-2: Implications on the origin of GW190521. PHYSICAL REVIEW D[J]. 2021, 104(10): [4] Cui, XiangHan, Zhang, ChengMin, Wang, ShuangQiang, Zhang, JianWei, Li, Di, Peng, Bo, Zhu, WeiWei, Wang, Na, Strom, Richard, Ye, ChangQing, Wang, DeHua, Yang, YiYan. Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles?. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2021, 500(3): 3275-3280, http://dx.doi.org/10.1093/mnras/staa3351.
[5] Cui, XiangHan, Zhang, ChengMin, Li, Di, Zhang, JianWei, Peng, Bo, Zhu, WeiWei, Wu, QingDong, Wang, ShuangQiang, Wang, Na, Wang, DeHua, Yang, YiYan, Diao, ZhenQi, Ye, ChangQing, Chang, HsiangKuang. Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars. 2021, [6] 张承民. 从阿雷西博到中国天眼射电望远镜. 科技导报. 2021, [7] Ye, ChangQing, Wang, DeHua, Zhang, ChengMin, Zhang, JianWei. Exploring the accretion-induced evolution of the spin period and magnetic field strength of Be/X-ray Pulsars. ASTROPHYSICS AND SPACE SCIENCE[J]. 2020, 365(7): [8] Wu, QingDong, Zhi, QiJun, Zhang, ChengMin, Wang, DeHua, Ye, ChangQing. Luminosity of a radio pulsar and its new emission death line. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2020, 20(11): 325-332, http://lib.cqvip.com/Qikan/Article/Detail?id=7103588860.
[9] Wang, DeHua, Zhang, ChengMin. The parallel tracks of kHz QPOs in low-mass X-ray binary 4U 1728-34: explorer of the bimodal accretion modes. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2020, 497(3): 2893-2898, https://www.webofscience.com/wos/woscc/full-record/WOS:000577137200029.
[10] Zhu, Weiwei, Li, Di, Luo, Rui, Miao, Chenchen, Zhang, Bing, Spitler, Laura, Lorimer, Duncan, Kramer, Michael, Champion, David, Yue, Youling, Cameron, Andrew, Cruces, Marilyn, Duan, Ran, Feng, Yi, Han, Jun, Hobbs, George, Niu, Chenhui, Niu, Jiarui, Pan, Zhichen, Qian, Lei, Shi, Dai, Tang, Ningyu, Wang, Pei, Wang, Hongfeng, Yuan, Mao, Zhang, Lei, Zhang, Xinxin, Cao, Shuyun, Feng, Li, Gan, Hengqian, Gao, Long, Gu, Xuedong, Guo, Minglei, Hao, Qiaoli, Huang, Lin, Huang, Menglin, Jiang, Peng, Jin, Chengjin, Li, Hui, Li, Qi, Li, Qisheng, Liu, Hongfei, Pan, Gaofeng, Peng, Bo, Qian, Hui, Shi, Xiangwei, Song, Jinyuo, Song, Liqiang, Sun, Caihong, Sun, Jinghai, Wang, Hong, Wang, Qiming, Wang, Yi, Xie, Xiaoyao, Yan, Jun, Yang, Li, Yang, Shimo, Yao, Rui, Yu, Dongjun, Yu, Jinglong, Zhang, Chengmin, Zhang, Haiyan, Zhang, Shuxin, Zheng, Xiaonian, Zhou, Aiying, Zhu, Boqin, Zhu, Lichun, Zhu, Ming, Zhu, Wenbai, Zhu, Yan. A Fast Radio Burst Discovered in FAST Drift Scan Survey. ASTROPHYSICAL JOURNAL LETTERS[J]. 2020, 895(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000536784000001.
[11] Wang, DeHua, Zhang, ChengMin, Qu, JinLu, Jia, ShuMei. Kilohertz quasi-periodic oscillations as probes of the X-ray color-color diagram and neutron star accretion-disk structure for Z sources. ASTRONOMY & ASTROPHYSICS[J]. 2020, 642: https://www.webofscience.com/wos/woscc/full-record/WOS:000581916000007.
[12] Wang, DeHua, Zhang, ChengMin, Wang, ShuangQiang. Investigation on the Binary Millisecond Pulsars at Radio and gamma-Ray Wavelengths: Links with the Orbital Parameters. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC[J]. 2020, 132(1013): https://www.webofscience.com/wos/woscc/full-record/WOS:000541753000001.
[13] Zhang, Jianwei, Zhang, Chengmin, Yang, Wuming, Yang, Yiyan, Li, Di, Bi, Shaolan, Zhang, Xianfei. Simulation of chirp mass distribution of neutron star and black hole merger events for gravitational-wave radiation. PHYSICAL REVIEW D[J]. 2020, 101(4): http://dx.doi.org/10.1103/PhysRevD.101.043018.
[14] YeZhao Yu, Bo Peng, Kuo Liu, ChengMin Zhang, Lin Wang, FeiFei Kou, JiGuang Lu, Meng Yu, FAST Collaboration. FAST ultra-wideband observation of abnormal emission-shift events of PSR B0919$+$06. SCIENCE CHINA Physics, Mechanics & Astronomy[J]. 2019, 62(5): 6-, https://www.sciengine.com/doi/10.1007/s11433-018-9358-8.
[15] Wang, DeHua, Zhang, ChengMin, Wang, ShuangQiang. Investigation of the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and gamma-Ray. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC[J]. 2019, 131(996): http://ir.xao.ac.cn/handle/45760611-7/2349.
[16] Wang, DeHua, Zhang, ChengMin, Wang, ShuangQiang. Investigation of the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and gamma-Ray. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC[J]. 2019, 131(996): http://libir.pmo.ac.cn/handle/332002/20562.
[17] Ye, ChangQing, Wang, DeHua, Zhang, ChengMin, Diao, ZhenQi. Evolution implications of neutron star magnetic fields: inferred from pulsars and cyclotron lines of HMXBs. ASTROPHYSICS AND SPACE SCIENCE[J]. 2019, 364(11): 7-, http://dx.doi.org/10.1007/s10509-019-3690-1.
[18] Zhang, Lei, Li, Di, Hobbs, George, Agar, Crispin H, Manchester, Richard N, Weltevrede, Patrick, Coles, William A, Wang, Pei, Zhu, Weiwei, Wen, Zhigang, Yuan, Jianping, Cameron, Andrew D, Dai, Shi, Liu, Kuo, Zhi, Qijun, Miao, Chenchen, Yuan, Mao, Cao, Shuyun, Feng, Li, Gan, Hengqian, Gao, Long, Gu, Xuedong, Guo, Minglei, Hao, Qiaoli, Huang, Lin, Jiang, Peng, Jin, Chengjin, Li, Hui, Li, Qi, Li, Qisheng, Liu, Hongfei, Pan, Gaofeng, Pan, Zhichen, Peng, Bo, Qian, Hui, Qian, Lei, Shi, Xiangwei, Song, Jinyou, Song, Liqiang, Sun, Caihong, Sun, Jinghai, Wang, Hong, Wang, Qiming, Wang, Yi, Xie, Xiaoyao, Yan, Jun, Yang, Li, Yang, Shimo, Yao, Rui, Yu, Dongjun, Yu, Jinglong, Yue, Youling, Zhang, Chengmin, Zhang, Haiyan, Zhang, Shuxin, Zheng, Xiaonian, Zhou, Aiying, Zhu, Boqin, Zhu, Lichun, Zhu, Ming, Zhu, Wenbai, Zhu, Yan. PSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST. ASTROPHYSICAL JOURNAL[J]. 2019, 877(1): [19] Yang, YiYan, Zhang, ChengMin, Li, Di, Chen, Li, Linghu, RongFeng, Zhi, QiJun. The Classifications of Double Neutron Stars and their Correlations with the Binary Orbital Parameters. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC[J]. 2019, 131(1000): [20] 叶长青, 王德华, 张承民, 吴庆东. x射线双星回旋吸收线研究进展. 天文学进展[J]. 2019, 37(2): 129-, http://lib.cqvip.com/Qikan/Article/Detail?id=7002350554.
[21] Liu, Peng, Zhang, ChengMin, Li, Di, Yang, YiYan, Zhang, Jie, Zhang, JianWei. The Simulation of Orbit Decay of Double Neutron Star System PSR J1906+0746 by the Gravitational Wave Radiation. ASTRONOMY REPORTS[J]. 2019, 63(12): 1090-1094, http://dx.doi.org/10.1134/S1063772919130031.
[22] Zhang, Jianwei, Yang, Yiyan, Zhang, Chengmin, Yang, Wuming, Li, Di, Bi, Shaolan, Zhang, Xianfei. The mass distribution of Galactic double neutron stars: constraints on the gravitational-wave sources like GW170817. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2019, 488(4): 5020-5028, http://dx.doi.org/10.1093/mnras/stz2020.
[23] 张承民, 杨佚沿, 支启军. 从宋代客星到中国天眼中的脉冲星李约瑟难题试答. 科技导报北京[J]. 2018, 36(12): 15-, http://lib.cqvip.com/Qikan/Article/Detail?id=675500315.
[24] 张承民, 杨佚沿, 支启军. 从宋代“客星”到中国“天眼”中的脉冲星——“李约瑟难题”试答. 科技导报[J]. 2018, 36(12): 15-21, http://lib.cqvip.com/Qikan/Article/Detail?id=675500315.
[25] 刘鹏, 王培, 李菂, 张洁, 张蕾, 张承民, 朱炜炜, 岳友岭, 代实. FAST 19波束脉冲星漂移扫描巡天模拟. 天文学进展[J]. 2018, 36(2): 173-, http://lib.cqvip.com/Qikan/Article/Detail?id=675860266.
[26] 杨佚沿, 岳友岭, 王双强, 张承民, 王娜, 李菂, 尚伦华, 王德华, 潘元月. 特殊类型脉冲星的研究进展. 天文学进展[J]. 2018, 36(1): 1-, http://ir.xao.ac.cn/handle/45760611-7/2468.
[27] Wang, DeHua, Zhang, ChengMin, Qu, JinLu, Yang, YiYan. Correlations between the frequencies of twin kHz QPOs and spins of neutron stars in LMXBs. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 473(4): 4862-4867, http://libir.pmo.ac.cn/handle/332002/22232.
[28] Pan, Y Y, Zhang, C M, Song, L M, Wang, N, Li, D, Yang, Y Y. The minimum magnetic field of millisecond pulsars calculated according to accretion: application to the X-ray neutron star SAX J1808.4-3658 in a low-mass X-ray binary. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 480(1): 692-696, http://ir.xao.ac.cn/handle/45760611-7/2130.
[29] Wang, DeHua, Zhang, ChengMin, Qu, JinLu. The kHz QPOs as a probe of the X-ray color-color diagram and accretion-disk structure for the atoll source 4U 1728-34. ASTRONOMY & ASTROPHYSICS[J]. 2018, 618: https://www.webofscience.com/wos/woscc/full-record/WOS:000449280200001.
[30] 张承民, 图. “天眼”遥望脉冲星. 当代贵州[J]. 2018, 18-19, http://lib.cqvip.com/Qikan/Article/Detail?id=675897269.
[31] Yang, YiYan, Zhang, ChengMin, Li, Di, Wang, DeHua, Pan, YuanYue, Lingfu, RongFeng, Zhou, ZhuWen. Similarity of PSR J1906+0746 to PSR J0737-3039: a Candidate of a New Double Pulsar System?. ASTROPHYSICAL JOURNAL[J]. 2017, 835(2): http://ir.bao.ac.cn/handle/114a11/8802.
[32] 张承民, 王培, 杨佚沿. FAST脉冲星发现新视野. 科技导报[J]. 2017, 35(21): 12-13, http://lib.cqvip.com/Qikan/Article/Detail?id=673850356.
[33] 戚湛强, 丁文波, 张承民, 侯佳为. 中子星内部中微子辐射的相对论修正. 天文学报[J]. 2017, 58(1): 8-, http://lib.cqvip.com/Qikan/Article/Detail?id=671269531.
[34] 张承民, 王双强, 尚伦华, 杨佚沿. 脉冲星发现50年. 科技导报[J]. 2017, 35(18): 52-, http://ir.xao.ac.cn/handle/45760611-7/1809.
[35] Shang, LunHua, Zhang, ChengMin, Li, Di, Wan, DeHua, Wang, ShuangQiang, Wang, Pei, Pan, YuanYue, Yang, YiYan, Zin, QiJun. State Switching of the X-Ray/Radio Transitional Millisecond Pulsar. ASTROPHYSICAL JOURNAL[J]. 2017, 849(2): http://libir.pmo.ac.cn/handle/332002/22550.
[36] 张承民, 杨佚沿, 支启军. 脉冲星发现50年:科学意义与未来观测. 科学[J]. 2017, 69(6): 50-52, http://lib.cqvip.com/Qikan/Article/Detail?id=674164665.
[37] Wang, D H, Zhang, C M, Lei, Y J, Chen, L, Qu, J L, Zhi, Q J. Probing the accretion disc structure by the twin kHz QPOs and spins of neutron stars in LMXBs. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2017, 466(1): 1111-1117, http://dx.doi.org/10.1093/mnras/stw3134.
[38] 张承民, 王培, 杨佚沿. fast脉冲星发现新视野. 科技导报北京[J]. 2017, 35(21): 12-, http://lib.cqvip.com/Qikan/Article/Detail?id=673850356.
[39] 张承民. 超级亮度X-射线源磁场与吸积磁星. MNRAS. 2016, [40] 张承民. 中子星转动演化. ASPC. 2016, [41] 张承民. “天眼”开启宇宙新发现值得期待. 中国战略新兴产业[J]. 2016, 94-94, http://lib.cqvip.com/Qikan/Article/Detail?id=670592691.
[42] 杨佚沿, 张承民, 王德华, 潘元月, 周筑文. 双中子星质量分布的统计研究. 天文学报[J]. 2016, 57(6): 647-, http://lib.cqvip.com/Qikan/Article/Detail?id=670786331.
[43] 张月竹, 付妍妍, 魏益焕, 张承民, 禺少华, 潘元月, 郭元旗, 王德华. 脉冲星减速研究与电磁和引力波辐射. 天文学报[J]. 2015, 56(3): 235-, http://lib.cqvip.com/Qikan/Article/Detail?id=664910735.
[44] 张承民. 吸积中子星磁场演化模拟. AN. 2015, [45] 张承民. 中子星低质量X射线源震荡研究. MNRAS. 2015, [46] 付妍妍, 张月竹, 魏益焕, 张承民, 禺少华, 潘元月, 郭元旗, 王德华. 中子星吸积加速与引力辐射影响. 天文学报[J]. 2015, 56(3): 225-, http://lib.cqvip.com/Qikan/Article/Detail?id=664910734.
[47] 张承民. 中子星准周期震荡分布. AN. 2014, [48] Lei, YaJuan, Zhang, Shu, Qu, JinLu, Yuan, HaiLong, Wang, YaNan, Dong, YiQiao, Zhang, HaoTong, Li, ZhiBing, Zhang, ChengMin, Zhao, YongHeng. THE PROPERTIES OF CROSS-CORRELATION AND SPECTRA OF THE LOW-MASS X-RAY BINARY 4U 1608-52. ASTRONOMICAL JOURNAL[J]. 2014, 147(3): http://ir.ihep.ac.cn/handle/311005/224833.
[49] 张承民. 中子星千赫兹准周期震荡. MNRAS. 2013, [50] 赵复垣, 徐琳, 张承民, Strom Richard. 新石器时代八角星图案与超新星爆发. 科技导报北京[J]. 2013, 31(23): 15-, [51] 程争, 张承民, 赵永恒, 王德华, 潘元月, 雷亚娟. 中子星质量分布的统计研究. 天文学报[J]. 2013, 54(6): 514-, http://lib.cqvip.com/Qikan/Article/Detail?id=47966408.
[52] 张承民. 毫秒脉冲星磁场. IAUS. 2013, [53] Lei, YaJuan, Zhang, HaoTong, Zhang, ChengMin, Qu, JinLu, Yuan, HaiLong, Dong, YiQiao, Zhao, YongHeng, Wang, DeHua, Yin, HongXing, Zhang, YanXia, Song, LiMing. EVOLUTION OF THE CROSS-CORRELATION AND TIME LAG OF 4U 1735-44 ALONG THE BRANCHES. ASTRONOMICAL JOURNAL[J]. 2013, 146(3): http://ir.ihep.ac.cn/handle/311005/224406.
[54] Taani, Ali, Naso, Luca, Wei, Yingchun, Zhang, Chengmin, Zhao, Yongheng. Modeling the spatial distribution of neutron stars in the Galaxy. ASTROPHYSICS AND SPACE SCIENCE[J]. 2012, 341(2): 601-609, http://ir.bao.ac.cn/handle/114a11/6174.
[55] 张承民. 加速脉冲星周期演化研究. AA. 2012, [56] Strom, Richard G, Zhao, FuYuan, Zhang, ChengMin. Could bright gamma-ray burst optical transients have been recorded historically?. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2012, 12(3): 260-268, http://ir.bao.ac.cn/handle/114a11/6083.
[57] Yan, ShuPing, Qu, JinLu, Ding, GuoQiang, Han, Peng, Song, LiMing, Zhang, Shu, Yin, HongXing, Zhang, ChengMin, Wang, JianMin. A systematic study on energy dependence of quasi-periodic oscillation frequency in GRS 1915+105. ASTROPHYSICS AND SPACE SCIENCE[J]. 2012, 337(1): 137-146, http://ir.bao.ac.cn/handle/114a11/6249.
[58] Taani, Ali, Zhang, Chengmin, AlWardat, Mashhoor, Zhao, Yongheng. Investigation of some physical properties of accretion induced collapse in producing millisecond pulsars. ASTROPHYSICS AND SPACE SCIENCE[J]. 2012, 340(1): 147-153, http://ir.bao.ac.cn/handle/114a11/6290.
[59] Strom Richard G, Zhao Fuyuan, Zhang Chengmin. Could bright γ-ray burst optical transients have been recorded historically?. 天文和天体物理学研究:英文版[J]. 2012, 12(3): 260-268, http://lib.cqvip.com/Qikan/Article/Detail?id=41348523.
[60] 蔡炎, 阿里塔尼, 赵永恒, 张承民. 脉冲星参数统计和演化. 天文学报[J]. 2011, 52(6): 449-, http://lib.cqvip.com/Qikan/Article/Detail?id=39964664.
[61] Wu, YuZhong, Zhang, EnPeng, Liang, YanChun, Zhang, ChengMin, Zhao, YongHeng. THE DIFFERENT NATURE OF SEYFERT 2 GALAXIES WITH AND WITHOUT HIDDEN BROAD-LINE REGIONS. ASTROPHYSICAL JOURNAL[J]. 2011, 730(2): http://ir.bao.ac.cn/handle/114a11/7869.
[62] 张承民. 中子星kHz QPO模型. AA. 2011, [63] Cai Yan, Taani, A, Wang Wei, Zhao YongHeng, Zhang ChengMin. Fermi gamma-Ray Pulsars: Spectral and Generation Order Parameters. CHINESE PHYSICS LETTERS[J]. 2011, 28(8): http://ir.bao.ac.cn/handle/114a11/7905.
[64] CAI Yan, ATaani, WANG Wei, ZHAO YongHeng, ZHANG ChengMin. Fermi y-Ray Pulsars:Spectral and Generation Order Parameters. Chinese Physics Letters[J]. 2011, 28(8): 089702-1, [65] Ren, Jun, Zhang, ChengMin. Neutrino oscillations in the Kerr-Newman spacetime. CLASSICAL AND QUANTUM GRAVITY[J]. 2010, 27(6): http://ir.bao.ac.cn/handle/114a11/7687.
[66] 张承民. 因为教育 中华民族可能遭遇未来危机——高锟获诺贝尔奖再中国教育. 大学指南[J]. 2010, 12-12, http://lib.cqvip.com/Qikan/Article/Detail?id=33144220.
[67] Wei YingChun, Zhang ChengMin, Wu XinJi, Zhao YongHeng, Chou ChiKang, Luo ALi. The spatial distribution of old neutron stars in the Galaxy. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2010, 53(10): 1939-1946, http://ir.bao.ac.cn/handle/114a11/7686.
[68] 张承民. QPO辐射机制. 中国科学. 2010, [69] Zhang ChengMin, Wei YingChun, Yin HongXing, Zhao YongHeng, Lei YaJuan, Song LiMing, Zhang Fan, Yan Yan. The emission positions of kHz QPOs and Kerr spacetime influence. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2010, 53(1): 114-116, http://ir.ihep.ac.cn/handle/311005/226253.
[70] 张承民. KN时空中微子震荡. CQG. 2010, [71] 张承民. 白矮星磁场减少和结构. MNRAS. 2009, [72] 张承民. QPO估计中子星质量. AN. 2009, [73] Chen, YuPeng, Zhang, Shu, Schurch, Nick, Wang, JianMin, Collmar, Werner, Li, TiPei, Qu, JinLu, Zhang, ChengMin. INTEGRAL and RXTE/ASM Observations on IGRJ17098-3628. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2008, 60(5): 1173-1180, http://ir.bao.ac.cn/handle/114a11/7470.
[74] 张承民. CYGX-2 时间延迟演化. APJ. 2008, [75] 陈尉, 屈进禄, 张澍, 张帆, 张国宝, 陈玉鹏. 大质量X射线双星脉冲星4U 1901+03的脉冲轮廓研究. 天文学报[J]. 2008, 18-28, http://lib.cqvip.com/Qikan/Article/Detail?id=26299499.
[76] 黄玉梅, 王运永, 汤克云, 康飞, 张承民, 徐军, 郭有光. 引力波理论和实验的新进展. 天文学进展[J]. 2007, 25(1): 58-, http://ir.siom.ac.cn/handle/181231/6019.
[77] 张承民. 中子星自旋和QPO关系. AA. 2007, [78] 张承民. 脉冲星发现40年——爱因斯坦预言引力波的验证. 科学[J]. 2007, 59(4): 25-, http://lib.cqvip.com/Qikan/Article/Detail?id=25265590.
[79] Zhang, Chengmin. Magnetic field and spin frequency of X-ray neutron star associated with the kHz QPOs. ADVANCES IN SPACE RESEARCH[J]. 2007, 40(10): 1480-1484, http://dx.doi.org/10.1016/j.asr.2007.06.011.
[80] 张承民. kHz QPO关系. MNRAS. 2006, [81] 张承民. 中子星磁场和磁球演化. MNRAS. 2006, [82] ZHANG Cheng-Min. Torsion Axial-Vector in an Alternative Kerr Tetrad Field. 理论物理通讯:英文版[J]. 2005, 279-282, http://lib.cqvip.com/Qikan/Article/Detail?id=18095379.
[83] 张承民, 吴鑫基. 引力自旋效应和脉冲星磁场演化. 河北师范学院学报:自然科学版[J]. 1991, 43-50, http://lib.cqvip.com/Qikan/Article/Detail?id=513782.

科研活动

   
科研项目

(1) 毫秒脉冲星研究, 主持, 国家级, 2012-01--2015-12 

(2) 中子星准周期震荡研究, 主持, 国家级, 2008-01--2010-12 

(3) 射电天文学---脉冲星研究子课题, 子课题负责, 国家级, 2012-01--2016-12 

(4) 基于FAST漂移扫描巡天的脉冲星统计观测和理论研究, 子课题负责, 国家级, 2018-01--2021-12 

(5)  基于HXMT研究中子星的磁场与结构,主持,国家级,2020-01--2022-12

参与会议

中国相对论与天体物理引力会议,贵州都匀,2019-04

中国射电天文研讨会,贵州平塘,2019-03

中国相对论与引力波会议,山东济南,2019-10


(1)脉冲星PSR1906分析研究   中国天文学年会   2018-10-28 

(2)FAST pulsar investigation    2018-06-13 

(3)脉冲星进展与FAST新发现   全国射电天文学年会   2017-11-29 

(4)脉冲星50年的发展评述   中国天文学会议   2017-08-03 

(5)中子星磁场演化   欧洲天文学与空间科学大会   2016-07-04 

(6)test of GR and pulsar   爱因斯坦百年会议   2015-05-04 

(7)FAST脉冲星科学   中国南非天文学双边会议   2015-03-01 

(8)J Bell and Pulsar science   平方公里阵科学会议   2014-02-03 

(9)pulsar in millisecond bands   射电天文科学与装置会议   新疆   2013-09-05 

(10)kHz QPO and accretion   国际天文学大会   CM ZHANG   2012-08-01