张承民,贵州师范大学物理与电子科学学院教师,研究方向为天文学、物理学及自然科学理论与方法;主要开展毫秒脉冲星、中子星物理、X射线双星、FAST观测模拟及相关多信使天体物理研究,代表成果包括《中国天眼新视角:毫秒脉冲星与引力波探针》《毫秒脉冲星40年回望:中子星磁场的奥秘》《The minimum spin and magnetic of millisecond pulsars》等。
杨佚沿,张承民,张见微,王德华 (2021). Constraints on the kinetic energy of type-Ic supernova explosion from young PSR J1906+0746 in a double neutron star candidate. Chinese Physics B.
崔翔翰,张承民,王双强,张见微,李菂,彭勃,朱炜玮,李查德,王娜,吴庆东,叶长青,王德华,杨佚沿,刁振琪 (2021). Statistical properties of fast radio bursts elucidate their origins:magnetars are favored over gamma-ray bursts. Research in Astronomy and Astrophysics.
张见微,张承民,李菂,崔翔翰,杨伍明,王德华,杨佚沿,毕少兰,张先飞 (2021). Simulation of the gravitational wave frequency distribution of neutron star–black hole mergers. Chinese Physics B.