个人简介
李少泽，1989年生，汉族。本科毕业于365365最快线路检测中心物理学专业，2019年于华中师范大学获得理学博士学位，2019-2022年在北京师范大学天文系做博士后研究工作，2023年入职365365最快线路检测中心365365最快线路检测中心。
研究方向
高能天体物理，伽马射线暴与致密星并合，目前的研究兴趣集中于双中子星并合产物及其对致密星状态方程和引力波的限制等方面。
学术成果
目前在ApJ，ApJL，MN等天文学主流期刊发表SCI收录论文10余篇。
[1] Wu, G.-L., Yu, Y.-W., & Li, S.-Z., Magnetar Wind-Driven Shock Breakout Emission after Double Neutron Star Mergers: The Effect of the Anisotropy of the Merger Ejecta, Universe, vol. 8, no. 12, p. 633, 2022
[2] Li, S.-Z., Yu, Y.-W., Gao, H., Dai, Z.-G., & Zheng, X.-P., A Powerful e±Outflow Driven by a Proto-strange Quark Star, The Astrophysical Journal, vol. 922, no. 2, 2021
[3] Lan, L., Gao, H., Ai, S., & Li, S.-Z., The Evolutionary Effects of the Radius and Moment of Inertia of Rapidly Rotating Neutron Stars, The Astrophysical Journal, vol. 919, no. 1, 2021
[4] Li, S.-Z., Yu, Y.-W., Gao, H., & Zhang, B., The Evolution of a Newborn Millisecond Magnetar with a Propeller-recycling Disk, The Astrophysical Journal, vol. 907, no. 2, 2021
[5] Yu, Y.-W., Chen, A., Dai, Z.-G., Li, S.-Z., Liu, L.-D., & Zhu, J.-P., Studying newborn neutron stars by the transient emission after stellar collapses and compact binary mergers, in Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy, 2019, vol. 2127, no. 1
[6] Li, S.-Z., Liu, L.-D., Yu, Y.-W., & Zhang, B., What Powered the Optical Transient AT2017gfo Associated with GW170817?, The Astrophysical Journal, vol. 861, no. 2, 2018
[7] Yu, Y.-W. & Li, S.-Z., A possible relation between flare activity in super-luminous supernovae and gamma-ray bursts, Monthly Notices of the Royal Astronomical Society, vol. 470, no. 1, pp. 197–201, 2017
[8] Yu, Y.-W., Zhu, J.-P., Li, S.-Z., Lü, H.-J., & Zou, Y.-C., A Statistical Study of Superluminous Supernovae Using the Magnetar Engine Model and Implications for Their Connection with Gamma-Ray Bursts and Hypernovae, The Astrophysical Journal, vol. 840, no. 1, 2017
[9] Li, S.-Z. & Yu, Y.-W., Shock Breakout Driven by the Remnant of a Neutron Star Binary Merger: An X-Ray Precursor of Mergernova Emission, The Astrophysical Journal, vol. 819, no. 2, 2016
[10] Li, S.-Z., Yu, Y.-W., & Huang, Y., SN 1054: A pulsar-powered supernova?, Research in Astronomy and Astrophysics, vol. 15, no. 11, 2015
[11] Huang, X., Zheng, X.-P., Wang, W.-H., & Li, S.-Z., Constraints on millicharged particles by neutron stars, Physical Review D, vol. 91, no. 12, 2015
[12] Yu, Y.-W., Li, S.-Z., & Dai, Z.-G., Rapidly Evolving and Luminous Transients Driven by Newly Born Neutron Stars, The Astrophysical Journal, vol. 806, no. 1, 2015
