基本信息
易疏序 男 中国科学院高能物理研究所
电子邮件: sxyi@ihep.ac.cn
通信地址: 北京市石景山区玉泉路19号乙多学科楼322
邮政编码:
电子邮件: sxyi@ihep.ac.cn
通信地址: 北京市石景山区玉泉路19号乙多学科楼322
邮政编码:
研究领域
我的以往研究经历涵盖以下领域:
- 脉冲星计时
- 高能致密双星理论研究
- 引力波天文学
其中,我的上一个项目题为《引力波宇宙工具箱》。其项目网站为:https://gw-universe.org
目前,我的研究重点在引力波与高能天体物理结合的多信使天文学方向。
招生信息
招生专业
070401-天体物理
招生方向
高能天体物理;多信使天文学;引力波天文学
教育背景
2010-08--2016-07 中国科学院大学 理学博士2006-08--2010-07 清华大学 理学学士
工作经历
工作简历
2018-09~2021-10,Radboud University, 天文系博士后2016-10~2018-08,香港大学, 天文系博士后
出版信息
发表论文
[1] ShuXu Yi, Zhen Zhang, Xilu Wang. Flares from Merged Magnetars: Their Prospects as a New Population of Gamma-Ray Counterparts of Binary Neutron Star Mergers. THE ASTROPHYSICAL JOURNAL[J]. 2023, 955(1): https://doaj.org/article/1385f34f1ac845f394ca529d4730aba9.[2] Xiao, Shuo, Yang, JiaoJiao, Luo, XiHong, Xiong, ShaoLin, Qu, YuanHong, Zhang, ShuangNan, Xue, WangChen, Li, XiaoBo, Tuo, YouLi, Dong, AiJun, Zhao, RuShuang, Dang, ShiJun, Shang, LunHua, Ma, QingBo, Cai, Ce, Wang, Jin, Wang, Ping, Li, ChengKui, Yi, ShuXu, Zhang, Zhen, Ge, MingYu, Zheng, ShiJie, Song, LiMing, Peng, WenXi, Wen, XiangYang, Li, XinQiao, An, ZhengHua, Xu, Xin, Wang, Yue, Zheng, Chao, Zhang, YanQiu, Liu, JiaCong, Zhang, Bin, Xie, Wei, Feng, JianChao, Wang, DeHua, Zhi, QiJun. The Minimum Variation Timescales of X-Ray Bursts from SGR J1935+2154. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES[J]. 2023, 268(1): http://dx.doi.org/10.3847/1538-4365/ace77c.[3] Yi, ShuXu, Nelemans, Gijs, Brinkerink, Christiaan, KostrzewaRutkowska, Zuzanna, Timmer, Sjoerd T, Stoppa, Fiorenzo, Rossi, Elena M, Zwart, Simon F Portegies. The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors. 2022, http://arxiv.org/abs/2106.13662.[4] Shu-Xu Yi, et. al.. The GW-Universe Toolbox II: constraining the binary black hole population with second and third generation detectors. Astronomy & Astrophysics[J]. 2022, [5] Zhang, Zhen, Yi, ShuXu, Zhang, ShuangNan, Xiong, ShaoLin, Xiao, Shuo. Tidally-induced Magnetar Super Flare at the Eve of Coalescence with Its Compact Companion. ASTROPHYSICAL JOURNAL LETTERS[J]. 2022, 939(2): [6] Ackley, K, Amati, L, Barbieri, C, Bauer, F E, Benetti, S, Bernardini, M G, Bhirombhakdi, K, Botticella, M T, Branchesi, M, Brocato, E, Bruun, S H, Bulla, M, Campana, S, Cappellaro, E, CastroTirado, A J, Chambers, K C, Chaty, S, Chen, TW, Ciolfi, R, Coleiro, A, Copperwheat, C M, Covino, S, Cutter, R, DAmmando, F, DAvanzo, P, De Cesare, G, DElia, V, Della Valle, M, Denneau, L, De Pasquale, M, Dhillon, V S, Dyer, M J, EliasRosa, N, Evans, P A, EylesFerris, R A J, Fiore, A, Fraser, M, Fruchter, A S, Fynbo, J P U, Galbany, L, Gall, C, Galloway, D K, Getman, F, I, Ghirlanda, G, Gillanders, J H, Gomboc, A, Gompertz, B P, GonzalezFernandez, C, GonzalezGaitan, S, Grado, A, Greco, G, Gromadzki, M, Groot, P J, Gutierrez, C P, Heikkila, T, Heintz, K E, Hjorth, J, Hu, YD, Huber, M E, Inserra, C, Izzo, L, Japelj, J, Jerkstrand, A, Jin, Z P, Jonker, P G, Kankare, E, Kann, D A, Kennedy, M, Kim, S, Klose, S, Kool, E C, Kotak, R, Kuncarayakti, H, Lamb, G P, Leloudas, G, Levan, A J, Longo, F, Lowe, T B, Lyman, J D, Magnier, E, Maguire, K, Maiorano, E, Mandel, I, Mapelli, M, Mattila, S, McBrien, O R, Melandri, A, Michalowski, M J, MilvangJensen, B, Moran, S, Nicastro, L, Nicholl, M, Guelbenzu, A Nicuesa, Nuttal, L, Oates, S R, OBrien, P T, Onori, F, Palazzi, E, Patricelli, B, Perego, A, Torres, M A P, Perley, D A, Pian, E, Pignata, G, Piranomonte, S, Poshyachinda, S, Possenti, A, Pumo, M L, QuirolaVasquez, J, Ragosta, F, Ramsay, G, Rau, A, Rest, A, Reynolds, T M, Rosetti, S S, Rossi, A, Rosswog, S, Sabha, N B, Carracedo, A Sagues, Salafia, O S, Salmon, L, Salvaterra, R, Savaglio, S, Sbordone, L, Schady, P, Schipani, P, Schultz, A S B, Schweyer, T, Smartt, S J, Smith, K W, Smith, M, Sollerman, J, Srivastav, S, Stanway, E R, Starling, R L C, Steeghs, D, Stratta, G, Stubbs, C W, Tanvir, N R, Testa, V, Thrane, E, Tonry, J L, Turatto, M, Ulaczyk, K, van der Horst, A J, Vergani, S D, Walton, N A, Watson, D, Wiersema, K, Wiik, K, Wyrzykowski, L, Yang, S, Yi, SX, Young, D R. Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger candidate S190814bv. ASTRONOMY & ASTROPHYSICS[J]. 2020, 643: http://dx.doi.org/10.1051/0004-6361/202037669.[7] Yi, ShuXu, Cheng, K S. Where Are the Electromagnetic-wave Counterparts of Stellar-mass Binary Black Hole Mergers?. ASTROPHYSICAL JOURNAL LETTERS[J]. 2019, 884(1): http://dx.doi.org/10.3847/2041-8213/ab459a.[8] Chen, A M, Takata, J, Yi, S X, Yu, Y W, Cheng, K S. Modelling multiwavelength emissions from PSR B1259-63/LS 2883: Effects of the stellar disc on shock radiations. ASTRONOMY & ASTROPHYSICS[J]. 2019, 627: [9] Yi, ShuXu, Cheng, K S. On the timing behaviour of PSR B1259-63 under the propeller torque from a transient accretion disc. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 476(1): 766-770, http://dx.doi.org/10.1093/mnras/sty337.[10] Yi, ShuXu, Cheng, K S, Taam, Ronald E. The Growth of Stellar Mass Black Hole Binaries Trapped in the Accretion Disks of Active Galactic Nuclei. ASTROPHYSICAL JOURNAL LETTERS[J]. 2018, 859(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000433932700002.[11] Yi, ShuXu. On gravitational wave-Cherenkov radiation from photons when passing through diffused dark matters. MODERN PHYSICS LETTERS A[J]. 2017, 32(9): https://www.webofscience.com/wos/woscc/full-record/WOS:000397961700006.[12] Yi, ShuXu, Cheng, K S. Probing the properties of the pulsar wind via studying the dispersive effects in the pulses from the pulsar companion in a double neutron-star binary system. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2017, 472(4): 4007-4012, https://www.webofscience.com/wos/woscc/full-record/WOS:000415652500019.[13] Yi, ShuXu, Zhang, ShuangNan. Detecting super-Nyquist-frequency gravitational waves using a pulsar timing array. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2016, 59(8): https://www.sciengine.com/doi/10.1007/s11433-016-0095-2.[14] Gao, XuDong, Zhang, ShuangNan, Yi, ShuXu, Xie, Yi, Fu, JianNing. Understanding the residual patterns of timing solutions of radio pulsars with a model of magnetic field oscillation. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2016, 459(1): 402-418, http://ir.bao.ac.cn/handle/114a11/5392.[15] Yi, ShuXu, Zhang, ShuangNan. The evolution of the magnetic inclination angle as an explanation of the long term red timing-noise of pulsars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2015, 454(4): 3674-3678, http://ir.ihep.ac.cn/handle/311005/229035.[16] Yi, Shuxu, Stappers, Benjamin W, Sanidas, Sotirios A, Bassa, Cees G, Janssen, Gemma H, Lyne, Andrew G, Kramer, Michael, Zhang, ShuangNan. Limits on the strength of individual gravitational wave sources using high-cadence observations of PSR B1937+21. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2014, 445(2): 1245-1252, http://ir.ihep.ac.cn/handle/311005/225193.[17] Yi, Shu-Xu, Cheng, K. S., Luo, Rui. Clumpy jets from black hole-massive star binaries as engines of Fast Radio Bursts. http://arxiv.org/abs/1811.11146.[18] Yi, Shu-Xu, Cheng, K. S.. A new approach to the GeV flare of PSR B1259-63/LS2883. http://arxiv.org/abs/1706.08715.
科研活动
学术期刊审稿经历:
Astronomy & Astrophysics
The Astrophysical Journal
Research in Astronomy and Astrophysic
参与会议
(1)The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors 2021-06-28(2)Detecting super-Nyquist-frequency gravitational waves using a pulsar timing array 国际脉冲星计时阵列年会 2015-07-19