基本信息
毕效军  男  博导  中国科学院高能物理研究所
电子邮件: bixj@mail.ihep.ac.cn
通信地址: 北京市玉泉路19乙高能物理所
邮政编码: 100049

研究领域

暗物质,超出粒子物理标准模型新物理

宇宙线传播,宇宙线物理

招生信息

   
招生专业
070202-粒子物理与原子核物理
070201-理论物理
070401-天体物理
招生方向
粒子天体物理,暗物质探测
新物理,对撞机,暗物质理论
宇宙线,伽马射线

教育背景

1997-09--2000-09 中科院理论物理研究所 理学博士
1994-09--1997-07 中国科学技术大学 理学硕士
学历
博士

学位
博士

工作经历

   
工作简历
2011-01--今 中科院高能物理研究所 研究员
2004-10--2010-12 中科院高能物理研究所 副研究员
2002-10--2004-10 中科院高能物理研究所 博士后
2000-10--2002-09 清华大学 博士后

出版信息

   
发表论文
[1] JCAP 07 (2024) 054. 2024, 第 2 作者  通讯作者  
[2] Phys.Rev.D 109 (2024) 12, 123033. 2024, 第 2 作者  通讯作者  
[3] Phys. Rev. D 109, 083036. 2024, 第 2 作者
[4] JCAP 01 (2024) 026. 2024, 第 2 作者
[5] Phys.Rev.D 109 (2024) 6, 063003. 2024, 第 2 作者
[6] Lv, XingJian, Bi, XiaoJun, Fang, Kun, Yin, PengFei, Zhao, MengJie. Reanalysis of the systematic uncertainties in the cosmic-ray antiproton flux. PHYSICAL REVIEW D[J]. 2024, 第 2 作者109(4): http://dx.doi.org/10.1103/PhysRevD.109.043006.
[7] Yang, Yu Ming, Bi, XiaoJun, Yin, PengFei. Constraints on Lorentz invariance violation from the LHAASO observation of GRB 221009A. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2024, 第 2 作者http://dx.doi.org/10.1088/1475-7516/2024/04/060.
[8] Phys.Rev.D 109 (2024) 2, 023023. 2024, 第 2 作者
[9] Zhao, MengJie, Bi, XiaoJun, Fang, Kun. Can the Production Cross-Section Uncertainties Explain the Cosmic Fluorine Anomaly?. PHYSICAL REVIEW D[J]. 2023, 第 2 作者107(63020): http://arxiv.org/abs/2209.03799.
[10] Xu, ZhiHui, Yuan, Qiang, Tang, ZhiCheng, Bi, XiaoJun. Potential for Constraining Propagation Parameters of Galactic Cosmic Rays with the High Energy Cosmic-radiation Detection Facility on Board China's Space Station. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2023, 第 4 作者23(8): 290-296, http://lib.cqvip.com/Qikan/Article/Detail?id=7110489782.
[11] Xiao-jun Bi, Yu Gao, Mingjie Jin, Yugen Lin, Qian-Fei Xiang. Soft scattering evaporation of dark matter subhalos by inner galactic gases. THE EUROPEAN PHYSICAL JOURNAL C[J]. 2023, 第 1 作者83(9): 1-10, http://dx.doi.org/10.1140/epjc/s10052-023-11987-w.
[12] Yao, RunMin, Bi, XiaoJun, Wang, JinWei, Yin, PengFei. Optical circular polarization induced by axionlike particles in blazars. PHYSICAL REVIEW D[J]. 2023, 第 2 作者  通讯作者  107(4): http://dx.doi.org/10.1103/PhysRevD.107.043031.
[13] Zhao, Bing, Liu, Wei, Yuan, Qiang, Hu, HongBo, Bi, XiaoJun, Wu, HanRong, Zhou, XunXiu, Guo, YiQing. Geminga SNR: Possible Candidate of the Local Cosmic-Ray Factory. ASTROPHYSICAL JOURNAL[J]. 2022, 第 5 作者926(1): http://dx.doi.org/10.3847/1538-4357/ac4416.
[14] Wang, JinWei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Electroweak dark matter model accounting for the CDF $W$-mass anomaly. PHYS.REV.D[J]. 2022, 第 2 作者106(55001): http://arxiv.org/abs/2205.00783.
[15] Gao, LinQing, Bi, XiaoJun, Wang, JinWei, Xiang, QianFei, Yin, PengFei. Exploring fermionic multiplet dark matter through precision measurements at the CEPC *. CHINESE PHYSICS C[J]. 2022, 第 2 作者46(9): 159-172, http://dx.doi.org/10.1088/1674-1137/ac7547.
[16] Wang, BingBing, Bi, XiaoJun, Fang, Kun, Lin, Sujie, Yin, PengFei. Solar modulation of cosmic proton and helium with AMS-02. PHYSICAL REVIEW D[J]. 2022, 第 2 作者106: 063006, http://arxiv.org/abs/2011.12531.
[17] Wang, JinWei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Electroweak dark matter model accounting for the CDF W-mass anomaly. PHYSICAL REVIEW D[J]. 2022, 第 2 作者  通讯作者  106(5): http://dx.doi.org/10.1103/PhysRevD.106.055001.
[18] Fang, Kun, Bi, XiaoJun. Interpretation of the puzzling gamma-ray spectrum of the Geminga halo. PHYSICAL REVIEW D[J]. 2022, 第 2 作者105(10): http://dx.doi.org/10.1103/PhysRevD.105.103007.
[19] 包力卓, 方堃, 毕效军. Slow Diffusion is Necessary to Explain the γ-Ray Pulsar Halos. Astrophys.J.[J]. 2022, 第 3 作者  通讯作者  936(2): 183, 
[20] Fang, Kun, Xi, ShaoQiang, Bao, LiZhuo, Bi, XiaoJun, Chen, EnSheng. Features of the gamma-ray pulsar halo HESS J1831-098. PHYSICAL REVIEW D[J]. 2022, 第 4 作者106(12): 
[21] HaiJunLi, XiaoJunBi, PengFeiYin. Searching for axion-like particles with the blazar observations of MAGIC and Fermi-LAT. Chinese Physics C[J]. 2022, 第 2 作者46(8): 5-11, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/ac6d4f.
[22] YuhuaYao, BingQiangQiao, WeiLiu, QiangYuan, HongBoHu, XiaoJunBi, ChaoWenYang, YiQingGuo. Constraining the cosmic ray propagation halo thickness using Fermi-LAT observations of high-latitude clouds. Chinese Physics C[J]. 2021, 第 6 作者45(10): 4-8, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/ac1064.
[23] Fang, Kun, Bi, XiaoJun, Lin, SuJie, Yuan, Qiang. Klein-Nishina Effect and the Cosmic Ray Electron Spectrum. CHINESE PHYSICS LETTERS[J]. 2021, 第 2 作者  通讯作者  38(3): 127-131, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=6964421&detailType=1.
[24] Fang, Kun, Bi, XiaoJun, Lin, SuJie, Yuan, Qiang. Klein-Nishina effect and the cosmic ray electron spectrum. 2021, 第 2 作者http://arxiv.org/abs/2007.15601.
[25] Li, HaiJun, Guo, JunGuang, Bi, XiaoJun, Lin, SuJie, Yin, PengFei. Limits on axionlike particles from Mrk 421 with 4.5-year period observations by ARGO-YBJ and Fermi-LAT. PHYSICAL REVIEW D[J]. 2021, 第 3 作者103(8): http://dx.doi.org/10.1103/PhysRevD.103.083003.
[26] JunGuangGuo, HaiJunLi, XiaoJunBi, SuJieLin, PengFeiYin. Implications of axion-like particles from the Fermi-LAT and H.E.S.S. observations of PG 1553+113 and PKS 2155−304. Chinese Physics C[J]. 2021, 第 3 作者45(2): 5-10, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/abcd2e.
[27] Wang, ShengHao, Fang, Kun, Bi, XiaoJun, Yin, PengFei. Test of the superdiffusion model in the interstellar medium around the Geminga pulsar. PHYSICAL REVIEW D[J]. 2021, 第 3 作者  通讯作者  103(6): http://dx.doi.org/10.1103/PhysRevD.103.063035.
[28] Bi, Xiaojun, Gao, Yu, Guo, Junguang, Houston, Nick, Li, Tianjun, Xu, Fangzhou, Zhang, Xin. Axion and dark photon limits from Crab Nebula high-energy gamma rays. PHYSICAL REVIEW D[J]. 2021, 第 1 作者103(4): https://www.webofscience.com/wos/woscc/full-record/WOS:000621594100002.
[29] Yuan, Qiang, Qiao, BingQiang, Guo, YiQing, Fan, YiZhong, Bi, XiaoJun. Nearby source interpretation of differences among light and medium composition spectra in cosmic rays. FRONTIERS OF PHYSICS[J]. 2021, 第 5 作者16(2): 195-200, https://journal.hep.com.cn/fop/EN/10.1007/s11467-020-0990-4.
[30] Fang, Kun, Xi, ShaoQiang, Bi, XiaoJun. Self-consistent interpretations of the multiwavelength gamma-ray spectrum of LHAASO J0621+3755. PHYSICAL REVIEW D[J]. 2021, 第 3 作者104(10): 103024, 
[31] Bi, XiaoJun, Gao, Yu, Guo, Junguang, Houston, Nick, Li, Tianjun, Xu, Fangzhou, Zhang, Xin. Axion and dark photon limits from Crab Nebula high energy gamma-rays. 2021, 第 1 作者http://arxiv.org/abs/2002.01796.
[32] Wang, JinWei, Bi, XiaoJun, Yao, RunMin, Yin, PengFei. Exploring axion dark matter through radio signals from magnetic white dwarf stars. PHYSICAL REVIEW D[J]. 2021, 第 2 作者103(11): http://dx.doi.org/10.1103/PhysRevD.103.115021.
[33] Wang, JinWei, Bi, XiaoJun, Yao, RunMin, Yin, PengFei. Explore the Axion Dark Matter through the Radio Signals from Magnetic White Dwarf Stars. 2021, 第 2 作者http://arxiv.org/abs/2101.02585.
[34] Fang, Kun, Bi, XiaoJun, Yin, PengFei. DAMPE proton spectrum indicates a slow-diffusion zone in the nearby ISM. 2020, 第 2 作者http://arxiv.org/abs/2003.13635.
[35] Guo, Junguang, Li, HaiJun, Bi, XiaoJun, Lin, SuJie, Yin, PengFei. The implications of the axion like particle from the Fermi-LAT and H.E.S.S. observations of PG 1553+113 and PKS 2155-304. 2020, 第 3 作者http://arxiv.org/abs/2002.07571.
[36] Fang, Kun, Bi, XiaoJun, Yin, PengFei. DAMPE Proton Spectrum Indicates a Slow-diffusion Zone in the nearby ISM. ASTROPHYSICAL JOURNAL[J]. 2020, 第 2 作者903(1): http://dx.doi.org/10.3847/1538-4357/abb8d7.
[37] Ahn, Y H, Bi, Xiaojun. QCD axion and neutrino physics induced by hidden flavor structure. NUCLEAR PHYSICS B[J]. 2020, 第 2 作者960: https://doaj.org/article/e3847cd238e44018a7436c2217a78814.
[38] He DongZe, Bi XiaoJun, Lin SuJie, Yin PengFei, Zhang Xin. Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission. 2020, 第 2 作者http://arxiv.org/abs/1910.05017.
[39] DongZeHe, XiaoJunBi, SuJieLin, PengFeiYin, XinZhang. Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission. Chinese Physics C[J]. 2020, 第 2 作者44(8): 1-8, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/44/8/085001.
[40] Yuan, Qiang, Qiao, BingQiang, Guo, YiQing, Fan, YiZhong, Bi, XiaoJun. Nearby source interpretation of differences among light and medium composition spectra in cosmic rays. FRONTIERSOFPHYSICS[J]. 2020, 第 5 作者16(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000579565500001.
[41] YidianChen, XiaoJunBi, MeiHuang. Holographic technicolor model and dark matter. Chinese Physics C[J]. 2020, 第 2 作者44(9): 2-9, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/44/9/093102.
[42] Yuan, Qiang, Zhu, ChengRui, Bi, XiaoJun, Wei, DaMing. Secondary cosmic-ray nucleus spectra disfavor particle transport in the Galaxy without reacceleration. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2020, 第 3 作者  通讯作者  http://dx.doi.org/10.1088/1475-7516/2020/11/027.
[43] Fang Kun, Bi XiaoJun, Yin PengFei. Possible origin of the slow-diffusion region around Geminga. 2019, 第 2 作者http://arxiv.org/abs/1903.06421.
[44] Lin, SuJie, Bi, XiaoJun, Yin, PengFei. Investigating the dark matter signal in the cosmic ray antiproton flux with the machine learning method. PHYSICAL REVIEW D[J]. 2019, 第 2 作者  通讯作者  100(10): http://dx.doi.org/10.1103/PhysRevD.100.103014.
[45] Fang, Kun, Bi, XiaoJun, Yin, PengFei. Possible origin of the slow-diffusion region around Geminga. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2019, 第 2 作者  通讯作者  488(3): 4074-4080, https://www.webofscience.com/wos/woscc/full-record/WOS:000485158400080.
[46] He, DongZe, Bi, XiaoJun, Lin, SuJie, Yin, PengFei, Zhang, Xin. Prospect for dark matter annihilation signatures from gamma-ray observation of dwarf galaxies by LHAASO. PHYSICAL REVIEW D[J]. 2019, 第 2 作者100(8): https://www.webofscience.com/wos/woscc/full-record/WOS:000489039100001.
[47] Wang, JinWei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Impact of fermionic electroweak multiplet dark matter on vacuum stability with one-loop matching. PHYSICAL REVIEW D[J]. 2019, 第 2 作者  通讯作者  99(5): http://dx.doi.org/10.1103/PhysRevD.99.055009.
[48] An Q, Asfandiyarov R, Azzarello P, Bernardini P, Bi X J, Cai M S, Chang J, Chen D Y, Chen H F, Chen J L, Chen W, Cui M Y, Cui T S, Dai H T, DAmone A, De Benedittis A, De Mitri I, Di Santo M, Ding M, Dong T K, Dong Y F, Dong Z X, Donvito G, Droz D, Duan J L, Duan K K, DUrso D, Fan R R, Fan Y Z, Fang F, Feng C Q, Feng L, Fusco P, Gallo V, Gan F J, Gao M, Gargano F, Gong K, Gong Y Z, Guo D Y, Guo J H, Guo X L, Han S X, Hu Y M, Huang G S, Huang X Y, Huang Y Y, Ionica M, Jiang W, Jin X, Kong J, Lei S J, Li S, Li W L, Li X, Li X Q, Li Y, Liang Y F, Liang Y M, Liao N H, Liu C M, Liu H, Liu J, Liu S B, Liu W Q, Liu Y, Loparco F, Luo C N, Ma M, Ma P X, Ma S Y, Ma T, Ma X Y, Marsella G, Mazziotta M N, Mo D, Niu X Y, Pan X, Peng W X, Peng X Y, Qiao R, Rao J N, Salinas M M, Shang G Z, Shen W H, Shen Z Q, Shen Z T, Song J X, Su H, Su M, Sun Z Y, Surdo A, Teng X J, Tykhonov A, Vitillo S, Wang C, Wang H, Wang H Y, Wang J Z, Wang L G, Wang Q, Wang S, Wang X H, Wang X L, Wang Y F, Wang Y P, Wang Y Z, Wang Z M, Wei D M, Wei J J, Wei Y F, Wen S C, Wu D, Wu J, Wu L B, Wu S S, Wu X, Xi K, Xia Z Q, Xu H T, Xu Z H, Xu Z L, Xu Z Z, Xue G F, Yang H B, Yang P, Yang Y Q, Yang Z L, Yao H J, Yu Y H, Yuan Q, Yue C, Zang J J, Zhang F, Zhang J Y, Zhang J Z, Zhang P F, Zhang S X, Zhang W Z, Zhang Y, Zhang Y J, Zhang Y L, Zhang Y P, Zhang Y Q, Zhang Z, Zhang Z Y, Zhao H, Zhao H Y, Zhao X F, Zhou C Y, Zhou Y, Zhu X, Zhu Y, Zimmer S. Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite. 2019, http://arxiv.org/abs/1909.12860.
[49] Fang, Kun, Bi, XiaoJun, Yin, PengFei. Reanalysis of the Pulsar Scenario to Explain the Cosmic Positron Excess Considering the Recent Developments. ASTROPHYSICALJOURNAL[J]. 2019, 第 2 作者884(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000501779300004.
[50] YiZhao, XiaoJunBi, SuJieLin, PengFeiYin. Nearby dark matter subhalo that accounts for the DAMPE excess. Chinese Physics C[J]. 2019, 第 2 作者43(8): 1-6, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/43/8/085101.
[51] Wang JinWei, 毕效军, Yin PengFei, Yu ZhaoHuan. Impact of Fermionic Electroweak Multiplet Dark Matter on Vacuum Stability with One-loop Matching. 2019, 第 2 作者http://arxiv.org/abs/1811.08743.
[52] Wang, BingBing, Bi, XiaoJun, Fang, Kun, Lin, SuJie, Yin, PengFei. Time-dependent solar modulation of cosmic rays from solar minimum to solar maximum. PHYSICAL REVIEW D[J]. 2019, 第 2 作者100(6): http://dx.doi.org/10.1103/PhysRevD.100.063006.
[53] Yi Zhao, XiaoJun Bi, PengFei Yin, Xinmin Zhang. Constraint on the velocity dependent dark matter annihilation cross section from gamma-ray and kinematic observations of ultrafaint dwarf galaxies. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2018, 第 2 作者97(6): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=1&recid=&FileName=SBQKF823B21561A5EC997D40321AA5DEB008&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[54] Fang, Kun, Bi, XiaoJun, Yin, PengFei. Discriminating local sources of high-energy cosmic electrons and positrons by current and future anisotropy measurements. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 第 2 作者  通讯作者  478(4): 5673-5683, http://dx.doi.org/10.1093/mnras/sty1463.
[55] Fang, Kun, Bi, XiaoJun, Yin, PengFei, Yuan, Qiang. Two-zone Diffusion of Electrons and Positrons from Geminga Explains the Positron Anomaly. ASTROPHYSICALJOURNAL[J]. 2018, 第 2 作者863(1): http://libir.pmo.ac.cn/handle/332002/21605.
[56] Yuan, Qiang, Liao, NengHui, Xin, YuLiang, Li, Ye, Fan, YiZhong, Zhang, Bing, Hu, HongBo, Bi, XiaoJun. Fermi Large Area Telescope Detection of Gamma-Ray Emission from the Direction of Supernova iPTF14hls. ASTROPHYSICALJOURNALLETTERS[J]. 2018, 第 8 作者854(2): http://libir.pmo.ac.cn/handle/332002/22310.
[57] JinWei Wang, XiaoJun Bi, QianFei Xiang, PengFei Yin, ZhaoHuan Yu. Exploring triplet-quadruplet fermionic dark matter at the LHC and future colliders. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2018, 第 2 作者97(3): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=1&CurRec=1&recid=&FileName=SBQK93DAD05811F918FDBE39CAB1CF3EF1AB&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[58] Zhao Yi, Bi Xiaojun, Yin Pengfei, Zhang Xinmin. Searching for γ-ray emission from Reticulum II by Fermi-LAT. CHINESE PHYSICS. C[J]. 2018, 第 2 作者42(2): 025102-1, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=6159789&detailType=1.
[59] BingBing Wang, XiaoJun Bi, SuJie Lin, PengFei Yin. Explanations of the DAMPE high energy electron/positron spectrum in the dark matter annihilation and pulsar scenarios. 中国科学:物理学 力学 天文学(英文版)[J]. 2018, 第 2 作者61(10): 19-29, http://lib.cqvip.com/Qikan/Article/Detail?id=676286259.
[60] Fang, Kun, Bi, XiaoJun, Yin, PengFei. Explanation of the Knee-like Feature in the DAMPE Cosmic e(-) + e(+) Energy Spectrum. ASTROPHYSICAL JOURNAL[J]. 2018, 第 2 作者854(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000424897400007.
[61] Wang, BingBing, Bi, XiaoJun, Lin, SuJie, Yin, PengFei. Explanations of the DAMPE high energy electron/positron spectrum in the dark matter annihilation and pulsar scenarios. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2018, 第 2 作者61(10): http://lib.cqvip.com/Qikan/Article/Detail?id=676286259.
[62] Ahmed, Waqas, Bi, XiaoJun, Li, Tianjun, Niu, JiaShu, Raza, Shabbar, Xiang, QianFei, Yin, PengFei. Status of natural supersymmetry from the generalized minimal supergravity in light of the current LHC run-2 and LUX data. PHYSICAL REVIEW D[J]. 2018, 第 2 作者98(1): 015040-1-015040-13, http://dx.doi.org/10.1103/PhysRevD.98.015040.
[63] Xiang, QianFei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Exploring fermionic dark matter via Higgs boson precision measurements at the Circular Electron Positron Collider. PHYSICAL REVIEW D[J]. 2018, 第 2 作者97(5): http://www.corc.org.cn/handle/1471x/2178095.
[64] Wang, JinWei, Bi, XiaoJun, Xiang, QianFei, Yin, PengFei, Yu, ZhaoHuan. Exploring triplet-quadruplet fermionic dark matter at the LHC and future colliders. PHYSICAL REVIEW D[J]. 2018, 第 2 作者97(3): http://www.corc.org.cn/handle/1471x/2178048.
[65] QianFei Xiang, XiaoJun Bi, PengFei Yin, ZhaoHuan Yu. Exploring fermionic dark matter via Higgs boson precision measurements at the Circular Electron Positron Collider. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2018, 第 2 作者97(5): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=1&recid=&FileName=SBQKEB912DCF8D34629A5C59776D90497D0D&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[66] Zhao, Yi, Bi, XiaoJun, Yin, PengFei, Zhang, Xinmin. Constraint on the velocity dependent dark matter annihilation cross section from gamma-ray and kinematic observations of ultrafaint dwarf galaxies. PHYSICAL REVIEW D[J]. 2018, 第 2 作者97(6): 063013-1-063013-10, http://www.corc.org.cn/handle/1471x/2178093.
[67] Xiang, QianFei, Bi, XiaoJun, Lin, SuJie, Yin, PengFei. A dark matter model that reconciles tensions between the cosmic-ray e(+/-) excess and the gamma-ray and CMB constraints. PHYSICS LETTERS B[J]. 2017, 第 2 作者773: 448-454, https://doaj.org/article/6b7f4dd4198b46a1a23719c6b6ea1bc9.
[68] Waqas Ahmed, XiaoJun Bi, Tianjun Li, Jia Shu Niu, Shabbar Raza, QianFei Xiang, PengFei Yin. Status of Natural Supersymmetry from the GmSUGRA in Light of the current LHC Run-2 and LUX data. 2017, 第 2 作者http://www.chinaxiv.org/abs/201711.02262.
[69] []. Constraints on dark matter annihilation and decay from the isotropic gamma-ray background. Chinese Physics C[J]. 2017, 41(4): 4-045104, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/41/4/045104.
[70] Bi, XiaoJun, Kang, Zhaofeng, Ko, P, Li, Jinmian, Li, Tianjun. Asymmetric dark matter bound state. PHYSICAL REVIEW D[J]. 2017, 第 1 作者  通讯作者  95(4): 043540-1-043540-9, https://www.webofscience.com/wos/woscc/full-record/WOS:000396025800006.
[71] Lin, SuJie, Bi, XiaoJun, Feng, Jie, Yin, PengFei, Yu, ZhaoHuan. Systematic study on the cosmic ray antiproton flux. PHYSICAL REVIEW D[J]. 2017, 第 2 作者96(12): 123010-1-123010-13, http://www.corc.org.cn/handle/1471x/2177813.
[72] Fang, Kun, Wang, BingBing, Bi, XiaoJun, Lin, SuJie, Yin, PengFei. Perspective on the Cosmic-ray Electron Spectrum above TeV. ASTROPHYSICAL JOURNAL[J]. 2017, 第 3 作者836(2): http://www.corc.org.cn/handle/1471x/2175675.
[73] Yuan, Qiang, Lin, SuJie, Fang, Kun, Bi, XiaoJun. Propagation of cosmic rays in the AMS-02 era. PHYSICAL REVIEW D[J]. 2017, 第 4 作者  通讯作者  95(8): 083007-1-083007-16, http://libir.pmo.ac.cn/handle/332002/22859.
[74] Wei Liu, XiaoJun Bi, SuJie Lin, BingBing Wang, PengFei Yin. Excesses of Cosmic Ray Spectra from A Single Nearby Source. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2017, 第 2 作者96(2): http://www.chinaxiv.org/abs/201711.02308.
[75] Wei Liu, XiaoJun Bi, SuJie Lin, PengFei Yin, Key Laboratory of Particle AstrophysicsInstitute of High Energy PhysicsChinese Academy of Sciences. Constraints on dark matter annihilation and decay from the isotropic gamma-ray background. CHINESEPHYSICSC. 2017, 第 2 作者41(4): http://www.corc.org.cn/handle/1471x/2177212.
[76] Xiang, QianFei, Bi, XiaoJun, Yan, QiShu, Yin, PengFei, Yu, ZhaoHuan. Measuring masses in semi-invisible final states at electron-positron colliders. PHYSICAL REVIEW D[J]. 2017, 第 2 作者95(7): http://www.corc.org.cn/handle/1471x/2177202.
[77] QianFei Xiang, XiaoJun Bi, QiShu Yan, PengFei Yin, ZhaoHuan Yu. Measuring masses in semi-invisible final states at electron-positron colliders. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2017, 第 2 作者95(7): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=1&recid=&FileName=SBQK36AD1B03DA941E3B87D4703DFE96754A&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[78] Liu, Wei, Bi, XiaoJun, Lin, SuJie, Wang, BingBing, Yin, PengFei. Excesses of cosmic ray spectra from a single nearby source. PHYSICAL REVIEW D[J]. 2017, 第 2 作者96(2): 023006-1-023006-10, http://www.corc.org.cn/handle/1471x/2176946.
[79] Zhao, Yi, Yuan, Qiang, Bi, XiaoJun, Zhu, FengRong, Jia, HuanYu. Perspective of detecting very high energy gamma-ray emission from active galactic nuclei with Large High Altitude Air Shower Observatory (LHAASO). INTERNATIONAL JOURNAL OF MODERN PHYSICS D[J]. 2016, 第 3 作者25(1): http://ir.ihep.ac.cn/handle/311005/248098.
[80] 毕效军. LHC上750GeV的双光子超出和暗物质限制. Nucl.Phys.B. 2016, 第 1 作者
[81] Bi, XiaoJun, Ding, Ran, Fan, Yizhou, Huang, Li, Li, Chuang, Li, Tianjun, Raza, Shabbar, Wang, XiaoChuan, Zhu, Bin. Promising interpretation of diphoton resonance at 750 GeV. PHYSICAL REVIEW D[J]. 2016, 第 1 作者  通讯作者  94(1): http://ir.itp.ac.cn/handle/311006/23268.
[82] XiaoJun Bi, Zhaofeng Kang, P Ko, Jinmian Li, Tianjun L. ADMonium: Asymmetric Dark Matter Bound State. 2016, 第 1 作者http://www.chinaxiv.org/abs/201608.00213.
[83] Bi, XiaoJun, Xiang, QianFei, Yin, PengFei, Yu, ZhaoHuan. The 750 GeV diphoton excess at the LHC and dark matter constraints. NUCLEAR PHYSICS B[J]. 2016, 第 1 作者909(C): 43-64, http://dx.doi.org/10.1016/j.nuclphysb.2016.04.042.
[84] Zhao, Yi, Bi, XiaoJun, Jia, HuanYu, Yin, PengFei, Zhu, FengRong. Constraint on the velocity dependent dark matter annihilation cross section from Fermi-LAT observations of dwarf galaxies. PHYSICAL REVIEW D[J]. 2016, 第 2 作者93(8): http://ir.ihep.ac.cn/handle/311005/248097.
[85] Xiang, QianFei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Searching for singlino-Higgsino dark matter in the NMSSM. PHYSICAL REVIEW D[J]. 2016, 第 2 作者94(5): http://dx.doi.org/10.1103/PhysRevD.94.055031.
[86] Yuan, Qiang, Bi, XiaoJun, Chen, GuoMing, Guo, YiQing, Lin, SuJie, Zhang, Xinmin. Implications of the AMS-02 positron fraction in cosmic rays. ASTROPARTICLE PHYSICS[J]. 2015, 第 2 作者  通讯作者  60: 1-12, http://dx.doi.org/10.1016/j.astropartphys.2014.05.005.
[87] 毕效军, 殷鹏飞, 周宁. Looking for dark matter in colliders. 物理[J]. 2015, 第 1 作者44(11): 714-721, http://ir.ihep.ac.cn/handle/311005/229257.
[88] Xiang, QianFei, Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan. Searches for dark matter signals in simplified models at future hadron colliders. PHYSICAL REVIEW D[J]. 2015, 第 2 作者91(9): http://dx.doi.org/10.1103/PhysRevD.91.095020.
[89] Bi, XiaoJun, Bian, Ligong, Huang, Weicong, Shu, Jing, Yin, PengFei. Interpretation of the Galactic Center excess and electroweak phase transition in the NMSSM. PHYSICAL REVIEW D[J]. 2015, 第 1 作者92(2): http://www.irgrid.ac.cn/handle/1471x/1114878.
[90] Lin, SuJie, Yuan, Qiang, Bi, XiaoJun. Quantitative study of the AMS-02 electron/positron spectra: Implications for pulsars and dark matter properties. PHYSICALREVIEWD[J]. 2015, 第 3 作者91(6): http://ir.ihep.ac.cn/handle/311005/228238.
[91] 毕效军. 在NMSSM模型解释银心的GeV伽马超出和电弱相变. Phys.Rev.D. 2015, 第 1 作者
[92] Yuan, Qiang, Bi, XiaoJun. Systematic study of the uncertainties in fitting the cosmic positron data by AMS-02. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2015, 第 2 作者  通讯作者  3(3): http://ir.ihep.ac.cn/handle/311005/228478.
[93] Yu, ZhaoHuan, Bi, XiaoJun, Yan, QiShu, Yin, PengFei. Tau portal dark matter models at the LHC. PHYSICAL REVIEW D[J]. 2015, 第 2 作者91(3): http://ir.ihep.ac.cn/handle/311005/228098.
[94] Yu, ZhaoHuan, Bi, XiaoJun, Yan, QiShu, Yin, PengFei. Dark matter searches in the mono-Z channel at high energy e(+)e(-) colliders. PHYSICAL REVIEW D[J]. 2014, 第 2 作者90(5): http://ir.ihep.ac.cn/handle/311005/224778.
[95] Huang, Xiaoyuan, Yuan, Qiang, Yin, PengFei, Bi, XiaoJun, Chen, Xuelei. constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations (vol 11, pg 48, 2013). JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. 2013, 第 4 作者http://ir.ihep.ac.cn/handle/311005/224729.
[96] Yin, PengFei, Yu, ZhaoHuan, Yuan, Qiang, Bi, XiaoJun. Pulsar interpretation for the AMS-02 result. PHYSICAL REVIEW D[J]. 2013, 第 4 作者88(2): http://ir.ihep.ac.cn/handle/311005/224505.
[97] Yu, ZhaoHuan, Bi, XiaoJun, Yan, QiShu, Yin, PengFei. Detecting light stop pairs in coannihilation scenarios at the LHC. PHYSICAL REVIEW D[J]. 2013, 第 2 作者87(5): http://ir.ihep.ac.cn/handle/311005/224565.
[98] Bi, XiaoJun, Yin, PengFei, Yuan, Qiang. Status of dark matter detection. FRONTIERS OF PHYSICS. 2013, 第 1 作者  通讯作者  8(6): 794-827, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=5017520&detailType=1.
[99] Yu, ZhaoHuan, Bi, XiaoJun, Yan, QiShu, Yin, PengFei. Detecting light stop pairs in coannihilation scenarios at the LHC. PHYSICAL REVIEW D[J]. 2013, 第 2 作者87(5): http://dx.doi.org/10.1103/PhysRevD.87.055007.
[100] Yin, PengFei, Yu, ZhaoHuan, Yuan, Qiang, Bi, XiaoJun. Pulsar interpretation for the AMS-02 result. PHYSICAL REVIEW D[J]. 2013, 第 4 作者88(2): http://ir.ihep.ac.cn/handle/311005/224505.
[101] Yuan, Qiang, Bi, XiaoJun. Reconcile the AMS-02 positron fraction and Fermi-LAT/HESS total e(+/-) spectra by the primary electron spectrum hardening. PHYSICS LETTERS B[J]. 2013, 第 2 作者  通讯作者  727(1-3): 1-7, http://ir.ihep.ac.cn/handle/311005/223748.
[102] Bi, XiaoJun, Yan, QiShu, Yin, PengFei. Light stop/sbottom pair production searches in the NMSSM. PHYSICAL REVIEW D[J]. 2013, 第 1 作者  通讯作者  87(3): http://dx.doi.org/10.1103/PhysRevD.87.035007.
[103] Yu, ZhaoHuan, Zheng, JiaMing, Bi, XiaoJun, Li, Zhibing, Yao, DaoXin, Zhang, HongHao. Constraining the interaction strength between dark matter and visible matter: II. Scalar, vector and spin-3/2 dark matter. NUCLEAR PHYSICS B[J]. 2012, 第 3 作者860(1): 115-151, http://dx.doi.org/10.1016/j.nuclphysb.2012.02.016.
[104] Zheng, JiaMing, Yu, ZhaoHuan, Shao, JunWen, Bi, XiaoJun, Li, Zhibing, Zhang, HongHao. Constraining the interaction strength between dark matter and visible matter: I. Fermionic dark matter. NUCLEAR PHYSICS B[J]. 2012, 第 4 作者854(2): 350-374, http://dx.doi.org/10.1016/j.nuclphysb.2011.09.009.
[105] Bi, XiaoJun, Yin, PengFei, Yuan, Qiang. Breit-Wigner enhancement considering the dark matter kinetic decoupling. PHYSICAL REVIEW D[J]. 2012, 第 1 作者  通讯作者  85(4): http://ir.ihep.ac.cn/handle/311005/224548.
[106] XiaoJun Bi, PengFei Yin, Qiang Yuan. Breit-Wigner enhancement considering the dark matter kinetic decoupling. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2012, 第 1 作者85(4): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=1&recid=&FileName=SBQKFF422E981FCD3B0865507F43871D0505&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[107] Liu, Jie, Yuan, Qiang, Bi, Xiaojun, Li, Hong, Zhang, Xinmin. NEUTRINO EMISSION FROM DARK MATTER ANNIHILATION/DECAY IN LIGHT OF COSMIC e(+/-) AND (p)over-bar DATA. INTERNATIONAL JOURNAL OF MODERN PHYSICS A[J]. 2012, 第 3 作者27(6): http://ir.iphy.ac.cn/handle/311004/49809.
[108] ZhaoHuan Yu, JiaMing Zheng, XiaoJun Bi, Zhibing Li, DaoXin Yao, HongHao Zhang. Constraining the interaction strength between dark matter and visible matter: II. Scalar, vector and spin-3/2 dark matter. NUCLEAR PHYSICS, SECTION B. 2012, 第 3 作者115-151, http://dx.doi.org/10.1016/j.nuclphysb.2012.02.016.
[109] XiaoJun Bi, QiShu Yan, PengFei Yin. Probing light stop pairs at the LHC. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2012, 第 1 作者85(3): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=2&recid=&FileName=SBQKC707736384D3F7136D507ED0023DB562&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[110] Feng, Lei, Yuan, Qiang, Yin, PengFei, Bi, XiaoJun, Li, Mingzhe. Search for dark matter signals with Fermi-LAT observation of globular clusters NGC 6388 and M15. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2012, 第 4 作者2012(4): http://dx.doi.org/10.1088/1475-7516/2012/04/030.
[111] Huang, Xiaoyuan, Yuan, Qiang, Yin, PengFei, Bi, XiaoJun, Chen, Xuelei. Constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2012, 第 4 作者http://dx.doi.org/10.1088/1475-7516/2012/11/048.
[112] Yuan, Qiang, Cao, Yixian, Liu, Jie, Yin, PengFei, Gao, Liang, Bi, XiaoJun, Zhang, Xinmin. Gamma rays from warm WIMP dark matter annihilation. PHYSICAL REVIEW D[J]. 2012, 第 6 作者86(10): http://dx.doi.org/10.1103/PhysRevD.86.103531.
[113] Liu, Jie, Yuan, Qiang, Bi, XiaoJun, Li, Hong, Zhang, Xinmin. Cosmic ray Monte Carlo: A global fitting method in studying the properties of the new sources of cosmic e(+/-) excesses. PHYSICAL REVIEW D[J]. 2012, 第 3 作者85(4): http://ir.ihep.ac.cn/handle/311005/224546.
[114] Yuan, Qiang, Liu, Siming, Bi, Xiaojun. AN ATTEMPT AT A UNIFIED MODEL FOR THE GAMMA-RAY EMISSION OF SUPERNOVA REMNANTS. ASTROPHYSICAL JOURNAL[J]. 2012, 第 3 作者761(2): http://www.irgrid.ac.cn/handle/1471x/558324.
[115] Bi, XiaoJun, Yin, PengFei, Yu, ZhaoHuan, Yuan, Qiang. Constraints and Tests of the OPERA Superluminal Neutrinos. PHYSICAL REVIEW LETTERS[J]. 2011, 第 1 作者107(24): http://www.corc.org.cn/handle/1471x/2176116.
[116] Yuan, Qiang, Yin, PengFei, Wu, XueFeng, Bi, XiaoJun, Liu, Siming, Zhang, Bing. A STATISTICAL MODEL FOR THE gamma-RAY VARIABILITY OF THE CRAB NEBULA. ASTROPHYSICAL JOURNAL LETTERS[J]. 2011, 第 4 作者730(2): http://www.irgrid.ac.cn/handle/1471x/464148.
[117] 毕效军, 秦波. 暗物质及暗物质粒子探测. 物理[J]. 2011, 第 1 作者40(1): 13, http://www.wuli.ac.cn/cn/article/id/31816.
[118] Yuan, Qiang, Yin, PengFei, Bi, XiaoJun. Neutrino emission of Fermi supernova remnants. ASTROPARTICLE PHYSICS[J]. 2011, 第 3 作者35(1): 33-38, http://dx.doi.org/10.1016/j.astropartphys.2011.03.004.
[119] Iminniyaz, Hoernisa, Chen XueLei, Bi XiaoJun, Dulat, Sayipjamal. Effects of Kinetic Decoupling on Relic Density with Sommerfeld Enhancement. COMMUNICATIONS IN THEORETICAL PHYSICS[J]. 2011, 第 3 作者56(5): 967-971, http://lib.cqvip.com/Qikan/Article/Detail?id=39985330.
[120] 李明哲, 毕效军, 张新民. WIMPs暗物质. 现代物理知识[J]. 2011, 第 2 作者28-32, http://lib.cqvip.com/Qikan/Article/Detail?id=39071016.
[121] 唐志成, 袁强, 毕效军, 陈国明. On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays. 中国物理C[J]. 2011, 第 3 作者725-734, http://ir.ihep.ac.cn/handle/311005/218048.
[122] 唐志成, 袁强, 毕效军, 陈国明. On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays. 中国物理C:英文版[J]. 2011, 第 3 作者35(8): 725-734, http://lib.cqvip.com/Qikan/Article/Detail?id=38748456.
[123] Hoernisa, Iminniyaz, 陈学雷, 毕效军, Sayipjamal, Dulat. Effects of Kinetic Decoupling on Relic Density with Sommerfeld Enhancement. 理论物理通讯:英文版[J]. 2011, 第 4 作者56(11): 967-971, http://lib.cqvip.com/Qikan/Article/Detail?id=39985330.
[124] Yuan, Qiang, Liu, Siming, Fan, Zhonghui, Bi, Xiaojun, Fryer, Christopher L. MODELING THE MULTI-WAVELENGTH EMISSION OF THE SHELL-TYPE SUPERNOVA REMNANT RX J1713.7-3946. ASTROPHYSICAL JOURNAL[J]. 2011, 第 4 作者735(2): http://dx.doi.org/10.1088/0004-637X/735/2/120.
[125] TANGZhiCheng, YUANQiang, BIXiaoJun, CHENGuoMing. On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays. Chinese Physics C[J]. 2011, 第 3 作者35(8): 725-734, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/35/8/006.
[126] Yuan, Qiang, Zhang, Bing, Bi, XiaoJun. Cosmic ray spectral hardening due to dispersion in the source injection spectra. PHYSICAL REVIEW D[J]. 2011, 第 3 作者84(4): http://www.corc.org.cn/handle/1471x/2176153.
[127] Huang, Feng, Chen, Xuelei, Yuan, Qiang, Bi, Xiaojun. Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: II. Dwarf spheroidal galaxy. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2010, 第 4 作者2010(11): http://ir.bao.ac.cn/handle/114a11/7815.
[128] Liu, Jie, Yuan, Qiang, Bi, Xiaojun, Li, Hong, Zhang, Xinmin. Markov chain Monte Carlo study on dark matter property related to the cosmic e(+/-) excesses. PHYSICAL REVIEW D[J]. 2010, 第 3 作者81(2): http://ir.ihep.ac.cn/handle/311005/240498.
[129] Bi, XiaoJun, He, XiaoGang, Ma, Ernest, Zhang, Juan. Cosmic e(+/-)s, (p)over-bars, gamma s, and neutrinos in leptocentric dark matter models. PHYSICAL REVIEW D[J]. 2010, 第 1 作者  通讯作者  81(6): http://dx.doi.org/10.1103/PhysRevD.81.063522.
[130] Qiang Yuan, PengFei Yin, XiaoJun Bi, XinMin Zhang, ShouHua Zhu. Gamma rays and neutrinos from dark matter annihilation in galaxy clusters. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2010, 第 3 作者82(2): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=9&recid=&FileName=SBQKE479DDFD6D5CACAD0A78E05292A3F2FF&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[131] Zhang, Juan, Yuan, Qiang, Bi, XiaoJun. GALACTIC DIFFUSE GAMMA RAYS-RECALCULATION BASED ON NEW MEASUREMENTS OF THE COSMIC ELECTRON SPECTRUM. ASTROPHYSICAL JOURNAL[J]. 2010, 第 3 作者720(1): 9-19, http://ir.ihep.ac.cn/handle/311005/225476.
[132] Bi, XiaoJun. CAN DARK MATTER ANNIHILATION ACCOUNT FOR THE COSMIC e(+/-) EXCESSES?. MODERN PHYSICS LETTERS A[J]. 2010, 第 1 作者  通讯作者  25(11-12): 962-968, http://ir.ihep.ac.cn/handle/311005/227789.
[133] Yuan, Qiang, Yue, Bin, Bi, XiaoJun, Chen, Xuelei, Zhang, Xinmin. Leptonic dark matter annihilation in the evolving universe: constraints and implications. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2010, 第 3 作者2010(10): http://dx.doi.org/10.1088/1475-7516/2010/10/023.
[134] Wang Bo, Yuan Qiang, Fan Chao, Zhang JianLi, Hu HongBo, Bi XiaoJun. A study on the sharp knee and fine structures of cosmic ray spectra. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2010, 第 6 作者53(5): 842-847, http://dx.doi.org/10.1007/s11433-010-0194-y.
[135] Wang Bo, Yuan Qiang, Fan Chao, Zhang Jianli, Hu Hongbo, Bi Xiaojun. A study on the sharp knee and fine structures of cosmic ray spectrat. SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY[J]. 2010, 第 6 作者53(5): 842-847, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=4078748&detailType=1.
[136] Yuan, Qiang, Yin, PengFei, Bi, XiaoJun, Zhang, XinMin, Zhu, ShouHua. Gamma rays and neutrinos from dark matter annihilation in galaxy clusters. PHYSICAL REVIEW D[J]. 2010, 第 3 作者82(2): http://ir.ihep.ac.cn/handle/311005/240493.
[137] Bi, XiaoJun, Cao, Zhen, Li, Ye, Yuan, Qiang. Testing Lorentz invariance with the ultrahigh energy cosmic ray spectrum. PHYSICAL REVIEW D[J]. 2009, 第 1 作者79(8): http://ir.ihep.ac.cn/handle/311005/240817.
[138] Hu, HongBo, Yuan, Qiang, Wang, Bo, Fan, Chao, Zhang, JianLi, Bi, XiaoJun. ON THE e(+)e(-) EXCESSES AND THE KNEE OF THE COSMIC RAY SPECTRA-HINTS OF COSMIC RAY ACCELERATION IN YOUNG SUPERNOVA REMNANTS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2009, 第 6 作者700(2): L170-L173, http://ir.ihep.ac.cn/handle/311005/240259.
[139] Bi, XiaoJun, He, XiaoGang, Yuan, Qiang. Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI. PHYSICS LETTERS B[J]. 2009, 第 1 作者678(2): 168-173, http://dx.doi.org/10.1016/j.physletb.2009.06.009.
[140] Bi, XiaoJun, Gu, PeiHong, Li, Tianjun, Zhang, Xinmin. ATIC and PAMELA results on cosmic e(+/-) excesses and neutrino masses. JOURNAL OF HIGH ENERGY PHYSICS[J]. 2009, 第 1 作者  通讯作者  2009(4): http://ir.ihep.ac.cn/handle/311005/240389.
[141] Yuan, Qiang, Bi, Xiaojun, Huang, Feng, Chen, Xuelei. Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. Galaxy cluster. JOURNALOFCOSMOLOGYANDASTROPARTICLEPHYSICS[J]. 2009, 第 2 作者2009(10): http://ir.ihep.ac.cn/handle/311005/240359.
[142] Yin, Pengfei, Yuan, Qiang, Liu, Jia, Zhang, Juan, Bi, Xiaojun, Zhu, Shouhua, Zhang, Xinmin. PAMELA data and leptonically decaying dark matter. PHYSICALREVIEWD[J]. 2009, 第 5 作者79(2): http://ir.ihep.ac.cn/handle/311005/240495.
[143] Yuan, Qiang, Bi, XiaoJun, Liu, Jia, Yin, PengFei, Zhang, Juan, Zhu, ShouHua. Clumpiness enhancement of charged cosmic rays from dark matter annihilation with Sommerfeld effect. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2009, 第 2 作者2009(12): http://ir.ihep.ac.cn/handle/311005/240356.
[144] YUANQiang, BIXiaoJun, ZHANGJuan. Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation. Chinese Physics C[J]. 2009, 第 2 作者33(10): 826-833, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/33/10/002.
[145] Pengfei Yin, Qiang Yuan, Jia Liu, Juan Zhang, Xiaojun Bi, Shouhua Zhu, Xinmin Zhang. PAMELA data and leptonically decaying dark matter. PHYSICAL REVIEW D: COVERING PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. 2009, 第 5 作者79(2): http://kns.cnki.net/KCMS/detail/detail.aspx?QueryID=0&CurRec=3&recid=&FileName=SBQKAE64C09F5DE92E5F8FDA13F009244593&DbName=SBQKLAST&DbCode=SBQK&yx=&pr=&URLID=&bsm=.
[146] 袁强, 毕效军, 张娟. Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation. 中国物理C:英文版[J]. 2009, 第 2 作者826-833, http://lib.cqvip.com/Qikan/Article/Detail?id=31674348.
[147] Bi, XiaoJun, Brandenberger, Robert, Gondolo, Paolo, Li, Tianjun, Yuan, Qiang, Zhang, Xinmin. Nonthermal production of WIMPs, cosmic e(+/-) excesses, and gamma rays from the Galactic Center. PHYSICAL REVIEW D[J]. 2009, 第 1 作者  通讯作者  80(10): http://ir.ihep.ac.cn/handle/311005/240903.
[148] Zhang, Juan, Bi, XiaoJun, Liu, Jia, Liu, SiMing, Yin, PengFei, Yuan, Qiang, Zhu, ShouHua. Discriminating different scenarios to account for the cosmic e(+/-) excess by synchrotron and inverse Compton radiation. PHYSICAL REVIEW D[J]. 2009, 第 2 作者80(2): http://ir.ihep.ac.cn/handle/311005/240489.
[149] Bi, XiaoJun, Chen, TianLu, Wang, Yue, Yuan, Qiang. THE DIFFUSE GeV-TeV gamma-RAY EMISSION OF THE CYGNUS REGION. ASTROPHYSICAL JOURNAL[J]. 2009, 第 1 作者  通讯作者  695(2): 883-887, http://ir.ihep.ac.cn/handle/311005/238676.
[150] GUPeiHong, BIXiaoJun, FENGBo, YOUNGBingLin, ZHANGXinMin. Detecting dark energy in long baseline neutrino oscillations. Chinese Physics C[J]. 2008, 第 2 作者32(7): 530-535, http://cpc.ihep.ac.cn:80/article/doi/10.1088/1674-1137/32/7/004.
[151] Bi, XiaoJun, Zhang, Juan, Yuan, Qiang. Diffuse gamma rays and (p)over-bar flux from dark matter annihilation: A model for consistent results with EGRET and cosmic ray data. PHYSICAL REVIEW D[J]. 2008, 第 1 作者  通讯作者  78(4): http://ir.ihep.ac.cn/handle/311005/240611.
[152] Yin, Pengfei, Liu, Jia, Yuan, Qiang, Bi, Xiaojun, Zhu, Shouhua. Constraints on the dark matter annihilations by neutrinos with substructure effects included. PHYSICAL REVIEW D[J]. 2008, 第 4 作者78(6): http://ir.ihep.ac.cn/handle/311005/240733.
[153] Bi, XiaoJun, Zhang, Juan, Yuan, Qiang, Zhang, JianLi, Zhao, HongSheng. The diffuse Galactic gamma-rays from dark matter annihilation. PHYSICS LETTERS B[J]. 2008, 第 1 作者  通讯作者  668(2): 87-92, http://ir.ihep.ac.cn/handle/311005/226049.
[154] 顾佩洪, 毕效军, 冯波, 杨炳麟, 张新民. Detecting dark energy in long baseline neutrino oscillations. 中国物理C:英文版[J]. 2008, 第 2 作者32(7): 530-535, http://lib.cqvip.com/Qikan/Article/Detail?id=27477261.
[155] Yuan, Qiang, Bi, XiaoJun. The galactic positron flux and dark matter substructures. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS[J]. 2007, 第 2 作者http://ir.ihep.ac.cn/handle/311005/240339.
[156] Bi, XiaoJun. Constraining supersymmetry from the satellite experiments. PHYSICAL REVIEW D[J]. 2007, 第 1 作者  通讯作者  76(12): http://ir.ihep.ac.cn/handle/311005/227971.
[157] Gu, PeiHong, Bi, XiaoJun, Zhang, Xinmin. Dark energy and neutrino CPT-violation. EUROPEAN PHYSICAL JOURNAL C[J]. 2007, 第 2 作者50(3): 655-659, http://ir.ihep.ac.cn/handle/311005/238203.
[158] Yuan, Qiang, Cao, Yixian, Liu, Jie, Yin, Peng-Fei, Gao, Liang, Bi, Xiao-Jun, Zhang, Xinmin. Gamma-rays From Warm WIMP Dark Matter Annihilation. 第 6 作者http://arxiv.org/abs/1203.5636.
[159] Fang, Kun, Bi, Xiao-Jun, Yin, Peng-fei. Discriminating Local Sources of High-Energy Cosmic-Ray Electrons and Positrons by Energy Spectrum and Anisotropy Measurements. 第 2 作者http://arxiv.org/abs/1706.03745.
[160] Liu, Jie, Yuan, Qiang, Bi, Xiao-Jun, Li, Hong, Zhang, Xinmin. CosRayMC: a global fitting method in studying the properties of the new sources of cosmic e$^{\pm}$ excesses. 第 3 作者http://arxiv.org/abs/1106.3882.
[161] Lin, Su-Jie, Bi, Xiao-Jun, Feng, Jie, Yin, Peng-Fei, Yu, Zhao-Huan. A systematic study on the cosmic ray antiproton flux. 第 2 作者http://arxiv.org/abs/1612.04001.
[162] Bi, Xiao-Jun, He, Xiao-Gang, Ma, Ernest, Zhang, Juan. Cosmic e^\pm, \bar p, \gamma and neutrino rays in leptocentric dark matter models. 第 1 作者http://arxiv.org/abs/0910.0771.
[163] Bi, Xiao-Jun, Cao, Zhen, Li, Ye, Yuan, Qiang. Testing Lorentz Invariance with Ultra High Energy Cosmic Ray Spectrum. 第 1 作者http://arxiv.org/abs/0812.0121.

科研活动

本人主要的科研活动围绕利用天体物理实验和天文观测寻找新物理信号开展,包括利用AMS-02、Fermi-LAT、DAMPE等空间实验和地面LHAASO、HESS等实验观测的高能伽马射线信号、精确宇宙线测量的数据寻找暗物质信号、寻找洛伦兹对称性破坏、寻找轴子效应等新物理信号。这些新物理问题是当前粒子物理和宇宙学研究的前沿课题,而实验室寻找往往受到很强的局限,天体物理过程有其独特的优势因而具备更高的灵敏度,比如天体物理具有实验室加速器无法获得的高能量、高能事例可以穿越宇宙学距离从而累积微小的效应等等。我们就是利用丰富天体物理和天文观测数据开展相关新物理信号的搜寻工作。暗物质问题无疑是当前新物理研究的核心问题之一,然而实验室的暗物质搜寻往往是针对某一个暗物质模型而设计,实验目标单一。丰富的天文观测可以给暗物质粒子一种模型无关的限制,我们也开展利用这些天文观测研究暗物质粒子属性的研究工作。比如,模型奇特的天文系统可能无法在标准的冷暗物质模型中实现,需要暗物质具有特殊属性,这无疑为暗物质研究提供了重要的线索。我们围绕这些观测开展研究。

科研项目
( 1 ) 暗物质探测和理论研究, 主持, 国家级, 2011-01--2013-12
( 2 ) 暗物质实验模拟, 主持, 部委级, 2010-01--2012-12
( 3 ) 暗物质暗能量的理论研究和实验预研, 参与, 国家级, 2010-01--2014-12
( 4 ) 卫星高级数据处理及科学研究, 主持, 国家级, 2016-07--2021-06
( 5 ) 暗物质粒子间接探测的本底研究, 主持, 国家级, 2018-01--2021-12

指导学生

已指导学生

余钊焕  博士研究生  070202-粒子物理与原子核物理  

方堃  博士研究生  070202-粒子物理与原子核物理  

王金伟  博士研究生  070202-粒子物理与原子核物理  

谭秀慧  博士研究生  070202-粒子物理与原子核物理  

李海军  博士研究生  070202-粒子物理与原子核物理  

郭俊广  博士研究生  070202-粒子物理与原子核物理  

现指导学生

陈恩生  博士研究生  070202-粒子物理与原子核物理  

包力卓  博士研究生  070202-粒子物理与原子核物理  

王圣豪  博士研究生  070202-粒子物理与原子核物理  

高林青  博士研究生  070202-粒子物理与原子核物理  

赵梦杰  博士研究生  070202-粒子物理与原子核物理  

张兆宸  硕士研究生  070202-粒子物理与原子核物理  

魏永健  博士研究生  070202-粒子物理与原子核物理  

姚润民  博士研究生  070202-粒子物理与原子核物理  

吕行健  硕士研究生  070202-粒子物理与原子核物理