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[会议论文] 作者：Xiao-Jun Bi,
来源：The 10th Sino-German Workshop on Galaxy Formation and Cosmol 年份：2014
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[期刊论文] 作者：Xiao-Jun Bi,Peng-Fei Yin,Qiang Yuan,
来源：黑龙江科技信息 年份：2013
本文通过对荣华二采区10...
[期刊论文] 作者：Yidian Chen,Xiao-Jun Bi,Mei Huang,
来源：中国物理C（英文版） 年份：2020
We investigate the strongly coupled minimal walking technicolor model (MWT) in the framework of a bottom-up holographic model,where the global S U(4) symmetry b...
[期刊论文] 作者：Kun Fang,Xiao-Jun Bi,Su-Jie Lin,Qiang Yuan,
来源：中国物理快报（英文版） 年份：2021
Radiative energy losses are very important in regulating the cosmic ray electron and/or positron (CRE) spectrum during their propagation in the Milky Way....
[期刊论文] 作者：Jun-Guang Guo,Hai-Jun Li,Xiao-Jun Bi,Su-Jie Lin,Peng-Fei Yin,
来源：中国物理C（英文版） 年份：2021
We investigate the axion-like particle(ALP)-photon oscillation effect in the high-energy y-ray spectra of PG 1553+113 and PKS 2155-304 measured by Fermi-LAT and...
Nearby source interpretation of differences among light and medium composition spectra in cosmic ray
[期刊论文] 作者：Qiang Yuan,Bing-Qiang Qiao,Yi-Qing Guo,Yi-Zhong Fan,Xiao-Jun Bi,
来源：物理学前沿 年份：2021
Recently the AMS-02 reported the precise measurements of the energy spectra of medium-mass com-positions(Neon,Magnesium,Silicon)of primary cosmic rays,which rev...
[期刊论文] 作者：Yang LI,You-bin DENG,Xiao-jun BI,Ya-ni LIU,Jun ZHANG,Li LI,Bin CHEN,
来源：华中科技大学学报（医学英德文版） 年份：2016
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[期刊论文] 作者：Xiang-Yu Wang,Xiao-Jun Bi,Zhen Cao,Piero Vallania,Han-Rong Wu,Da-Hai Yan,Qiang Yuan,
来源：中国物理C（英文版） 年份：2022
Extra-galactic gamma-ray sources,such as gamma-ray bursts,active galactic nuclei,starburst galaxies,are interesting and important targets for LHAASO observations.In this chapter,the prospects of detecting these sources with LHAASO and their......
Constraining the cosmic ray propagation halo thickness using Fermi-LAT observations of high-latitude
[期刊论文] 作者：Yuhua Yao,Bing-Qiang Qiao,Wei Liu,Qiang Yuan,Hong-Bo Hu,Xiao-Jun Bi,Chao-Wen Yang,Yi-Qing Guo,
来源：中国物理C（英文版） 年份：2021
The diffusive halo is a basic characteristic of cosmic ray(CR)propagation and can advance our under-standing of many CR-related phenomena and indirect dark matter.The method used to derive the halo size often has degeneracy problems and is ......
[期刊论文] 作者：Yang Chen,Xiao-Jun Bi,Kun Fang,Yi-Qing Guo,Ye Liu,P.H.Thomas Tam,S.Vernetto,Zhong-Xiang Wang,Rui-Zhi,
来源：中国物理C（英文版） 年份：2022
In the γ-ray sky,the highest fluxes come from Galactic sources:supernova remnants (SNRs),pulsars and pulsar wind nebulae,star forming regions,binaries and micro-quasars,giant molecular clouds,Galactic center,and the large extended area aro......
[期刊论文] 作者：Xiao-Jun Bi,Andrea Addazi,Konstantin Belotsky,Vitaly Beylin,Marco Cirelli,Arman Esmaili,Nicolao Fornengo,
来源：中国物理C（英文版） 年份：2022
In order to reveal the nature of dark matter,it is crucial to detect its non-gravitational interactions with the standard model particles.The traditional dark matter searches focused on the so-called weakly interacting massive particles.How......
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