Neutrino emission of Fermi supernova remnants
Yuan Q(袁强); Yin PF(殷鹏飞); Bi XJ(毕效军); Yuan, Q; Yin, PF; Bi, XJ
刊名ASTROPARTICLE PHYSICS
2011
卷号35期号:1页码:33-38
关键词Radiation mechanism non-thermal Supernova remnants Gamma rays Neutrinos
学科分类Astronomy & Astrophysics; Physics
DOI10.1016/j.astropartphys.2011.03.004
通讯作者[Yuan, Qiang ; Yin, Peng-Fei ; Bi, Xiao-Jun] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China ; [Bi, Xiao-Jun] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
文章类型Article
英文摘要The Fermi gamma-ray space telescope reported the observation of several Galactic supernova remnants recently, with the gamma-ray spectra well described by hadronic pp collisions. The possible neutrino emissions from these Fermi detected supernova remnants are discussed in this work, assuming the hadronic origin of the gamma-ray emission. The muon event rates induced by the neutrinos from these supernova remnants on typical km(3) neutrino telescopes, such as the IceCube and the KM3NeT, are calculated. The results show that for most of these supernova remnants the neutrino signals are too weak to be detected by the on-going or up-coming neutrino experiment. Only for the TeV bright sources RX J1713.7-3946 and possibly W28 the neutrino signals can be comparable with the atmospheric background in the TeV region, if the protons can be accelerated to very high energies. The northern hemisphere based neutrino telescope might detect the neutrinos from these two sources. (C) 2011 Elsevier B.V. All rights reserved.
类目[WOS]Astronomy & Astrophysics ; Physics, Particles & Fields
研究领域[WOS]Astronomy & Astrophysics ; Physics
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语种英语
WOS记录号WOS:000295759400006
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被引频次:7[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/236798
专题中国科学院高能物理研究所_粒子天体物理中心_期刊论文
中国科学院高能物理研究所_粒子天体物理中心
作者单位中国科学院高能物理研究所
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Yuan Q,Yin PF,Bi XJ,et al. Neutrino emission of Fermi supernova remnants[J]. ASTROPARTICLE PHYSICS,2011,35(1):33-38.
APA 袁强,殷鹏飞,毕效军,Yuan, Q,Yin, PF,&Bi, XJ.(2011).Neutrino emission of Fermi supernova remnants.ASTROPARTICLE PHYSICS,35(1),33-38.
MLA 袁强,et al."Neutrino emission of Fermi supernova remnants".ASTROPARTICLE PHYSICS 35.1(2011):33-38.
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