Pionic Photons and Neutrinos from Cosmic Ray Accelerators
Pionic Photons and Neutrinos from Cosmic Ray Accelerators
复制标题
来自宇宙射线加速器的介子光子和中微子
DOI：
10.5506/aphyspolb.42.2525
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发表时间：
2011
期刊：
影响因子：
--
通讯作者：
F. Halzen
中科院分区：
文献类型：
--
作者：
F. Halzen
确定产生银河系和河外宇宙射线的加速器一直是几代高能伽马射线和中微子望远镜的优先使命;到目前为止，成功还遥遥无期。随着第一个对预期通量具有灵敏度的中微子探测器IceCube的完成，以及CTA的建造，探测与宇宙射线相关的伽马射线和中微子通量达到了一个新的分水岭，CTA是一个地基伽马射线探测器，将以前所未有的精度绘制和研究候选源。本文回顾了用多波长方法揭示宇宙线源的前景，并对超新星遗迹、γ射线爆发、活动星系和GZK中微子等进行了详细的讨论。
Identifying the accelerators that produce the Galactic and extragalactic cosmic rays has been a priority mission of several generations of high energy gamma ray and neutrino telescopes; success has been elusive so far. Detecting the gamma-ray and neutrino fluxes associated with cosmic rays reaches a new watershed with the completion of IceCube, the first neutrino detector with sensitivity to the anticipated fluxes, and the construction of CTA, a ground-based gamma ray detector that will map and study candidate sources with unprecedented precision. In this paper, we revisit the prospects for revealing the sources of the cosmic rays by a multiwavelength approach; after reviewing the methods, we discuss supernova remnants, gamma ray bursts, active galaxies and GZK neutrinos in some detail.
影响因子：
3.5
作者：
Ahrens, J;Bahcall, JN;Yoshida, S
通讯作者：
Yoshida, S