High energy neutrinos from astrophysical accelerators of cosmic ray nuclei

被引:62
作者
Anchordoqui, Luis A. [1 ]
Hooper, Dan [2 ]
Sarkar, Subir [3 ]
Taylor, Andrew M. [4 ]
机构
[1] Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA
[2] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[3] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England
[4] Univ Oxford, Oxford OX1 3RH, England
基金
美国国家航空航天局;
关键词
D O I
10.1016/j.astropartphys.2007.10.006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the expectation that astrophysical accelerators of cosmic ray protons would also generate neutrinos through interactions with ambient matter and/or photons. However, there will be a reduction in the predicted neutrino flux if cosmic ray sources accelerate not only protons but also significant numbers of heavier nuclei, as is indicated by recent air shower data. We consider plausible extragalactic sources such as active galactic nuclei, gamma ray bursts and starburst galaxies and demand consistency with the observed cosmic ray composition and energy spectrum at Earth after allowing for propagation through intergalactic radiation fields. This allows us to calculate the expected neutrino fluxes from the sources, normalized to the observed cosmic ray spectrum. We find that the likely signals are still within reach of next generation neutrino telescopes such as IceCube. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 13
页数:13
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