High-energy neutrino astronomy

被引：1

作者：

Montaruli, Teresa ^{[1
]}

机构：

[1] Univ Geneva, DPNC, CH-1211 Geneva, Switzerland

来源：

12TH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP 2011), PTS 1-6 | 2012年 / 375卷

关键词：

D O I：

10.1088/1742-6596/375/1/052032

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Neutrino astronomy, conceptually conceived four decades ago, has entered an exciting phase for providing results on the quest for the sources of the observed highest energy particles. Ice Cube and ANTARES are now completed and are scanning in space and time possible signals of high energy neutrinos indicating the existence of such sources. Deep Core, inside Ice Cube, is a playground for vetoed neutrino measurement with better potential below 1 TeV. A larger and denser detector is now being discussed. ARA, now in test phase, will be composed by radio stations that could cover up to similar to 100 km(2) and aims at the highest energy region of cosmogenic neutrinos. The non observation of cosmic events is on one side a source of disappointment, on the other it represents by itself an important result. If seen in the context of a multi-messenger science, the combination of photon and cosmic ray experiment results brings invaluable information. The experimental upper bounds of the cubic-kilometer telescope Ice Cube are now below the theoretical upper bounds for extragalactic fluxes of neutrinos from optically thin sources. These are responsible for accelerating the extragalactic cosmic rays. Such limits constrain the role of gamma-ray bursts, described by the fireball picture, as sources of ultra-high energy cosmic rays. Neutrino telescopes are exciting running multi-task experiments that produce astrophysics and particle physics results some of which have been illustrated at this conference and are summarized in this report.

引用

页数：9

共 29 条

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