High Energy Neutrino and Gamma-Ray Astronomy

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 2010 English Publisher:Springer International Publishing

Authors: Todor Stanev;

doi: 10.1007/978-3-030-71567-0_10 , 10.1007/978-3-540-85148-6_10

High Energy Neutrino and Gamma-Ray Astronomy

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Abstract

There are at least three arguments why we need a new type of astronomy — high energy neutrino astronomy. Low energy (MeV) neutrino astronomy exists. It detected the neutrinos from SN 1987a and continuously monitors the emission of solar neutrinos in different energy ranges. Davis and Koshiba received the 2002 Nobel prize in physics for these observations.

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University of Delaware
United States

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