Neutrino Propagation in Dense Astrophysical Systems

Details Neutrino Propagation in Dense Astrophysical Systems Neutrino Propagation in Dense Astrophysical Systems

2001-03-06

arxiv.org/abs/astro-ph/0103095v1

Ann.Rev.Nucl.Part.Sci. 51 (2001) 295-344

Astronomy and Astrophysics

Astrophysics

77 pages, 13 figures; a final version of this manuscript is scheduled to be published in the Annual Review of Nuclear & Partic

Scientific paper

10.1146/annurev.nucl.51.101701.1

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the fundamental properties of the neutrinos themselves. The physical sites of interest include the early universe, supernovae, and newly-born neutron stars. Detection of neutrinos from these vastly different eras using the new generation of neutrino detectors holds great promise for enhancing our understanding of neutrino-matter interactions and astrophysical phenomena.

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