LANL Abstract: High-energy Neutrino Astronomy

From: Amara Graps (amara@amara.com)
Date: Wed May 01 2002 - 11:28:49 MDT


This is a nice survey article about neutrino astronomy. I have only
skimmed it (83 pages...), but it seems very readable to people outside
the field (like me).

Amara

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Astrophysics, abstract
astro-ph/0204527

From: Dan Hooper <hooper@pheno.physics.wisc.edu>
Date: Tue, 30 Apr 2002 19:41:46 GMT (544kb)

High-energy Neutrino Astronomy: The Cosmic Ray Connection

Authors: Francis Halzen, Dan Hooper
Comments: 83 pages, 18 figures, submitted to Reports on Progress in Physics
Report-no: MADPH-02-1265

      This is a review of neutrino astronomy anchored to the
      observational fact that Nature accelerates protons and photons to
      energies in excess of $10^{20}$ and $10^{13}$ eV, respectively.
      Although the discovery of cosmic rays dates back close to a
      century, we do not know how and where they are accelerated. Basic
      elementary-particle physics dictates a universal upper limit on
      their energy of $5\times10^{19}$ eV, the so-called
      Greisen-Kuzmin-Zatsepin cutoff; however, particles in excess of
      this energy have been observed by all experiments, adding one more
      puzzle to the cosmic ray mystery. Mystery is fertile ground for
      progress: we will review the facts as well as the speculations
      about the sources including gamma ray bursts, blazars and top-down
      scenarios.

      The important conclusion is that, independently of the specific
      blueprint of the source, it takes a kilometer-scale neutrino
      observatory to detect the neutrino beam associated with the
      highest energy cosmic rays and gamma rays. We also briefly review
      the ongoing efforts to commission such instrumentation.

Paper: PostScript, PDF, or Other formats

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Computational Physics     vita:  ftp://ftp.amara.com/pub/resume.txt
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