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hep-phDec 31, 1997
authors
  • G. G. Raffelt
institutions
  • Max Planck Institute for Physics
arXiv abstractPDF
paper

Astro-Particle Physics

arXiv:hep-ph/9712548

Abstract

Recent developments of those areas of astro-particle physics are discussed that were represented at the HEP97 conference. In particular, the current status of direct and indirect dark-matter searches and of TeV neutrino and gamma-ray astronomy will be reviewed.

10 pages, 4 eps figures included, Proc. HEP97 Jerusalem, August 1997

References in corpus (10)

  • Supersymmetric Dark Matter
  • Possible Gravitational Microlensing of a Star in the Large Magellanic Cloud
  • Stars within the Large Magellanic Cloud as Potential Lenses for Observed Microlensing Events
  • Neutrino Fluxes from Active Galaxies: a Model-Independent Analysis
  • MACHO Alert 95-30 : First Real-Time Observation of Extended Source Effects in Gravitational Microlensing
  • Limits on direct detection of neutralino dark matter from b -> s gamma decays
  • Results from a Survey of Gravitational Microlensing towards M31
  • Model-Independent Comparison of Direct vs. Indirect Detection of Supersymmetric Dark Matter
  • The MACHO Project: Limits on Planetary Mass Dark Matter in the Galactic Halo from Gravitational Microlensing
  • First results from a second generation galactic axion experiment
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