Working Group Report on the "TeV Particle Astrophysics and Physics Beyond the Standard Model"
arXiv:astro-ph/0610962 · doi:10.1088/1742-6596/60/1/015
Abstract
This working group focused mainly on the complementarity among particle physics and astrophysics. The analysis of data from both fields will better constrain theoretical models. Much of the discussion focused on detecting dark matter and susy particles, and on the potential of neutrino and gamma-ray astrophysics for seeking or constraining new physics.
Report on Working Group in the TeV Particle Astrophysics Workshop II - Madison - Aug 2006
References in corpus (14)
- Cosmological dark matter annihilations into gamma-rays - a closer look
- Spectral Gamma-ray Signatures of Cosmological Dark Matter Annihilation
- A New Signature of Dark Matter Annihilations: Gamma-Rays from Intermediate-Mass Black Holes
- Annihilating Cold Dark Matter
- The unidentified TeV source (TeVJ2032+4130) and surrounding field: Final HEGRA IACT-System results
- Galactic Point Sources of TeV Antineutrinos
- Probing Planck scale physics with IceCube
- Probing Quantum Decoherence with High-Energy Neutrinos
- Neutrino Telescopes as a Direct Probe of Supersymmetry Breaking
- Prospects For Detecting Dark Matter With Neutrino Telescopes In Light Of Recent Results From Direct Detection Experiments
- Prospects for detecting Dark Matter with neutrino telescopes in Intermediate Mass Black Holes scenarios
- IceHEP High Energy Physics at the South Pole
- Propagation of supersymmetric charged sleptons at high energies
- Long-Lived Staus at Neutrino Telescopes