The Status of Neutralino Dark Matter
arXiv:1312.7505 · doi:10.1063/1.4883417
Abstract
The lightest neutralino in supersymmetry is the most studied dark matter candidate. This writeup reviews the status of neutralino dark matter in minimal and nonminimal supersymmetric models in light of recent null results at the XENON100 experiment and the observation of a 130 GeV gamma ray signal from the Galactic Center by the Fermi LAT.
Contribution to the proceedings of the CETUP* 2013 Dark Matter Program, Lead/Deadwood, South Dakota
References in corpus (6)
- Dark Matter Results from 225 Live Days of XENON100 Data
- The Well-Tempered Neutralino
- A Tentative Gamma-Ray Line from Dark Matter Annihilation at the Fermi Large Area Telescope
- Strong Evidence for Gamma-ray Line Emission from the Inner Galaxy
- Searching for the continuum spectrum photons correlated to the 130 GeV gamma-ray line
- Higgs Couplings and Naturalness in -SUSY