The status of neutralino dark matter

Journal Article · Tue Jun 24 00:00:00 EDT 2014 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4883417· OSTI ID:22306144

Shakya, Bibhushan ^[1]

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1. Laboratory for Elementary Particle Physics, Cornell University, Ithaca, NY 14853 (United States)

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.

• OSTI ID: 22306144
• Journal Information: AIP Conference Proceedings, Vol. 1604, Issue 1; Conference: PPC 2013: 7. international conference on interconnections between particle physics and cosmology, Lead-Deadwood, SD (United States), 24 Jun - 6 Jul 2013; Other Information: (c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
GAMMA RADIATION
GEV RANGE 100-1000
NONLUMINOUS MATTER
SIGNALS
SUPERSYMMETRY