Titlebook: Sources and Detection of Dark Matter and Dark Energy in the Universe; Proceedings of the 1 David Cline Conference proceedings 2013 Springer

amenity

Emg827

Nutrient

guardianship

Repatriate

生气地

Searches for Galactic Dark Matter Substructure with the Fermi LATre applied to super-symmetric DM particle models derived from a phenomenological scan of the MSSM. We derive additional constraints from searches for spatially extended, hard-spectrum .-ray sources lacking counterparts in other wavelengths, since they may be associated with DM substructures predicted from simulations.

东西

高原

Radiative Natural Supersymmetry with Mixed Axion/Higgsino Cold Dark Matterodel of . (RNS), with large mixing in the top squark sector, allows for finetuning at the 5–10 % level with TeV-scale top squarks and a 125 GeV light Higgs scalar .. If the strong CP problem is solved via the PQ mechanism, then we expect an axion-higgsino admixture of dark matter, where either or both the DM particles might be directly detected.

性学院

The X,100 Detectorcm. at a WIMP mass of 50 GeV/c.. A new run started in March 2011, and more than 200 live days of WIMP-search data have been acquired. Results of this second run are expected to be released in summer 2012.

Incisor

Conference proceedings 2013ter (SUSY, axions, sterile neutrinos, etc.).•Status of the indirect search for dark matter.•Status of the direct search for dark matter in detectors around the world.•The low-mass wimp search region.•The next generation of very large dark matter detectors.•New underground laboratories for dark matter search. .