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

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楼主: dejected
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Approaches on Self-Gravitating Bose-Einstein Condensatesess under the influence of gravity remains an open question, even though different approaches have already been considered. Here, we give a short introduction to the study of self-gravitating bosons in the cosmological context and in the case of an isolated object in the Newtonian regime.
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Light Sneutrino Dark Matter in the NMSSM RH sneutrinos can annihilate into either a fermion-antifermion pair, very light pseudo scalars or RH neutrinos. We investigate the prospects for their direct detection and the implications for Higgs phenomenology for each cases. We also calculate the gamma ray flux from RH sneutrino annihilation in
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Bounds on Dark Matter from CMB Observationsrmed the existence of dark matter, yet its nature remains a mystery. A well motivated dark matter candidate is the supersymmetric neutralino. While neutralinos are stable particles, they annihilate in pairs, releasing energy in the form of standard model particles. Some of this energy is absorbed by
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Searches for Galactic Dark Matter Substructure with the Fermi LAT(DM) searches via . rays. We derive robust constraints on the DM annihilation cross section from a combined analysis of ten dSphs. These constraints are applied to super-symmetric DM particle models derived from a phenomenological scan of the MSSM. We derive additional constraints from searches for
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The SuperCDMS Experimental Programtor payload, and a generation 2 experiment at SNOLAB with a 200 kg payload has been proposed. First results from the SuperCDMS Soudan experiment are expected in 2013. The Soudan and SNOLAB experiments will reach a sensitivity to the WIMP-nucleon cross section of 5 × 10. cm. and 8 × 10. cm., respecti
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