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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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书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe
副标题Proceedings of the 1
编辑David Cline
视频video
概述Covers the latest results from scientists from the most active universities in this hot topic.Includes supplementary material:
丛书名称Springer Proceedings in Physics
图书封面Titlebook: Sources and Detection of Dark Matter and Dark Energy in the Universe; Proceedings of the 1 David Cline Conference proceedings 2013 Springer
描述.These proceedings provide the latest results on dark matter and dark energy research. The UCLA Department of Physics and Astronomy hosted its tenth Dark Matter and Dark Energy conference in Marina del Rey and brought together all the leaders in the field. The symposium provided a scientific forum for the latest discussions in the field.. .Topics covered at the symposium:. .•Status of measurements of the equation of state of dark energy and new experiments.•The search for missing energy events at the LHC and implications for dark matter search.•Theoretical calculations on all forms of dark matter (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. .
出版日期Conference proceedings 2013
关键词Big Baryon Spectroscopic Survey; Canonical Wimps; Cosmic Microwave Background; Dark Matter Debris Flow;
版次1
doihttps://doi.org/10.1007/978-94-007-7241-0
isbn_softcover978-94-024-0675-7
isbn_ebook978-94-007-7241-0Series ISSN 0930-8989 Series E-ISSN 1867-4941
issn_series 0930-8989
copyrightSpringer Science+Business Media Dordrecht 2013
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David G. Cerdeño,Ji-Haeng Huh,Miguel Peiró,Osamu Seto
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Sources and Detection of Dark Matter and Dark Energy in the UniverseProceedings of the 1
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Finite Temperature Density Profile in SFDMt produces cores naturally and that does not require large amounts of feedback would be preferable. We find both requirements to be satisfied in the scalar field dark matter model. Here, we consider that the dark matter is an auto-interacting real scalar field in a thermal bath of temperature T with
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The X,1T Dark Matter Search Experimentand housed in a water Cherenkov muon veto at LNGS, is presented. With an experimental aim of probing WIMP interaction cross-sections above of order .. ∼ 2 × 10. cm. within 2 years of operation, X.1T will provide the sensitivity to probe a particularly favourable region of electroweak physics on a ti
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