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2641por Muronga, Azwinndini“…In order to evaluate qualitatively the space-time evolution of hot and dense nuclear matter the underlying equation of state and transport coefficients must be known. …”
Publicado 2007
Enlace del recurso
Enlace del recurso
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2642
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2643
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2644
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2645“…We review the uncertainties in the spin-independent and -dependent elastic scattering cross sections of supersymmetric dark matter particles on protons and neutrons. We propagate the uncertainties in quark masses and hadronic matrix elements that are related to the $\pi$-nucleon $\sigma$ term and the spin content of the nucleon. …”
Enlace del recurso
Enlace del recurso
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2646por Marquit, Mirandu“…One of the biggest mysteries of the universe deals with questions of dark matter. There are several experiments and models being designed all over the world to try and determine what would make good dark matter candidates. …”
Publicado 2008
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2647por Menzel, R“…It explains the essentials of linear interactions and most nonlinear interactions between light and matter in both the transparent and absorbing cases. …”
Publicado 2007
Enlace del recurso
Enlace del recurso
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2648por Vahsen, S E“…Comparing these quantities with results from Dark Matter direct-detection experiments, and with results from Observational Cosmology, would enable us to establish the role of the SUSY LSP in the Dark Matter within the next decade.…”
Publicado 2008
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2649
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2650
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2651
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2652“…New results which correlate SUSY dark matter with LHC signals are presented, and a brief review of recent developments in supersymmetric and hidden sector dark matter is given. …”
Enlace del recurso
Enlace del recurso
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2653“…The growing evidence that our universe is filled with about 10 times more matter than is visible and the question: What is dark matter made of? …”
Enlace del recurso
Enlace del recurso
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2654
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2655
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2656“…We analyze scenarios in which some flavour of sneutrino is the next-to-lightest supersymmetric particle (NLSP), assuming that the gravitino is the lightest supersymmetric particle (LSP) and provides the cold dark matter. Such scenarios do not arise in the constrained supersymmetric extension of the Standard Model (CMSSM) with universal gaugino and scalar masses input at the GUT scale. …”
Enlace del recurso
Enlace del recurso
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2657“…We introduce an explicit model with technifermion matter transforming according to multiple representations of the underlying technicolor gauge group. …”
Enlace del recurso
Enlace del recurso
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2658“…These neutrinos could potentially become a source of background in the future dark matter searches aiming at nucleon cross sections in the region well below the few events per ton per year.…”
Enlace del recurso
Enlace del recurso
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2659
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2660