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5221
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5222“…The second class has heavier gluinos and squarks but the LSP has a significant Higgsino component and should be seen by the next generation of direct dark matter detection experiments. The combined information from the 7 TeV LHC run and the next generation of direct detection experiments can test almost all of the CMSSM parameter space consistent with dark matter and EW constraints, corresponding to a fine-tuning not worse than 1:100. …”
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5223“…These scenarios do not change the observable cosmology but relic dark matter density bounds strongly depend on them. We consider few benchmark points excluded by standard cosmology dark matter bounds and suggest that loosening the dark matter constraints is necessary in order to avoid a too strong (cosmological) model dependence in the limits that are obtained for these models. …”
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5224
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5225
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5226“…This volume covers the main topics in the theory of superdense QCD matter and its application to the astrophysics of compact stars in a comprehensive and yet accessible way. …”
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5227“…Lieb links the difficult question of the stability of matter with important problems in functional analysis. …”
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5228
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5229
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5230por Lovell, Mark, Eke, Vincent, Frenk, Carlos, Gao, Liang, Jenkins, Adrian, Theuns, Tom, Wang, Jie, White, Simon D M, Boyarsky, Alexey, Ruchayskiy, Oleg“…High resolution N-body simulations of galactic cold dark matter haloes indicate that we should expect to find a few satellite galaxies around the Milky Way whose haloes have a maximum circular velocity in excess of 40 kms. …”
Publicado 2011
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5231
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5232
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5233
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5234por Buchmueller, O., Cavanaugh, R., Colling, D., De Roeck, A., Dolan, M.J., Ellis, J.R., Flacher, H., Heinemeyer, S., Isidori, G., Santos, D.Martinez, Olive, K.A., Rogerson, S., Ronga, F.J., Weiglein, G.“…We also discuss the impact of the Xenon100 constraint on spin-independent dark matter scattering, stressing the importance of taking into account the uncertainty in the pi-nucleon sigma term, that affects the spin-independent scattering matrix element, and we make predictions for spin-dependent dark matter scattering. …”
Publicado 2011
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5235por Giovannini, Massimo“…The growth rate of matter perturbations is computed in a magnetized environment for the LambdaCDM and wCDM paradigms. …”
Publicado 2011
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5236
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5237
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5238
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5239por Kono, T“…It also provides a natural candidate of dark matter when the lighest SUSY particle (LSP) is stable. …”
Publicado 2011
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5240