Mostrando 5,221 - 5,240 Resultados de 79,334 Para Buscar '"matter"', tiempo de consulta: 0.57s Limitar resultados
  1. 5221
  2. 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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    Enlace del recurso
  3. 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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    Enlace del recurso
  4. 5224
  5. 5225
  6. 5226
    por Blaschke, David, Sedrakian, David
    Publicado 2006
    “…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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    Enlace del recurso
  7. 5227
    por Lieb, Elliott H, Thirring, Walter
    Publicado 2005
    “…Lieb links the difficult question of the stability of matter with important problems in functional analysis. …”
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    Enlace del recurso
  8. 5228
  9. 5229
  10. 5230
    “…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. …”
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    Enlace del recurso
  11. 5231
  12. 5232
  13. 5233
  14. 5234
    “…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. …”
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    Enlace del recurso
  15. 5235
    por Giovannini, Massimo
    Publicado 2011
    “…The growth rate of matter perturbations is computed in a magnetized environment for the LambdaCDM and wCDM paradigms. …”
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    Enlace del recurso
  16. 5236
  17. 5237
  18. 5238
  19. 5239
    por Kono, T
    Publicado 2011
    “…It also provides a natural candidate of dark matter when the lighest SUSY particle (LSP) is stable. …”
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  20. 5240
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