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The power spectrum of SUSY-CDM on sub-galactic scales

The formation of large scale structure is independent of the nature of the cold dark matter (CDM), however the fate of very small scale inhomogeneities depends on the micro-physics of the CDM particles. We investigate the matter power spectrum for scales that enter the Hubble radius well before matt...

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Detalles Bibliográficos
Autores principales: Green, A M, Hofmann, S, Schwarz, Dominik J
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1111/j.1365-2966.2004.08232.x
http://cds.cern.ch/record/644336