PBHs-as-CDM scenario and Gravitational Waves
Sala Alberto Lobo (ICE building, UAB Campus)
08/07/2019 - 00/00/0000
We argue that primordial black holes (PBHs) with the mass of an asteroid can be CDM of the Universe. In this scenario, the associated curvature perturbations will produce secondary gravitational waves with a unique spectral feature, and the amount produced will be large enough to be detected by the future space gravitational wave antenna, LISA.
Attached Documents
Generalitat de CatalunyaUniversitat de BarcelonaUniversitat Autònoma de BarcelonaUniversitat Politècnica de CatalunyaConsejo Superior de Investigaciones CientíficasCentres de Recerca de Catalunya