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08.03.2024   at 11:30 - 13:00

Journal Club: PBHs and Primordial non-gaussianity: from their abundance to gravitational waves

Speaker:听Antonio Iovino,听master student
Abstract:听The recent data releases by multiple pulsar timing array (PTA) experiments show evidence for Hellings-Downs angular correlations indicating that the observed stochastic common spectrum can be interpreted as a stochastic gravitational wave background. We study whether the signal may originate from gravitational waves induced by high-amplitude primordial curvature perturbations. Such large perturbations may be accompanied by the generation of a sizeable primordial black hole (PBH) abundance. We discuss in which scenarios the inclusion of non-Gaussianities in the computation of the abundance can lead to a signal compatible with the PTA experiments without overproducing PBHs. Eventually we briefly discuss other astrophysical and cosmological explanations for the PTA data.
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