Skip to main content
Menu

Other

08.03.2024   at 11:30 - 13:00

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

Speaker: Antonio Iovino, master student
Abstract: 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.
Location: The DIAS Meetingroom Syd (V22-503a-2)
You can also join via Zoom (passcode: 060379).

The event is open to all.