PIRSA:23110050

Video URL

https://pirsa.org/23110050

The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities - VIRTUAL

Iovino, A. (2023). The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities - VIRTUAL. Perimeter Institute for Theoretical Physics. https://pirsa.org/23110050

Iovino, Antonio. The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities - VIRTUAL. Perimeter Institute for Theoretical Physics, Nov. 07, 2023, https://pirsa.org/23110050 

          @misc{ scivideos_PIRSA:23110050,
            doi = {10.48660/23110050},
            url = {https://pirsa.org/23110050},
            author = {Iovino, Antonio},
            keywords = {Particle Physics},
            language = {en},
            title = {The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities - VIRTUAL},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2023},
            month = {nov},
            note = {PIRSA:23110050 see, \url{https://scivideos.org/pirsa/23110050}}
          }

Antonio Iovino Sapienza University of Rome

Talk numberPIRSA:23110050
DOI10.48660/23110050
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

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 sizable 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.

---

Zoom link https://pitp.zoom.us/j/95261778825?pwd=QndRd0xQVFpNVzk0VXpRUkNqR1JXZz09