PIRSA:21010009

Video URL

https://pirsa.org/21010009

The parents of LIGO black holes and their hometown

Baibhav, V. (2021). The parents of LIGO black holes and their hometown . Perimeter Institute for Theoretical Physics. https://pirsa.org/21010009

Baibhav, Vishal. The parents of LIGO black holes and their hometown . Perimeter Institute for Theoretical Physics, Jan. 14, 2021, https://pirsa.org/21010009 

          @misc{ scivideos_PIRSA:21010009,
            doi = {10.48660/21010009},
            url = {https://pirsa.org/21010009},
            author = {Baibhav, Vishal},
            keywords = {Strong Gravity},
            language = {en},
            title = {The parents of LIGO black holes and their hometown },
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2021},
            month = {jan},
            note = {PIRSA:21010009 see, \url{https://scivideos.org/index.php/pirsa/21010009}}
          }

Vishal Baibhav Johns Hopkins University - Department of Physics & Astronomy

Talk numberPIRSA:21010009
DOI10.48660/21010009
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Two of the dominant channels to produce black-hole binary mergers are believed to be the isolated evolution of stellar binaries in the field and dynamical formation in star clusters. Pair instabilities prevent stellar collapse from generating black holes more massive than about 45-60 solar mass. This  “mass gap” only applies to the field formation scenario: repeated mergers in clusters can fill the gap. A similar reasoning applies to the binary’s spin parameters. If black holes are born slowly rotating, the high-spin portion of the parameter space (the “spin gap”) can only be filled by black-hole binaries that are assembled dynamically. I will discuss how such signatures are a smoking gun for the hierarchical origin, and how recent detections (GW190521 and GW190412) fit in this context. I will also talk about how we may be able to reconstruct the properties of progenitors of second-generation black holes.