PIRSA:24100134

Video URL

https://pirsa.org/24100134

Nano-Hz Gravitational Wave Astronomy: Its implications and promises

Gopakumar, A. (2024). Nano-Hz Gravitational Wave Astronomy: Its implications and promises. Perimeter Institute for Theoretical Physics. https://pirsa.org/24100134

Gopakumar, Achamveedu. Nano-Hz Gravitational Wave Astronomy: Its implications and promises. Perimeter Institute for Theoretical Physics, Oct. 24, 2024, https://pirsa.org/24100134 

          @misc{ scivideos_PIRSA:24100134,
            doi = {10.48660/24100134},
            url = {https://pirsa.org/24100134},
            author = {Gopakumar, Achamveedu},
            keywords = {Strong Gravity},
            language = {en},
            title = {Nano-Hz Gravitational Wave Astronomy: Its implications and promises},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {oct},
            note = {PIRSA:24100134 see, \url{https://scivideos.org/index.php/pirsa/24100134}}
          }

Achamveedu Gopakumar Tata Institute of Fundamental Research (TIFR)

Talk numberPIRSA:24100134
DOI10.48660/24100134
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Maturing Pulsar Timing Arrays are expected to inaugurate the era of nano-hertz GW astronomy in the coming days under the auspices of the International Pulsar Timing Array. Implications of ongoing IPTA efforts for astrophysics and cosmology will be discussed while focussing on PTA contributions. Ongoing IPTA efforts should lead to persistent multi-messenger GW astronomy with massive BH binaries especially during the Square Kilometre Array era, and its implications will be discussed.