Abstract Details

Name: Bhal Chandra Joshi
Affiliation: National Centre for Radio Astrophysics, Pune / Indian Institute of Technology, Roorkee
Conference ID : ASI2024_1132
Title : Ultra-long wavelength gravitational waves with the pulsar timing array experiments
Authors : Bhal Chandra Joshi on behalf of InPTA collaboration
Authors Affiliation: National Centre for Radio Astrophysics, Pune-411007,India Department of Physics, Indian Institute of Technology, Roorkee, India
Mode of Presentation: Invited
Abstract Category : Plenary
Abstract : Pulsar Timing Array experiments (PTAs), employing a collection of rapidly rotating millisecond pulsar clocks, have found a growing evidence for a stochastic gravitational wave background (SGWB) last year. This isotropic SGWB is formed by an incoherent superposition of ultra-long wavelength continuous gravitational waves believed to originate by the superposition of continuous gravitational waves emitted by an ensemble of gravitational radiation dominated in-spiralling super-massive black hole binary systems. PTAs have uncovered the characteristic spectrum of the SGWB spatially correlated across the radio pulsar pairs. A brief discussion of these experiments, with a particular emphasis on the Indo-Japnese experiment called the Indo-Japanese Pulsar Timing Array (InPTA), is presented with a review of our results jointly obtained with the European pulsar timing array (EPTA) alongwith similar results from Parkes pulsar timing array (PPTA), North American nanoHertz Observatory for gravitational waves (NANOgrav) and Chinese pulsar timing array (CPTA). After a brief peep at the current ongoing work, the implications of the current and future results of the PTAs on our knowledge of the solar system, galaxy evolution and cosmology are discussed towards the end of the presentation. The talk concludes listing potential inputs from these diverse areas of astronomy research in unvieling the astrophysics as seen through this new window of the gravitational wave messenger.