PIRSA:10060064

Interfacing numerical and analytical relativity for gravitational-wave astronomy: Status and prospects

APA

Parameswaran, A. (2010). Interfacing numerical and analytical relativity for gravitational-wave astronomy: Status and prospects. Perimeter Institute for Theoretical Physics. https://pirsa.org/10060064

MLA

Parameswaran, Ajith. Interfacing numerical and analytical relativity for gravitational-wave astronomy: Status and prospects. Perimeter Institute for Theoretical Physics, Jun. 24, 2010, https://pirsa.org/10060064

BibTex

          @misc{ scivideos_PIRSA:10060064,
            doi = {10.48660/10060064},
            url = {https://pirsa.org/10060064},
            author = {Parameswaran, Ajith},
            keywords = {},
            language = {en},
            title = { Interfacing numerical and analytical relativity for gravitational-wave astronomy: Status and prospects},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2010},
            month = {jun},
            note = {PIRSA:10060064 see, \url{https://scivideos.org/pirsa/10060064}}
          }
          

Ajith Parameswaran Tata Institute of Fundamental Research (TIFR)

Talk numberPIRSA:10060064
Talk Type Conference

Abstract

Recent progress in numerical- and analytical relativity enables us to construct analytical waveform templates coherently describing the inspiral, merger and ring down of coalescing black-hole binaries. Such waveform templates not only improve the sensitivity of the searches for gravitational waves from high-mass binaries significantly, but also the accuracy of the parameter estimation. This talk summarizes the status and prospects of different approaches of the modeling of gravitational waveform from binary black holes calibrated to numerical- relativity simulations.