PIRSA:21060026

Video URL

https://pirsa.org/21060026

Redshift factor from numerical relativity simulations

Navarro Albalat, S. (2021). Redshift factor from numerical relativity simulations. Perimeter Institute for Theoretical Physics. https://pirsa.org/21060026

Navarro Albalat, Sergi. Redshift factor from numerical relativity simulations. Perimeter Institute for Theoretical Physics, Jun. 08, 2021, https://pirsa.org/21060026 

          @misc{ scivideos_PIRSA:21060026,
            doi = {10.48660/21060026},
            url = {https://pirsa.org/21060026},
            author = {Navarro Albalat, Sergi},
            keywords = {Other Physics},
            language = {en},
            title = {Redshift factor from numerical relativity simulations},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2021},
            month = {jun},
            note = {PIRSA:21060026 see, \url{https://scivideos.org/pirsa/21060026}}
          }

Sergi Navarro Albalat The University of Texas at Austin

Talk numberPIRSA:21060026
DOI10.48660/21060026
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

Abstract

We present a method to extract the redshift factor in numerical relativity simulations by means of its connection to the surface gravity. We proceed to analyze the small mass ratio limit and extract 2nd and higher orders in the case of non-spinning, quasi-circular binaries. We also compare our results to analytic post-newtonian and self-force calculations.