PIRSA:11030114

Gravitational wave phenomenology for LIGO, LISA and co from effective field theories

APA

Ross, A. (2011). Gravitational wave phenomenology for LIGO, LISA and co from effective field theories. Perimeter Institute for Theoretical Physics. https://pirsa.org/11030114

MLA

Ross, Andreas. Gravitational wave phenomenology for LIGO, LISA and co from effective field theories. Perimeter Institute for Theoretical Physics, Mar. 31, 2011, https://pirsa.org/11030114

BibTex

          @misc{ scivideos_PIRSA:11030114,
            doi = {10.48660/11030114},
            url = {https://pirsa.org/11030114},
            author = {Ross, Andreas},
            keywords = {Strong Gravity},
            language = {en},
            title = {Gravitational wave phenomenology for LIGO, LISA and co from effective field theories},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {mar},
            note = {PIRSA:11030114 see, \url{https://scivideos.org/pirsa/11030114}}
          }
          

Andreas Ross Carnegie Mellon University

Talk numberPIRSA:11030114
Source RepositoryPIRSA
Collection

Abstract

The effective field theory framework yields a systematic treatment of gravitational bound states such as binary systems. Gravitational waves emitted from compact binaries are one of the prime event candidates at direct detection experiments. Due to the multiple scales involved in the binary problem, an effective field theory treatment yields many advantages in perturbative calculations. My talk will review the setup of the effective field theory framework and report on recent progress in gravitational wave phenomenology.