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. https://pirsa.org/11030114
MLA
Ross, Andreas. Gravitational wave phenomenology for LIGO, LISA and co from effective field theories. Perimeter Institute, Mar. 31, 2011, https://pirsa.org/11030114
BibTex
@misc{ pirsa_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}, year = {2011}, month = {mar}, note = {PIRSA:11030114 see, \url{https://pirsa.org}} }
Carnegie Mellon University
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Talk Type
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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.