Video URL
https://pirsa.org/17030015Unlocking the potential of pulsar timing arrays
APA
Mingarelli, C. (2017). Unlocking the potential of pulsar timing arrays. Perimeter Institute for Theoretical Physics. https://pirsa.org/17030015
MLA
Mingarelli, Chiara. Unlocking the potential of pulsar timing arrays. Perimeter Institute for Theoretical Physics, Mar. 06, 2017, https://pirsa.org/17030015
BibTex
@misc{ scivideos_PIRSA:17030015, doi = {10.48660/17030015}, url = {https://pirsa.org/17030015}, author = {Mingarelli, Chiara}, keywords = {Other Physics}, language = {en}, title = {Unlocking the potential of pulsar timing arrays}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2017}, month = {mar}, note = {PIRSA:17030015 see, \url{https://scivideos.org/index.php/pirsa/17030015}} }
Chiara Mingarelli California Institute of Technology
Abstract
Galaxy mergers are a standard aspect of galaxy formation and evolution, and most (likely all) large galaxies contain supermassive black holes. As part of the merging process, the supermassive black holes should in-spiral together and eventually merge, generating both continuous gravitational waves and a background of gravitational radiation in the nanohertz to microhertz regime. An array of precisely timed pulsars spread across the sky can form a galactic-scale gravitational wave detector in the nanohertz band. I describe the current efforts to develop and extend the pulsar timing array concept, together with recent limits which have emerged from international efforts to constrain astrophysical phenomena at the heart of supermassive black hole mergers.