13-18 December 2015
International Conference Centre Geneva
Europe/Zurich timezone

Lessons on massive black hole binaries from pulsar timing arrays

17 Dec 2015, 17:41
Level 2, Room 13 (International Conference Centre Geneva)

Level 2, Room 13

International Conference Centre Geneva

17 Rue de Varembé, 1211 Geneva


Dr Alberto Sesana (University of Birmingham)


Pulsar timing arrays (PTAs) are dramatically improving their sensitivity. Current upper limits start to be in tension with vanilla models of gravitational wave driven, circular supermassive black hole binaries (SMBHBs), although nothing can be safely ruled out yet. I will discuss how we can use current and future PTA limits to investigate the nature of SMBHBs and learn about their overall cosmic population and the dynamics bringing them to the final gravitational wave driven merger.

Primary author

Dr Alberto Sesana (University of Birmingham)

Presentation Materials