CCRG Lunch-Alberto Sesana-Supermassive black hole astrophysics with pulsar timing arrays

Date: 
11/12/2015 - 1:00pm
Speaker: 
Alberto Sesana
Speaker affiliation: 
University of Birmingham
Location: 
CIMS 2015

 

The detection of gravitational waves (GWs) may soon be a reality, opening a completely new window on the Universe. At nHz frequencies, pulsar timing arrays (PTAs) promise to detect the signal coming from the cosmological population of supermassive black hole binaries (SMBHBs) within the next few years. After reviewing the astrophysics of SMBHBs, I will describe the current status of the PTA effort, present the most recent limits, and their astrophysical implications.

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