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Astrophysics Luncheon Seminar

Gravitational-wave Limit Forces Re-think of Supermassive Black Hole Evolution
Presented by Vikram Ravi
California Institute of Technology

Monday, September 28, 2015
12:00 noon in 169-336

Abstract
Mergers of massive galaxies are thought to host binary supermassive black holes, which are driven to coalesce by their gravitational-wave emission. For the last decade, collaborations worldwide have been searching for signatures of these gravitational waves in millisecond radio pulsar timing data. The design sensitivities of these experiments, based on theoretical predictions for the gravitational-wave signal, have now been surpassed. However, no gravitational waves have been detected. This startling result necessitates a shift in thinking on the fates of supermassive black holes in galaxy mergers, or indeed on the supermassive black hole occupation fraction. I will describe recent results from the Parkes Pulsar Timing Array collaboration, and their implications for supermassive black hole and galaxy assembly.

JPL Contact: Jorge Pineda (4-3347)


SVCP Astrophysics


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