Multi-Messenger Astrophysics With Pulsar Timing Arrays
by Luke Kelley, M. Charisi, S. Burke-Spolaor, J. Simon, L. Blecha, T. Bogdanovic, M. Colpi, J. Comerford, D. D'Orazio, M. Dotti, M. Eracleous, M. Graham, J. Greene, Z. Haiman, K. Holley-Bockelmann, E. Kara, B. Kelly, S. Komossa, S. Larson, X. Liu, C.-P. Ma, S. Noble, V. Paschalidis, R. Rafikov, V. Ravi, J. Runnoe, A. Sesana, D. Stern, M. A. Strauss, V. U, M. Volonteri, and The NANOGrav Collaboration
Published onMay 31, 2019
Multi-Messenger Astrophysics With Pulsar Timing Arrays
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Abstract
Pulsar timing arrays are on the verge of detecting low-frequency gravitational waves from supermassive black hole binaries. Multi-messenger observations will revolutionize our understanding of: 1. co-evolution of BHs with their hosts, 2. interactions of binaries with their environments, 3. fundamental physics of accretion, 4. cosmological distances
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