Gravitational waves from binary supermassive black holes missing in pulsar observations

Gravitational waves from binary supermassive black holes missing in pulsar observations

Gravitational waves are expected to be radiated by supermassive black hole binaries formed during galaxy mergers. A stochastic superposition of gravitational waves from all such binary systems would modulate the arrival times of pulses from radio pulsars. Using observations of millisecond pulsars ob...

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Bibliographic Details
Main Authors: Shannon, Ryan, Ravi, V., Lentati, L., Lasky, P., Hobbs, G., Kerr, M., Manchester, R., Coles, W., Levin, Y., Bailes, M., Bhat, N., Burke-Spolaor, S., Dai, S., Keith, M., Oslowski, S., Reardon, D., Van Strateni, W., Toomey, L., Wang, J., Wen, L., Wyithe, J., Zhu, X.
Format: Journal Article
Published: American Association for the Advancement of Science 2015
Online Access:http://hdl.handle.net/20.500.11937/4891

Internet

http://hdl.handle.net/20.500.11937/4891

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