The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays
@article{Sesana2008TheSG, title={The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays}, author={A. Sesana and A. Vecchio and C. Colacino}, journal={Monthly Notices of the Royal Astronomical Society}, year={2008}, volume={390}, pages={192-209} }
Massive black hole binary systems, with masses in the range � 10 4 10 10 M⊙, are among the primary sources of gravitational waves in the frequency window � 10 −9 Hz 0.1Hz. Pulsar Timing Arrays (PTAs) and the Laser Interferometer Space Antenna (LISA) are the observational means by which we will be able to observe gravitational radiation from these systems. We carry out a systematic study of the generation of the stochastic gravitational-wave background from the cosmic population of massive black… CONTINUE READING
Figures and Tables from this paper
224 Citations
Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
- Physics
- 2009
- 155
- PDF
Gravitational waves and pulsar timing: stochastic background, individual sources and parameter estimation
- Physics
- 2010
- 38
- PDF
Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band
- Physics
- 2013
- 105
- PDF
Gravitational-Wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution
- Physics, Medicine
- Science
- 2013
- 108
- PDF
Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
- Physics
- 2015
- 46
- Highly Influenced
- PDF
References
SHOWING 1-10 OF 74 REFERENCES
The Gravitational Wave Signal from Massive Black Hole Binaries and Its Contribution to the LISA Data Stream
- Physics
- 2005
- 108
- PDF
Low-Frequency Gravitational Waves from Massive Black Hole Binaries: Predictions for LISA and Pulsar Timing Arrays
- Physics
- 2003
- 200
- Highly Influential
- PDF
Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
- Physics
- 2006
- 262
- Highly Influential
- PDF
Low-Frequency Gravitational Radiation from Coalescing Massive Black Hole Binaries in Hierarchical Cosmologies
- Physics
- 2004
- 153
- PDF
Gravitational Waves from Supermassive Black Hole Coalescence in a Hierarchical Galaxy Formation Model
- Physics
- 2004
- 75
- PDF