Probing the formation of the seeds of supermassive black holes with gravitational waves
@article{Colpi2019ProbingTF, title={Probing the formation of the seeds of supermassive black holes with gravitational waves}, author={M. Colpi}, journal={arXiv: High Energy Astrophysical Phenomena}, year={2019}, pages={241-268} }
The existence of black holes in the intermediate mass interval between one hundred and ten thousand solar masses, filling the gap between the stellar and the supermassive black holes is a key prediction to explain the origin of luminous QSOs at redshifts as large as seven. There is a sheer difficulty in forming giant black holes of billion suns in less than one billion years. This has led to the concept of seed black holes. They are high redshift intermediate mass black holes that formed during… CONTINUE READING
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SHOWING 1-10 OF 68 REFERENCES
The characteristic black hole mass resulting from direct collapse in the early Universe
- Physics
- 2013
- 99
- PDF
The imprint of massive black hole formation models on the LISA data stream
- Physics
- 2007
- 121
- Highly Influential
- PDF
Observing Supermassive Black Holes Across Cosmic Time: From Phenomenology to Physics
- Physics
- 2015
- 20
- PDF
The first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range
- Physics, Medicine
- Nature
- 2016
- 407
- Highly Influential
- PDF