The universe is crowded with black holes

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SUMMARY

Astronomers have developed a comprehensive model predicting hundreds of massive black hole (BH) mergers annually, observable with second-generation gravitational wave detectors. While black holes have been proposed as candidates for dark matter (DM), the current understanding indicates that their distribution would not match observed data, and insufficient microlensing events challenge their viability as DM. The existence of intermediate-mass black holes (IMBHs) remains uncertain due to their low number density, complicating detection efforts. The ongoing advancements in gravitational wave astronomy may provide further insights into the actual existence of these black holes.

PREREQUISITES
  • Understanding of gravitational wave detection technology
  • Familiarity with black hole physics and mergers
  • Knowledge of dark matter theories and candidates
  • Awareness of microlensing events and their significance in astrophysics
NEXT STEPS
  • Research the capabilities of second-generation gravitational wave detectors
  • Explore the implications of intermediate-mass black holes in cosmic evolution
  • Study the role of Population III stars in black hole formation
  • Investigate the relationship between gamma-ray backgrounds and black hole candidates for dark matter
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in gravitational wave astronomy, black hole studies, and dark matter research will benefit from this discussion.

wolram
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I am not sure if this is true, if it is can these black holes be the dark matter we have been searching for.

https://www.sciencedaily.com/releases/2016/06/160622144930.htm

Date:
June 22, 2016
Source:
Rochester Institute of Technology
Summary:
Astronomers have presented one of the most complete models of matter in the universe and predict hundreds of massive black hole mergers each year observable with the second generation of gravitational wave detectors.
 
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BH's have been suggested as DM before, they would be a form of MACHO.

It is generally thought that not enough micro-lensing events have been observed to verify the existence of such objects. However there is a window of possible mass for IMBHs in which their larger masses would require a low enough number density so that detections becomes too infrequent.

Another problem would be to develop an IMF that would dump most mass in massive black holes rather than stars, but perhaps PopIII remnants may provide them.

Now we are in the epoch of gravitational wave astronomy perhaps the detection rate of BH mergers will show more such objects actually exist in which case we will have to think again!

Garth
 
wolram said:
I am not sure if this is true, if it is can these black holes be the dark matter we have been searching for.

As far as I know, no, they can't. The distribution would be different from what we currently observe, and you'd need enough black holes to account for several times the mass of observable matter. It should be easy to detect these black holes if there were so many, but we do not.
 
The gamma ray background excludess all but large black holes as DM candidates. See https://arxiv.org/abs/1604.05349 for discussion. Your cited article basically acknowledges this fact, but fails to account for the deficiency in microlensing events expected from a large population of massive black holes.
 
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