Σ Black Hole Masses in Universe

In summary, the estimated total mass of all black holes in the universe is less than 1% of the average density of the observable universe. This has been determined through various observations and models of galactic and stellar formation. It is predicted that all black holes, regardless of size, will eventually emit Hawking Radiation and evaporate, but this has not been directly observed yet. Some powerful explosions, such as Gamma ray bursts, may be caused by the final stages of an evaporating black hole. However, this is still speculative and other processes are thought to be more likely causes.
  • #1
CosmiCarl
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Are there any estimates of the total aggregate mass of all the black holes in the universe? How does this compare with the estimated total mass of all normal matter in the universe?
 
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  • #2
The total mass of the Universe, or any component of it can't be defined since the Universe is larger than the observable part that we can see and possibly infinite. We can however talk about the relative amounts of mass in different forms given what we can see. When we do this we find that black holes make up a tiny fraction of the average density of the Universe, much less than 1%. See one of the images on http://star-www.st-and.ac.uk/~spd3/" page for a breakdown of the mass in the Universe.
 
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  • #3
Thanks for your reply!

I should have said "the OBSERVABLE Universe". Thanks for anticipating what I MEANT to say!

OK. What evidence led to that 1% ?
 
  • #4
There is no single observation or piece of evidence, rather the models we have describing the formation and evolution of galaxies and stars, which involve many different types of observations to arrive at those theories, suggest that breakdown in relative contributions to the total density that are summarised in the figure I linked to.

Briefly though, the mass in stellar black holes is a little tricky to measure, since we don't see these very well, but can be estimated via knowledge of the Initial Mass Function (IMF) of star clusters, since only the most massive stars end as stellar black holes. For supermassive black holes (those at the centres of galaxies) we can get an estimate of their masses from seeing either their dynamic effect on matter orbiting near them or through theories suggesting relationships between the black hole mass and the spectrum of the radiation emitted from the active region near the black hole.
 
  • #5
Wallace,

Thanks for the clarification and especially the great link. It would have taken me a long time to find such a resource by myself!

One more question:

Is it generally thought that ALL black holes cause Hawking Radiation?

CosmiCarl
 
  • #6
Yes, however the prediction is that large (very massive) black holes will have a low flux of Hawking Radiation and smaller (less massive) ones will have a larger flux. This means that in principle, since Hawking Radiation removes energy from the black hole, that all Black Holes will eventually 'evaporate' releasing their energy as radiation. Bear in mind that no one has actually observed Hawking Radiation. It is possible (though I think it is thought to be unlikely) that some very powerful explosions observed mainly through Gamma rays could have been produced by the final stages of an evaporating black hole. Since the rate of Hawking radiation produced increases as the hole gets lighter, the final death throngs of a black hole is though to be a very energetic process.

Bear in mind though that this is still all speculation, and it's thought that other processes are probably more likely to be the cause of Gamma ray bursts, but it's possible that at least some of those observed were due to Hawking radiation.
 

1. What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, not even light, can escape from it. This is due to the extreme warping of space and time caused by the immense mass of the black hole.

2. How do scientists measure the mass of a black hole?

Scientists use a variety of methods to measure the mass of a black hole, including observing the orbital motion of stars or gas around the black hole, studying the effects of gravitational lensing, and analyzing the properties of the accretion disk surrounding the black hole.

3. How do black hole masses vary in the universe?

The masses of black holes can vary greatly in the universe, ranging from a few times the mass of our sun to billions of times the mass of our sun. Generally, the larger the galaxy, the larger the black hole at its center tends to be.

4. How do black hole masses affect their surroundings?

The mass of a black hole plays a crucial role in shaping its surroundings. The immense gravitational pull of a black hole can cause gas and dust to spiral into it, forming an accretion disk and releasing large amounts of energy. Black holes also have a significant impact on the growth and evolution of galaxies.

5. Are there any limitations to measuring black hole masses in the universe?

While scientists have developed various methods for measuring black hole masses, there are still limitations to these techniques. For example, it can be challenging to accurately measure the mass of a black hole in a distant galaxy, and there may be discrepancies in measurements due to uncertainties in the data or assumptions made in the calculations.

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