Black holes and only photons going in

In summary: But the black hole radiates at a fixed rate! So if your black hole is radiating 10J/s, you cannot extract more than 10J/s (as you point out, you can extract less, but not more). And since the radiation rate for any sizable black hole is paltry at best, you'll need to wait a very long time to get a sizable sum of energy.In summary, if you want to keep the mass of a black hole from "falling in" you need to build a Dyson sphere around it. This will increase the mass-energy of the black hole, and eventually it will die out.
  • #1
stanjones
2
0
Build a Dyson sphere around a black hole (this is a thought experiment), so no more mass "falls in". Line the sphere with insanely bright lights. What happens to the black hole?

I ask this because Prof. Sean Carroll in "From Eternity To Here" discusses whether there is a limit to the entropy that can be put in a fixed space. He mentions using photons, but then drops that line of inquiry.
 
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  • #2
welcome to pf!

hi stan! welcome to pf! :smile:
stanjones said:
Build a Dyson sphere around a black hole (this is a thought experiment), so no more mass "falls in". Line the sphere with insanely bright lights. What happens to the black hole?

the photons (although they have no rest-mass) have energy and therefore mass, so the black hole gets more massive, and the Dyson sphere is now in the wrong position :wink:
 
  • #3
Amplifying on what tiny-tim said, a black hole's radius is proportional to its mass-energy. As you add photons to it, its mass-energy increases, and so does its radius. Therefore you aren't using a fixed amount of space.
 
  • #4
Thank you both. I re-read the section in Carroll's book and it makes sense now, which for such a non-intuitive subject is something.
 
  • #5
Sound like the most energy dense battery you could ever make. To charge it you turn on the lights and add photons/mass. To discharge you absorb hawking radiation and convert it to a usable form. Should work as long as you don't let the black hole completely evaporate.
 
  • #6
mrspeedybob said:
To discharge you absorb hawking radiation and convert it to a usable form. Should work as long as you don't let the black hole completely evaporate.

Unfortunately if you want to do this you have no control over the rate of energy extraction. Much better to use the penrose process, but that requires a rotating hole.
 
  • #7
Nabeshin said:
Unfortunately if you want to do this you have no control over the rate of energy extraction. Much better to use the penrose process, but that requires a rotating hole.

Sure you could control the rate of extraction...

Suppose your extraction method is thermal in nature. Hawking radiation heats the inside of the containment sphere. From there the heat either goes through a heat engine and performs work, gets radiated away from the black hole, or gets radiated back toward it where it falls back in. If you decide to run your heat engine at less then full capacity and your sphere is well insulated then most of the remaining energy from the hawking radiation will be coveted into heat and radiated right back into the hole.
 
  • #8
mrspeedybob said:
Sure you could control the rate of extraction...

Suppose your extraction method is thermal in nature. Hawking radiation heats the inside of the containment sphere. From there the heat either goes through a heat engine and performs work, gets radiated away from the black hole, or gets radiated back toward it where it falls back in. If you decide to run your heat engine at less then full capacity and your sphere is well insulated then most of the remaining energy from the hawking radiation will be coveted into heat and radiated right back into the hole.

But the black hole radiates at a fixed rate! So if your black hole is radiating 10J/s, you cannot extract more than 10J/s (as you point out, you can extract less, but not more). And since the radiation rate for any sizable black hole is paltry at best, you'll need to wait a very long time to get a sizable sum of energy.
 

Related to Black holes and only photons going in

1. What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, including light, can escape. This extreme gravitational force is caused by a large amount of mass packed into a small area.

2. How do black holes form?

Black holes are formed when a massive star dies and its core collapses under its own gravity. This collapse causes an intense gravitational pull that traps all matter and light within a certain radius, known as the event horizon.

3. How do photons behave near a black hole?

Photons, which are particles of light, are affected by the extreme gravitational pull of a black hole. They can be pulled into the black hole and cannot escape once they pass the event horizon. However, photons can also be bent and distorted by the strong gravitational field, creating fascinating visual effects.

4. Can anything escape from a black hole?

Once an object passes the event horizon of a black hole, it is unlikely that it can escape. This includes photons and any other form of matter. However, there are some theories that suggest that a form of radiation called Hawking radiation can escape from a black hole, but it has not been observed yet.

5. Can we see black holes?

Black holes themselves are invisible because no light can escape from them. However, we can observe the effects of a black hole on surrounding matter and light. For example, we can see the light from stars being bent and distorted as they orbit a black hole, giving us indirect evidence of the black hole's presence.

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