Entropy, heat death and black holes

AI Thread Summary
Black holes are theorized to eventually evaporate through a process known as Hawking Radiation, where particle-antiparticle pairs near the event horizon result in one particle being absorbed while the other escapes, causing the black hole to lose mass over time. This evaporation process is extremely slow, taking approximately 10^100 years for a large supermassive black hole to completely disappear. The temperature of a black hole increases as it nears evaporation, becoming significantly hotter just before it fully dissipates. The lifespan of a black hole can be estimated using a specific formula that relates its mass to the mass of the sun. Ultimately, black holes do "die," but the timescales involved are incomprehensibly long.
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Talking about the big bounce and black holes in another thread made me wonder about the life span of black holes, especially in the heat death scenario.

If the U went through heat death, does that mean that black holes would also exhaust their energy? Do black holes die, and if so, what happens? I seem to remember a theory about black holes emitting radiation and eventually evaporating, depending on their size.
 
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Yes, black holes evaporate very slowly and eventually evaporate entirely. But it takes a long, long time. As in around 10^100 years for a large supermassive black hole.
 
One can 'experiment' and possibly amuse oneself with a black hole's lifetime using the following formula:

t_{life} = 10^{66} years (M_{bh} / M_{sun})^{3}

The mass of the sun is about 2 X 10^30 kg

Reference: Black Holes A Traveler's Guide, Pickover, P.112
 
narrator said:
I seem to remember a theory about black holes emitting radiation and eventually evaporating, depending on their size.



Your talking about 'Hawking Radiation" What happens is that particle/anti particle pairs that come into existense at or near the BH event horizon become seperated. One particle gets sucked in due to the BH, and the other escapes, therefore the BH slowly losses mass over time. It has temperature, It radiates.
 
alex2515 said:
Your talking about 'Hawking Radiation" What happens is that particle/anti particle pairs that come into existense at or near the BH event horizon become seperated. One particle gets sucked in due to the BH, and the other escapes, therefore the BH slowly losses mass over time. It has temperature, It radiates.
And this temperature is usually very cold but will get very hot just before the black hole totally evaporates. From the earlier reference I listed, the temperature at the black hole event horizon is:

T_{horizon} = \frac{6 X 10^{-8} Kelvin}{M_{bh} / M_{sun}}
 
what is the current status of the field for quantum cosmology, are there any observations that support any theory of quantum cosmology? is it just cosmology during the Planck era or does it extend past the Planck era. what are the leading candidates into research into quantum cosmology and which physics departments research it? how much respect does loop quantum cosmology has compared to string cosmology with actual cosmologists?
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