Entropy, heat death and black holes

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SUMMARY

This discussion centers on the lifespan of black holes, particularly in the context of the heat death of the universe. Black holes do indeed evaporate over time through a process known as Hawking Radiation, which results in a gradual loss of mass. The formula for estimating the lifetime of a black hole is given by tlife = 1066 years (Mbh / Msun)3, where Mbh is the mass of the black hole and Msun is the mass of the sun (approximately 2 x 1030 kg). As black holes lose mass, they emit radiation and their temperature increases, particularly just before complete evaporation.

PREREQUISITES
  • Understanding of Hawking Radiation
  • Familiarity with black hole physics
  • Knowledge of thermodynamics related to black holes
  • Basic grasp of cosmological concepts such as heat death
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  • Research the implications of Hawking Radiation on black hole thermodynamics
  • Explore the concept of heat death in cosmology
  • Study the mathematical derivation of black hole evaporation formulas
  • Investigate the relationship between black hole mass and temperature at the event horizon
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Astronomers, physicists, and students of cosmology interested in the lifecycle of black holes and the fundamental principles of black hole thermodynamics.

narrator
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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 separated. 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 separated. 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}}
 

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