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@ThinkWiselyMatt Wear a suit to the bank and tell them “they need to please cash your money as you’re a social media influencer and not doing anything wrong. Thats where the money came from” you can say. @ThinkWiselyMatt
@ThinkWiselyMatt You should do the advice I said to say it was a bonus for being a social media influencer! It makes perfect sense to me. @ThinkWiselyMatt
The second law of thermodynamics says that the total entropy of a closed system cannot decrease. Entropy is a measure of how many microscopic states are possible in a system.
At first, black holes might seem to have very little entropy because they are described by only a few properties, such as their mass, charge, and angular momentum.
However, in 1972, physicist Jacob Bekenstein proposed that black holes should have entropy.
His argument was based on the second law of thermodynamics. If an object with entropy falls into a black hole, its entropy would no longer be directly accessible outside the black hole. If the black hole had no entropy of its own, this could lead to a decrease in the total entropy of the universe, which would conflict with the second law.
So, how much entropy does a black hole have?
In 1974, Stephen Hawking showed that black holes have a temperature and emit thermal radiation, now called Hawking radiation. This means that black holes have thermodynamic properties.
Using the relationship between energy, temperature, and entropy, physicists found that the entropy of a black hole is proportional to the area of its event horizon.
This result is known as the Bekenstein–Hawking formula:
S = A/4ℓₚ²
where S is the black hole's entropy, A is the area of its event horizon, and ℓₚ is the Planck length.
The important point is that black holes do not violate the second law of thermodynamics. Instead, they can contain an extremely large amount of entropy. For a given region of space, a black hole represents the maximum possible entropy allowed by known physics.
So, although a black hole looks simple from the outside, its entropy can be extremely large.