Exploring the Mysteries of Black Hole Entropy and the Holographic Principle

In summary, there is no observational evidence for Hawking radiation from black holes, but similar effects have been observed in other types of horizons. The computation of black hole entropy does not depend on the holographic principle and would be the same regardless. Hawking did not come up with the holographic principle and it took others to realize its implications.
  • #1
Edward Wij
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How exactly did Hawking compute that black hole entropy is 1/4 that of a Planck area and concluded about the holographic principle where information of a volume is located on the area of black hole? And if there was no holographic principle, how big should entropy of the black hole be with reference to Planck area (would it be say 1/8 or twice that of Planck area for example)? How is this computed?

What observational evidence is there for these? Do all observations still obey the holographic principle?
 
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  • #2
Edward Wij said:
How exactly
Black Holes and Entropy
Bekenstein, Phys. Rev. D 7, 2333, abstract

Black hole explosions?
Hawking, Nature 248, 30 - 31 (01 March 1974), abstract

There is no observational evidence for hawking radiation from black holes at all - but that is not unexpected as the radiation is so weak. There are some experiments that see similar effects in other types of effective horizons (water waves, I think currents, and whatever).
 
  • #3
Edward Wij said:
the holographic principle where information of a volume is located on the area of black hole?

Hawking didn't come up with this principle, and it is a separate concept from the computation of entropy in terms of the horizon area. See here:

http://en.wikipedia.org/wiki/Holographic_principle

Edward Wij said:
if there was no holographic principle, how big should entropy of the black hole be with reference to Planck area (would it be say 1/8 or twice that of Planck area for example)?

The computation of the black hole entropy, as above, does not depend on the holographic principle; it is the same whether that principle is true or false.
 
  • #4
mfb said:
There is no observational evidence for hawking radiation from black holes at all - but that is not unexpected as the radiation is so weak. There are some experiments that see similar effects in other types of effective horizons (water waves, I think currents, and whatever).
Yes, the primary evidence for Hawking Radiation from black holes is that when we create a horizon in some other wave medium (such as sound waves in a fluid), we get Hawking radiation emitted from the horizon.
 
  • #5
PeterDonis said:
Hawking didn't come up with this principle, and it is a separate concept from the computation of entropy in terms of the horizon area. See here:

http://en.wikipedia.org/wiki/Holographic_principle
The computation of the black hole entropy, as above, does not depend on the holographic principle; it is the same whether that principle is true or false.

Ok I realized now, but I wondered this (and caused of my initial confusion). Since Hawking was the first one to discover about the computation of entropy in the terms of the horizon area, how come he didn't conclude that all information of physical systems can be located in the area and not volume. How come it needs others (Susskind) to realize this?
 
  • #6
Edward Wij said:
Since Hawking was the first one to discover about the computation of entropy in the terms of the horizon area, how come he didn't conclude that all information of physical systems can be located in the area and not volume. How come it needs others (Susskind) to realize this?

I couldn't say. Anyway, that's not a question of physics, it's a question of history and human psychology.
 

FAQ: Exploring the Mysteries of Black Hole Entropy and the Holographic Principle

What is Black Hole entropy?

Black Hole entropy is a measure of the disorder or randomness of information within a Black Hole. It is a physical property that describes the amount of information that is contained within the event horizon of a Black Hole.

How is Black Hole entropy related to the Second Law of Thermodynamics?

The Second Law of Thermodynamics states that the total entropy of a closed system will always increase or remain constant over time. Black Hole entropy is an example of this law, as the entropy of a Black Hole can never decrease and only increases as matter falls into the Black Hole.

Can the entropy of a Black Hole ever decrease?

No, the entropy of a Black Hole can never decrease. This is due to the Second Law of Thermodynamics, which states that the total entropy of a closed system will always increase or remain constant over time.

How is Black Hole entropy calculated?

Black Hole entropy is calculated using a formula known as the Bekenstein-Hawking formula, which relates the area of the event horizon of a Black Hole to its entropy. The formula is S = kA/4ℓP2, where S is the entropy, k is the Boltzmann constant, A is the area of the event horizon, and ℓP is the Planck length.

What is the significance of Black Hole entropy?

Black Hole entropy is significant because it is linked to important concepts in physics, such as the Second Law of Thermodynamics and the idea of information preservation. It also provides insight into the fundamental nature of Black Holes and their role in the universe.

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