Explore Entropy & Event Horizons: Self-Taught Physics

In summary, the conversation discusses the relationship between the event horizon and entropy in black holes, as well as the breakdown of space and time at the event horizon. The speaker also mentions their interest in understanding the fundamental nature of the universe and their current reading of "Trespassing on Einstein's Lawn" by Amanda Gefter. There is a discussion about the validity of matter breaking down into pure energy at the event horizon and the concept of an observer within the black hole. It is suggested that actual textbooks and peer-reviewed papers may be more reliable sources for understanding the physics involved.
  • #1
Alicowie
1
0
I am by no means an expert in physics being largely self taught (day job is a medical student) but have an avid interest in trying to understand the fundamental nature of our universe. In doing so I'm currently reading the book "Trespassing on Einstein's Lawn" by Amanda Gefter and came across something interesting. The following is really a list of questions and postulations. I would appreciate help in understanding what might be correct or wrong and why if anybody is able to :)

Firstly, as the title mentions comes the link between the event horizon being proportianal to entropy due to a relationship between the laws of thermodynamics and black holes, in particular with the total entropy being linked to the event horizon rather than total volume of the black hole. Given E=mc2 it doesn't seem too strange that upon reaching the event horizon matter may break down into pure energy rather than remaining as matter (is this correct), especially given mass cannot travel at the speed of light. I also read that both space and time break down at the point of the event horizon (which again makes sense) but then the book begins to talk about an observer within the black hole (past the horizon) viewing out. Surely if both space and time have broken down at the event horizon it would make more sense of there was no inside of the black hole, since the term inside would have no meaning. Instead surely any particle which managed to reach the event horizon would instead be converted to energy which would then be frozen in place at the event horizon creating what from the outside might loom like a shell around something, but in reality from the frozen view point of the event horizon itself it would be impossible to conceive an "inside" but rather that would be it. This might be why rather than the entropy being linked to the volume of a black hole it is linked to the surface area - there is no volume.

As I said, being self taught it is highly possible I have missed something very elementary or made logical leaps which should not have been made so I would appreciate guidance to help correct my understanding where needed :)
 
Physics news on Phys.org
  • #2
Firstly, as the title mentions comes the link between the event horizon being proportianal to entropy due to a relationship between the laws of thermodynamics and black holes, in particular with the total entropy being linked to the event horizon rather than total volume of the black hole.
volume, for a black hole, doesn't really mean anything. However, you realize that the radius and volume of a sphere are linked right?

Given E=mc2 it doesn't seem too strange that upon reaching the event horizon matter may break down into pure energy rather than remaining as matter (is this correct),
No. There is nothing special, as far as the infalling body is concerned, about crossing the event horizon.

especially given mass cannot travel at the speed of light. I also read that both space and time break down at the point of the event horizon (which again makes sense) but then the book begins to talk about an observer within the black hole (past the horizon) viewing out. Surely if both space and time have broken down at the event horizon it would make more sense of there was no inside of the black hole, since the term inside would have no meaning.
its a mathematical breakdown, not a physical one. You use a different set of equations to describe space-time from the pov of an observer within the swarzchilde radius.

Its like how, on a map of the Earth, the surface breaks down at the poles. People can still stand on the poles even though their position is smeared over the edge of the map. They can get around fine just by using a different map.

Relativity is all about the observer. What a black hole looks like depends on where you are in relation to it. The black ball the size of the swartzchild radius is a non-rotating black hole viewed from a long way away.

The book you are reading is entertaining, but not a good reslurce for learning physics.
 
Last edited:
  • #3
Alicowie said:
have an avid interest in trying to understand the fundamental nature of our universe. In doing so I'm currently reading the book "Trespassing on Einstein's Lawn" by Amanda Gefter

You should not try to learn actual science by reading pop science books. Even the good ones aren't the same as a real textbook. Simon Bridge has correctly pointed out several ways in which the book you are reading has apparently misled you.

If you are really interested in learning about the physics you are referring to, I would strongly recommend getting an actual textbook. Sean Carroll's online lecture notes on GR are a pretty good start in the general area you seem interested in. Black hole entropy is a more advanced concept, though, and you might need to look at recent peer-reviewed papers to get a better idea of the current state of play in that area. Ultimately quantum mechanics is going to be involved, and we don't currently have a good theory of quantum gravity, so this is an area in which we don't completely understand how things work.
 

1. What is entropy and why is it important in physics?

Entropy is a measure of the disorder or randomness in a system. In physics, it is important because it helps us understand the direction of natural processes and the efficiency of energy conversions. It also plays a key role in thermodynamics, statistical mechanics, and information theory.

2. How does entropy relate to the second law of thermodynamics?

The second law of thermodynamics states that the total entropy of a closed system can only increase or remain constant, never decrease. This means that natural processes tend to move towards a state of increasing disorder and randomness. Entropy is a quantification of this tendency and helps us understand and predict the behavior of thermodynamic systems.

3. Can entropy be reversed or decreased?

In a closed system, entropy cannot be reversed or decreased. However, in an open system where energy and matter can enter or leave, it is possible for local decreases in entropy to occur. For example, living organisms are able to decrease their own entropy by taking in energy from their surroundings and using it to maintain their internal organization and order.

4. What is an event horizon and how does it relate to entropy?

An event horizon is a boundary in space around a black hole beyond which nothing, including light, can escape. Entropy is related to event horizons through the concept of the holographic principle, which suggests that the information and entropy contained within a region of space can be fully described by the information and entropy on its boundary, such as the event horizon of a black hole.

5. Can someone without a formal physics education fully understand the concepts of entropy and event horizons?

Yes, it is possible for someone without a formal physics education to understand the concepts of entropy and event horizons through self-study and research. However, a solid understanding of mathematics and physics principles is necessary to fully grasp these concepts and their implications. It may also be helpful to seek guidance from experts in the field or to read accessible explanations from reputable sources.

Similar threads

  • Special and General Relativity
Replies
8
Views
947
  • Special and General Relativity
Replies
21
Views
2K
Replies
35
Views
1K
  • Special and General Relativity
Replies
7
Views
1K
  • Special and General Relativity
Replies
3
Views
1K
  • Special and General Relativity
2
Replies
39
Views
3K
  • Special and General Relativity
Replies
24
Views
2K
  • Special and General Relativity
Replies
21
Views
2K
  • Special and General Relativity
Replies
12
Views
3K
  • Special and General Relativity
Replies
29
Views
2K
Back
Top