The CC and cosmological event horizon radiation

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Discussion Overview

The discussion centers on the relationship between the cosmological constant and radiation associated with the cosmological event horizon. Participants explore whether the radiation produced by this horizon is equivalent to the energy of the cosmological constant, considering implications of space's accelerating expansion.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests a potential equivalence between the radiation from the cosmological event horizon and the energy of the cosmological constant, questioning if this is a coincidence or if there is a necessary relation.
  • Another participant references a paper that seems to support the initial claim but does not clarify the connection between the cosmological constant and the radiation.
  • A different participant expresses skepticism about the paper's implications, noting that it does not suggest a relationship between the cosmological constant and the radiation from the cosmological event horizon.
  • Further elaboration includes a discussion on Killing horizons and their relation to thermal radiation, mentioning that the cosmological Killing horizon emits radiation with a temperature proportional to the square root of the cosmological constant.
  • Participants mention the complexity of horizons in more realistic cosmological models, indicating that multiple types of horizons can exist, complicating the relationship between them.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the relationship between the cosmological constant and the radiation from the cosmological event horizon. Multiple competing views and uncertainties remain regarding the implications of the discussed papers and concepts.

Contextual Notes

Participants note that the relationship between the cosmological constant and the radiation is not straightforward, with references to different types of horizons and their properties, indicating potential limitations in the current understanding.

friend
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There is Hawking radiation associated with black hole event horizons. And there is Unruh radiation associated with horizons produced by acceleration. I've also heard some suggest that there is radiation associated with the cosmological event horizon due to space itself accelerating in its expansion.

My question is would the radiation produced by the cosmological event horizon be equal to the energy of the cosmological constant? It would seem intuitively so, since each point in space is on the cosmological event horizon of some other point in space. If so, is this coincidence? Or is there some necessary relation between the CC and the acceleration of expansion such that it will produce an event horizon with the right area to produce the same radiation energy as the cosmological constant? Thanks.
 
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friend said:
This paper seems to suggest all this.

I'm not a cosmologist, but I didn't see anything in the paper that suggests that the cosmological constant and the radiation produced by the cosmological event horizon are related. What exactly in the paper suggests a link between the two?
 
Drakkith said:
[...] I didn't see anything in the paper that suggests that the cosmological constant and the radiation produced by the cosmological event horizon are related. [...]
In general, Killing horizons are associated with emission of thermal radiation at a temperature related to a property of the horizon known as "surface gravity". Some Killing horizons (such as the ordinary light cone in Minkowski space) have zero surface gravity, hence emit no thermal radiation. In contrast, the cosmological Killing horizon in de Sitter space at ##r = \sqrt{3/\Lambda}## emits thermal radiation with temperature proportional to ##\sqrt{\Lambda}##.

For more realistic FLRW-like universes, the situation is more complicated, since more than one kind of horizon can exist (e.g., particle horizon, event horizon, apparent horizon, etc). I'm finding the following book quite good (I'm still digesting it) as it contains a lot of relevant information, with a modern perspective. The Gibbons and Hawking paper from 1977 is just an early contribution to this large subject.

V. Faraoni, "Cosmological and Black Hole Apparent Horizons",
Springer Lecture Notes in Physics, 2015, ISBN 978-3-319-19239-0
 
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I see. Thanks, Strangerep.
 
strangerep said:
V. Faraoni, "Cosmological and Black Hole Apparent Horizons",
Springer Lecture Notes in Physics, 2015, ISBN 978-3-319-19239-0

Yes, thank you.
 

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