Dark energy and the Cosmological Constant

Click For Summary

Discussion Overview

The discussion revolves around the concepts of dark energy and the cosmological constant, particularly in relation to the expansion of the universe. Participants explore the implications of the changing rates of expansion over time and the role of dark energy in both inflation and the current accelerated expansion of the universe.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants question why the cosmological constant is still considered if the universe's expansion rate has changed over time.
  • It is noted that dark energy is not known to have been responsible for inflation, and there is uncertainty about what caused inflation.
  • Some argue that dark energy is only responsible for the acceleration of the universe's expansion, not the expansion itself.
  • One participant explains that the cosmological constant has become dominant in the latter history of the universe as matter and radiation densities have diluted over time.
  • There is a suggestion that if dark energy is not the cosmological constant, it might evolve over time and could potentially be linked to the inflaton field from an earlier stage of the universe.
  • Participants discuss the distinction between the cosmological constant (Λ) and dark energy (DE), with some asserting that they are not equivalent in all contexts.
  • Concerns are raised about the clarity of terminology and the potential for confusion in understanding the relationship between Λ and DE.
  • Numerical values for the current rate of distance expansion are provided, indicating a fractional growth rate of 1/144 of one percent per million years.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between the cosmological constant and dark energy, with some asserting they are distinct while others suggest they are equivalent. The discussion remains unresolved regarding the implications of the changing expansion rates and the role of dark energy in the early universe.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the nature of dark energy and the cosmological constant, as well as the definitions used in the context of general relativity. The mathematical implications of the Bianchi identities in relation to the cosmological constant and dark energy are also noted but not fully resolved.

  • #31
The cosmological constant business on the left hand side vs right hand side is quite silly to be honest. It's a complete triviality mathematically and there is no classical sense in which you can prefer one over the other, and in neither case are things any more or less mysterious with respect to the cosmological constant problem. (it is still 120 orders of magnitude too small on the left hand side if you want to think of it that way --curvature undergoes renormalization just like matter does when you promote the equations into the more fundamental quantum realm)

The only sense in which it might be important whether to group the term on the left vs the right is the ultimate prejudice about whether Einsteins equations holds through all energy scales. If for instance a modification occurs, then it is in fact important where you group things, b/c you may have a situation where physical quantities will differ.
 
Space news on Phys.org
  • #32
Personally I find this physical interpretation of Lambda interesting (not one that is interchangeable with energy density however.)
The paper is only two pages so people who are interested in non-DE might want to take a look.
http://arxiv.org/abs/1105.1898

It goes back to some earlier papers by John Madore on the "fuzzy sphere". quantum uncertainty in measuring angle (as opposed to position, momentum...)
  1. John Madore, “The Fuzzy sphere,” Class.Quant.Grav., 9, 69–88 (1992).
  2. John Madore, “Gravity on fuzzy space-time,” (1997), dedicated to Walter Thirring on the occasion of his 70th birthday, arXiv:gr-qc/9709002 [gr-qc].
  3. John Madore, An introduction to Noncommutative Differential Geometry and its Physical Applications., London Mathematical Society Lecture Note Series, Vol. 257 (Cambridge University Press, 2002).
 
Last edited:
  • #33
Within a certain theoretical context all curvature can be converted back and forth with energy etc---and Lambda is simply a curvature interconvertible with an energy density, with no special physical meaning outside that context. Someone only familiar with that context may well think it is a mere formality how one treats the constant---doesn't make any difference which side, treat it as an energy density if you want, and so on.

But such a person might be interested in other research lines and open to giving them a hearing, because they are different from his or her own familiar context.
Another interpretation of the Lambda constant has to do with the compactness of the phase space of geometry. And the finiteness of the number of distinguishable states of geometry. This is not the phase space of a system particles moving in a fixed geometry but actually that of the geometry itself.
It is work that is just getting started, which gives what I think is a new physical meaning to Lambda. I'll get the link.
http://arxiv.org/abs/1502.00278
Compact phase space, cosmological constant, discrete time
Carlo Rovelli, Francesca Vidotto
(Submitted on 1 Feb 2015)
We study the quantization of geometry in the presence of a cosmological constant, using a discretization with constant-curvature simplices. Phase space turns out to be compact and the Hilbert space finite dimensional for each link. Not only the intrinsic, but also the extrinsic geometry turns out to be discrete, pointing to discreetness of time, in addition to space. We work in 2+1 dimensions, but these results may be relevant also for the physical 3+1 case.
6 pages

Again it is a short paper, only 6 pages. So not terribly burdensome to read. :smile:
 
Last edited:
  • #34
marcus said:
Another interpretation of the Lambda constant has to do with the compactness of the phase space of geometry.

Yes, in the context of quantum gravity, as I understand it, having a nonzero ##\Lambda## turns out to make a big difference to the phase space of the theory. AFAIK, at the level of ordinary classical GR, this would require ##\Lambda## to be constant, not variable, so it would not exchange energy or momentum with anything else (which is consistent with our best current observations).
 
  • Like
Likes   Reactions: marcus
  • #35
You put it concisely! In addition to this incipient compact phase space idea (which needs to be worked out in 4d) there are a bunch of papers by various people which explore incorporating Lambda in QG by replacing SU(2) with the quantum group version SU(2)q. where q is a version of Lambda on the unit circle of the complex plane. Some authors:
Fairbairn and Meusburger
M. Han
S. Major
I should mention that the while the Lambda constant occurring on the LHS of the Einstein GR equation is a reciprocal area (and is formally interconvertible with energy density) what these authors are finding to be physically meaningful is the square root of Lambda, the reciprocal of a length constant. So in that work it is the square root of the Lambda we are used to, which is more fundamentally significant. that's what I should have said when I was talking about the quantum group q constant being a version of Lambda.
 
Last edited:
  • #36
This kinda reminds me of the shrinking universe idea. I still prefer the geometric interpretation - purely on the grounds of simplicity. Dark energy makes for a much more complicated universe, IMO.
 
  • #37
  • #38
Buzz Bloom said:
It involves an alternative to Lambda/Dark Energy which would also cause an acceleration of the Universe expansion.

See my replies in that thread.
 
Last edited:

Similar threads

  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 17 ·
Replies
17
Views
3K
  • · Replies 6 ·
Replies
6
Views
4K
  • · Replies 29 ·
Replies
29
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 18 ·
Replies
18
Views
2K
  • · Replies 17 ·
Replies
17
Views
4K
  • · Replies 134 ·
5
Replies
134
Views
12K
  • · Replies 4 ·
Replies
4
Views
929
  • · Replies 2 ·
Replies
2
Views
2K