Formula for the dark energy density (dark energy formula)

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Discussion Overview

The discussion centers around a proposed formula for dark energy density, exploring its validity and applicability over different cosmological epochs. Participants examine the formula's alignment with observational data and its limitations, particularly regarding early universe conditions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant proposes a formula for dark energy density: ΩΛ = ΩbAeh/t2, suggesting it aligns with observed values from WMAP data.
  • Another participant argues that the formula implies ΩΛ > Ωb for early times, which contradicts observational requirements.
  • The original proposer acknowledges the formula's limitations for early times, stating that acceleration began around 5 billion years ago and that the concept of an event horizon does not apply in matter or radiation-dominated models.
  • A later reply suggests that the formula may only be applicable for the present time and admits the possibility of it being incomplete or coincidental.
  • Another participant checks the formula against 2013 Planck Collaboration results, indicating that it works well with the inclusion of density fluctuations at 8h−1 Mpc, leading to a revised formula: ΩΛ = σ8ΩbAeh/t2.
  • This revised formula is claimed to adequately describe the state of the Universe, aligning with empirical evidence from the Planck results.

Areas of Agreement / Disagreement

Participants express disagreement regarding the applicability of the proposed formula for early times, with some acknowledging its limitations while others question its validity as an explanation. The discussion remains unresolved regarding the completeness and general applicability of the formula.

Contextual Notes

The discussion highlights limitations related to the assumptions of the proposed formula, particularly its dependence on the epoch being considered and the definitions of cosmological parameters involved.

Alexroma
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I propose a formula for the dark energy density (dark energy formula):

ΩΛ = ΩbAeh/t2

In this equation:
ΩΛ is the dark energy density, with the estimated value from 0.712 to 0.743, according to WMAP seven-year data release [1];
Ωb is the baryon density, 0.0456 ±0.0016, according to WMAP seven-year data release [1];
Aeh is the area of a sphere represented by the event horizon of the Universe, calculated as 4πr2, where r is the distance to the event horizon (currently estimated at about 16 billion light years [2]);
t is the age of the Universe, currently 13.75 ±0.11 billion years, according to WMAP seven-year data release [1].

This formula adequately describes the state of the Universe, as the calculated value of the dark energy density is in conformity with its actual value within the established margins (from 0.712 to 0.743):
for the minimum calculated value, ΩΛ = 0.044×4π×162/13.862 = 0.737
for the maximum calculated value, ΩΛ = 0.0472×4π×162/13.642 = 0.816

References
[1] Table 8 on p. 39 of Jarosik, N., et.al. (WMAP Collaboration). Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results (PDF). nasa.gov (2010). (http://lambda.gsfc.nasa.gov/product...year/basic_results/wmap_7yr_basic_results.pdf, retrieved 2011-10-18).
[2] Tamara M. Davis, Charles H. Lineweaver. Misconceptions about the Big Bang, Scientific American (2005), and Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe, Publications of the Astronomical Society of Australia, 2004, 21, 97-109.
 
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To get good agreement with observation, we need ΩΛ≈0 for early times. Your formula would have ΩΛ> Ωb then.
 
You are right, my formula doesn't work for "early times", but there is a good reason for that: the acceleration began only about 5 billion years ago. My formula makes no sense for the times when there was no acceleration, because there wasn't cosmological event horizon either. I mean, there is no "event horizon" in the models of universes dominated by matter or by radiation.
 
Alexroma said:
You are right, my formula doesn't work for "early times", but there is a good reason for that: the acceleration began only about 5 billion years ago. My formula makes no sense for the times when there was no acceleration, because there wasn't cosmological event horizon either. I mean, there is no "event horizon" in the models of universes dominated by matter or by radiation.
Then why would you think this is an explanation?
 
Chalnoth said:
Then why would you think this is an explanation?

Good point. May be, this formula works only for the present time. May be, it's not complete. May be, it's just a coincidence that it works. I'll be working on it further.
 
Reality check: how it works with 2013 Planck Collaboration results

I checked if this dark energy formula works with the cosmological parameter values (Planck+WP+highL+BAO, Best fit) produced in 2013 by the Planck Collaboration [1].
It turned out that it perfectly works with the addition of one previously missed element, i.e. density fluctuations at 8h−1 Mpc (σ8).

The dark energy formula now looks like this:
ΩΛ = σ8ΩbAeh/t2

In this equation:
ΩΛ is the dark energy density, 0.6914, according to Planck 2013 results [1];
σ8 is the density fluctuations at 8h−1 Mpc, 0.8288, according to Planck 2013 results [1];
Ωb is the baryon density, 0.05, according to Planck 2013 results [2];
Aeh is the area of a sphere represented by the event horizon of the Universe, calculated as 4πr2, where r is the distance to the event horizon (currently estimated at about 16 billion light years [3]);
t is the age of the Universe, 13.7965 billion years, according to Planck 2013 results [1].

With all this cosmological parameter values, the formula adequately describes the state of the Universe, as the calculated value of the dark energy density (0.7004) is in accordance with the empirical evidence (0.6914).

References
[1] Planck 2013 results. I. Overview of products and scientific results. Astronomy & Astrophysics manuscript no. Planck Mission 2013. March 22, 2013. http://arxiv.org/pdf/1303.5062v1.pdf, page 36, Table 9.
[2] Planck 2013 results. I. Overview of products and scientific results. Astronomy & Astrophysics manuscript no. Planck Mission 2013. March 22, 2013. http://arxiv.org/pdf/1303.5062v1.pdf, page 34.
[3] Tamara M. Davis, Charles H. Lineweaver. Misconceptions about the Big Bang, Scientific American (2005), and Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe, Publications of the Astronomical Society of Australia, 2004, 21, 97-109.
 

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