Light travel time since dark energy - matter equivalence

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SUMMARY

The discussion focuses on calculating the light travel time since the equivalence of matter and dark energy, assuming dark energy dominance thereafter. The user employs the Friedmann equation, specifically for a flat universe with parameters Ω0m = 0.315 and Ω0Λ = 0.685, to derive a redshift value of z = 0.296. They explore using the relationship R^(3/2) ∝ t to determine the age of the universe at this redshift, which is calculated to be approximately 9.29 billion years. The user seeks guidance on incorporating the universe's expansion into their light travel time calculations.

PREREQUISITES
  • Understanding of Friedmann equations in cosmology
  • Knowledge of redshift calculations and their implications
  • Familiarity with the concepts of dark energy and matter density parameters
  • Basic grasp of co-moving distances in an expanding universe
NEXT STEPS
  • Study the Friedmann equation under dark energy dominance conditions
  • Research the concept of co-moving distance in cosmology
  • Learn about the implications of a flat universe on light travel time calculations
  • Examine methods for calculating light travel time using cosmological parameters
USEFUL FOR

Astronomers, cosmologists, and physics students interested in the dynamics of the universe's expansion and the relationship between matter and dark energy.

leonmate
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So I'm looking to find the distance light has traveled since matter - dark energy equivalence. Assume dark energy dominance from equivalence.

Space-time has flat geometry and Ω0m = 0.315 , Ω0 = 1
Thus: Ω will equal Ω0 - Ω0m= 0.685

ρ0m (1 + zeq)3 = ρ

where: ρ0m = ρ0c * Ω0m
and: ρ = ρ0c * Ω

I used this to find z = 0.296

Next, I need to use this somehow to find the light travel time. My guess is that I should use a solution of the Friedmann equation and use it to find a time? I haven't been able to figure out how to do this so far. I think I may just need to find the right Friedmann equation for dark energy dominance and work it out from there. But, it's missing from my notes and I don't know how to get there.

Any pointers here guys?
 
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leonmate said:
Next, I need to use this somehow to find the light travel time. My guess is that I should use a solution of the Friedmann equation and use it to find a time?
That would help. You know the matter and dark energy density as function of the scale factor, this allows to calculate its derivatives (using the values observed today).
I guess assuming a linear expansion wouldn't be so completely wrong, however.
 
Ok,

Not entirely sure this is the best way to get a result but here's how I did it:

I showed in a previous question on this assignment that if you take the friedmann equation for a matter dominated universe you get:

(dR/dT)2 * R-2 = 8*π*G*ρ / 3 * R03/R3

If you solve this you eventually get to

R3/2 ∝ t

Using this relationship I found the age of the Universe at z = 0.296 (9.29 billion years) and assumed that after this moment dark energy dominates.

In order to find my light travel time do I need to take into account that the universe is expanding? Use co-moving distance maybe? We're taking a flat universe btw.
 

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