Mass-dominated vs. radiation-dominated.

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The discussion clarifies that the terms "mass-dominated" and "radiation-dominated" refer to the energy-density of the universe being primarily influenced by mass or radiation, respectively. It explains that the energy density of radiation decreases as the universe expands, following a proportionality of ρ_rad ∝ a^(-4), while matter density decreases as ρ_mat ∝ a^(-3). The equivalence epoch, denoted as a_eq, is the point at which both densities are equal, marking the transition from a radiation-dominated era to a matter-dominated era. Additionally, it notes that Hubble's law describes the expansion of the universe but is not directly proportional to the expansion factor in cosmological terms. Understanding these concepts is crucial for grasping the dynamics of the universe's expansion.
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I have a simple question:
What does it mean that the universe is mass-dominated or radiation-dominated?
I can't find the answer anywhere on the internet. But i kind of think that it means that the energy-density of the universe is either dominated by the energy from mass or radiation. Is this correct? Thanks alot.
 
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Yes, that's correct.
 
Thanks!
 
If you call a the expansion factor, the energy density of the radiation goes as \rho_{rad}\propto a^{-4}, while for the matter you have \rho_{mat}\propto a^{-3}. If you plot logarithmically these quantities, you will see that at a certain a_{eq} the two densities will be equal: there it is the equivalence epoch. Before equivalence the radiation energy is greater that the matter energy, so you talk about "radiation-dominated era". For a>a_{eq}, you have the matter-dominated era.
 
And this means because of Hubbles law, v=Hr, you can say that a \propto r? Since the expansion factor is proportional to the speed that objects move from each other in space?
 
Not exactly, since in cosmology, H(t) is defined as (da/dt)/a (sort of like your v/r).

Hubble's law is really just a local observation of the universe expanding.
 
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https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.

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