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0 votes
1 answer
42 views

$Ω = ρ/ρ[c]$, so although near to 1, for an accelerating expansion $Ω$ must be below 1. What's its value?

$Ω$ is taken to have different components - ordinary matter, dark matter, dark energy. But because it is expressed in relation to the critical density for attractive gravity, it seems that omega is ...
user141183's user avatar
1 vote
1 answer
104 views

Given current densities of dark energy, dark matter and normal matter in universe currently, calculate ratio of density of dark matter at CMB to now? [closed]

I stumbled upon this question while preparing for the astronomy Olympiad. It is question #17 in this pdf. Given that dark energy is vacuum energy, and that the densities of dark energy, dark matter ...
YUBRAJ BHANDARI's user avatar
2 votes
1 answer
214 views

Formula for the bias of galaxies

From the article "Large-Scale Galaxy Bias", I try to deduce the equation that my teacher told me which links 2 quantities: the global number density of galaxies the local number density of galaxies ...
user avatar
6 votes
2 answers
160 views

How do we know that dark matter energy density scales as $\rho\propto a^{-3}$?

How do we know that dark matter energy density scales as $\rho\propto a^{-3}$?
SRS's user avatar
  • 26.8k
3 votes
1 answer
2k views

Average Density of the Universe over Time

For reference: Referring to a question I posted in Feb. 2015: Could Hyper-Massive Black Holes be due to Dark Matter in the Early Universe? User10851 answered, and I replied. He then replied to my ...
SigSeg's user avatar
  • 189