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0 votes
1 answer
55 views

How to find critical density?

In Cosmology critical density is defined as the minimum density for a flat universe to keep expanding, by Friedmann Equation: ${\left({\frac {\dot {a}}{a}}\right)^{2}={\frac {8\pi G}{3}}\rho -{\frac {...
Polaris5744's user avatar
1 vote
1 answer
61 views

How to understand critical density?

In Cosmology, critical density is given by setting $\Lambda = 0$ and $k = 0$, in other words, a universe without dark energy and zero curvature. According to my understanding and Wikipedia, this ...
Polaris5744's user avatar
0 votes
1 answer
67 views

Solve Friedmann equation for non-zero curvature and non-zero cosmological constant

I tried to find an elegant way to solve (without approximating for low densities) $$\dot{R}^2=\frac{8 \pi G}{3 c^2} \rho R^2-k c^2+\frac{c^2 \Lambda}{3} R^2$$ for $k=\pm 1$ and $\Lambda \neq 0$ (one ...
Vincent ISOZ's user avatar
0 votes
0 answers
48 views

Big Bang as stretching space time?

I am still new to researching the big bang so please be patient. I am having trouble envisioning the expansion. As I understand under current theory it is not to be thought of as a singularity ...
Stargazer's user avatar
  • 101
5 votes
2 answers
415 views

Properties of anti-deSitter space

I have some questions about anti-deSitter space, (note: I am not a physicist) When describing deSitter space it is almost always mentioned that it has a positive cosmological constant and is therefore ...
Steven Vernau's user avatar
2 votes
1 answer
161 views

DeSitter cosmological horizon stability?

If the universe keeps expanding at an accelerated rate (given by the cosmological constant) then the universe would approach a DeSitter spacetime where there would be a cosmological horizon that would ...
vengaq's user avatar
  • 2,462
0 votes
0 answers
40 views

What exactly do astrophysicists mean when they say that the universe is expanding at an accelerated rate? [duplicate]

What exactly do astrophysicists mean when they say that the universe is expanding at an accelerated rate? Assuming that the universe is a sphere, do they mean that the radius of the universe increases ...
SPANDAN DASH's user avatar
1 vote
0 answers
33 views

The General form of the Friedmann equation written in another way

Using the general form of the Friedmann equation: $$H^2 =H_0^2(Ω_{m0}(1+z)^3+Ω_{r0}(1+z)^4+Ω_{k0}(1+z)^2+Ω_Λ)$$ and taking $a_0=1$, How can I derive that the Friedmann can be writing in the following ...
Voldewort's user avatar
2 votes
1 answer
94 views

About a hypothetical universe

Imagine a universe dominated by matter, but it is balanced with a cosmological constant $\Lambda=4\pi G\rho$ so the universe is static ($H=0$). However, what would happen if some of that matter turns ...
Carlos Gutierrez's user avatar
20 votes
1 answer
869 views

Did Einstein really invent the cosmological constant to make the universe static in his 1917 paper?

The popular account of Einstein inventing the cosmological constant goes like this: Einstein finds that the Einstein Field Equations predict an expanding universe Unable to accept this, Einstein adds ...
eigenchris's user avatar
0 votes
1 answer
117 views

Absence of matter stretches the fabric of space?

If matter attracts matter, because it curves the space, could it be that the absence of matter stretches the space, and that's why the universe expansion is accelerating? I mean that could be ...
Jose Renato's user avatar
0 votes
0 answers
35 views

What is the dark energy & dark matter? [duplicate]

Can anyone explain to me simply what is the dark energy or what is the dark matter. I have been trying to understand it deeply. but I somehow failed.
Carlos Werbock's user avatar
1 vote
1 answer
463 views

Einstein's Static Solution with $\Lambda =0$ to The Friedmann Equations?

Is it possible to show the universe is static (i.e., $a=a_*=\rm{const}$) without assuming $a=\rm{const}$ to begin with, and using a mix of $w=0$ and $w=-1$? Let $\Lambda=0$ in the Friedmann equations, ...
CCGBLADE's user avatar
2 votes
1 answer
897 views

Static solution to the Friedmann equation [duplicate]

I want to find the static solution for the Friedmann equation: $$ \bigg(\frac{\dot{a}}{a}\bigg)^2=H_0^2\bigg(\Omega_m\bigg(\frac{a_0}{a}\bigg)^3+\Omega_v+\Omega_k\bigg(\frac{a_0}{a}\bigg)^2\bigg) $$ ...
Yep's user avatar
  • 135
1 vote
0 answers
51 views

Can a cosmological constant model inhomogeneities?

Consider the following zero-order approximation to the universe: Spacetime is perfectly homogeneous, and The cosmological constant is exactly zero. This doesn't quite work. Neither assumption is ...
AccidentalFourierTransform's user avatar

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