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1 vote
3 answers
79 views

Can a light signal from Earth reach a galaxy outside the Hubble Horizon?

Is this video on the FLRW metric (timestamp 19:00 minutes) mistaken in its claim that a light signal from Earth cannot catch up with a galaxy outside the Hubble horizon, due to the horizon receding at ...
KDP's user avatar
  • 5,551
0 votes
1 answer
40 views

Friedmann Equation and a contracting universe

Consider a universe with a nonzero curvature and matter. One can write the Friedmann Equation in this universe as such: $$\frac{H(t)^2}{H_0^2} = \frac{\Omega_0}{a^3}+\frac{1-\Omega_0}{a^2}$$ Where $H(...
Polaris5744's user avatar
-4 votes
0 answers
45 views

Simple question about finite Universe [duplicate]

If, by Big Bang, Universe was created from initial singularity, with finite "speed" of expansion of matter, shouldnt it be finite as well?
Влад Дедков's user avatar
9 votes
4 answers
631 views

Understanding expansion of the Universe as things flying apart

Say that we have a Universe uniformly filled just with matter (let's not bring dark energy into this). And say that we fill it with very light particles (so that the gravitational interaction between ...
Negredol Nekaj's user avatar
0 votes
2 answers
110 views

Is it true that $\dot{H}(t)\sim H(t)$, and if so, why?

In the context of working with the FRW metric in Cosmology, I'm trying to reproduce the results of a paper where an expansion of the metric in terms of perturbations is performed. The author gives a ...
Wild Feather's user avatar
1 vote
2 answers
525 views

Please help me with this paradox [closed]

Physicists believe that some galaxies are moving away from us at faster than the speed of light. A galaxy that is moving away from us at faster than the speed of light would be moving backwards in ...
Cecilia's user avatar
  • 35
2 votes
1 answer
280 views

Negative Horizon distance

Consider a flat universe, here, proper distance can be given by R-W Metric: $$d_p (t_0) = c\int_{t_e}^{t_0}\frac{dt}{a(t)},$$ $t_e$ is the time when a photon is emitted from a distant galaxy, $t_0$ is ...
Polaris5744's user avatar
1 vote
1 answer
76 views

Why is the First Law of Thermodynamic related to Fluid Equation?

In Cosmology, there is a equation called Fluid Equation: $$\dot{{\varepsilon}}+3\frac{\dot{a}}{a}(\varepsilon+P)=0.$$ It is derived by taking time derivative of the First Law of Thermodynamic: $\dot{E}...
Polaris5744's user avatar
6 votes
4 answers
2k views

Accelerating Expansion of Universe - Why Not Caused by Radiation?

As I understand it, dark matter and dark energy are used as an 'explanation' for how universe expansion is accelerating; because without it gravity would be expected to cause a long term shrinking. ...
Claud's user avatar
  • 181
0 votes
4 answers
132 views

Why does Hubble's Law indicate motion?

I have been trying to understand and find some justification about why Hubble's Law needs to implicate any sort of relative motion between galaxies. I can understand why and how one would explain the ...
Spongie's user avatar
1 vote
3 answers
83 views

Does the fact that we are able to see CMBR implies that universe expanded faster than light?

Supposedly, the universe underwent rapid expansion immediately after the big bang, surpassing the speed of light. If we can detect remnants from that era, does this suggest they moved faster than ...
Mr. Spock's user avatar
0 votes
2 answers
92 views

Could Space and Time Be Decoupled Pre- Big Bang?

The traditional view holds that both space and time emerged together from the Big Bang. However, I'm curious about the possibility that time could be eternal, with no beginning, while space began to ...
VVM's user avatar
  • 487
4 votes
3 answers
197 views

Change of variables from FRW metric to Newtonian gauge

My question arises from a physics paper, where they state that if we take the FRW metric as follows, where $t_c$ and $\vec{x}$ are the FRW comoving coordinates: $$ds^2=-dt_c^2+a^2(t_c)d\vec{x}_c^2$$ ...
Wild Feather's user avatar
0 votes
1 answer
41 views

Friedmann fluid equation in the non-relativistic case

The Friedmann fluid equation I am referring to is: $$ a\frac{d\rho}{da} = -3(\rho+P) .$$ In the non-relativistic (low temperature) case for an ideal gas universe (representing matter), I know that the ...
Andreas Christophilopoulos's user avatar
1 vote
0 answers
45 views

How to find the relation between flow-parameters and number of e-folds?

In models of single field inflation the Friedmann equation reads $$ H(t)^2 = \frac{8\pi G}{3} \big(V(\varphi) + \frac{\dot{\varphi}^2}{2}\big) \tag{1}\label{eq1}. $$ In the slow-roll approximation one ...
ouroboros's user avatar
  • 126

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