Perfect cosmological principle in co-moving co-ordinates

In summary, the Steady State model of the Universe was proposed in 1948 by Bondi and Gold. It assumes that the Universe is the same at all times, and that the Hubble parameter is a constant. If the Universe is the same at all times, then it has a finite lifespan. However, this model has been discredited due to evidence of a Big Bang Universe with a finite age. A variant of the Milne model called Milne-Dirac is possible if antimatter repels matter, but the odds of this are not favorable.
  • #1
johne1618
371
0
To quote cosmologist Ned Wright:

The Steady State model of the Universe was proposed in 1948 by Bondi and Gold and by Hoyle.

Bondi and Gold adopted the "Perfect Cosmological Principle", and added the assumption that the Universe was the same at all times to homogeneity (the same in all places) and isotropy (the same in all directions).

If the Universe is the same at all times, it is argued that the value of the Hubble parameter must be a constant [itex]H_0[/itex], so

[itex] H = \frac{\dot{a}}{a} = H_0[/itex]

leading to an exponential cosmology

[itex]a(t) = e^{H_0 (t - t_0)}[/itex]

where [itex]t_0[/itex] is the present age of the Universe.

This model is an expanding model that does not change its appearance over a time interval from [itex]-\infty[/itex] to [itex]+\infty[/itex].

However this model has been discredited as there is good evidence of a Big Bang Universe with a finite age.

But perhaps one could save the Perfect Cosmological Principle by saying the Universe should look the same at all times in co-moving cordinates.

Now we have

[itex] H = \frac{c}{R_H} [/itex]

where [itex]R_H[/itex] is the Hubble radius.

Therefore if the Universe is to look the same at all times in co-moving co-ordinates then [itex]R_H[/itex] must be co-moving and so

[itex]R_H = a(t) R_0[/itex]

where [itex]R_0[/itex] is constant.

Therefore we have

[itex]\frac{\dot{a}}{a} = \frac{c}{a R_0}[/itex]

As [itex]H_0 = c/R_0[/itex] we have

[itex]\frac{\dot{a}}{a} = \frac{H_0}{a}[/itex]

with solution

[itex] a(t) = H_0 t[/itex]

This model is static in co-moving co-ordinates with a finite lifetime.
 
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  • #2
Congratulations you've used reinvented the Milne model!

You can search the forums for lots of detail on the problems with Milne. The short answer is 1) it requires gravity to work differently than we think it does 2) it causes the early universe to expand rather slowly which causes problems with big bang nucleosynthesis and CMB 3) it doesn't fit with the most recent supernova measurements.

There is a variant of the Milne model called Milne-Dirac in which antimatter repels matter. In one recent thread, I was sort of defending it as "probably wrong, but not totally crazy."
 
  • #3
Yes, twofish occasionally argues the less probable side of issues [he is old and enjoys stirring the pot now and then]. The odds favoring anti gravity from anti matter are not favorable. Gravity is almost surely mediated by an integer boson, and integer bosons appear to be indifferent to charge.
 
  • #4
twofish-quant said:
Congratulations you've used reinvented the Milne model!

The co-moving perfect cosmological principle is also consistent with the Coasting Cosmology model with equation of state:

[itex] p = -\frac{\rho c^2}{3} [/itex]

In any flat model without cosmological constant we have

[itex] \rho \propto \frac{1}{R_H^2} [/itex]

In the CC model [itex]R_H[/itex] is constant in comoving co-ordinates and therefore the energy density [itex]\rho[/itex] is constant in co-moving co-ordinates.

This makes sense to me because if you factor out the expansion of space then you would expect the energy density to remain constant as energy is conserved locally.
 
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  • #5
This has actually been discussed quite a bit recently. Here's a paper you might find interesting: http://arxiv.org/abs/1109.5189

(and no, it's not correct :)
 

1. What is the Perfect Cosmological Principle?

The Perfect Cosmological Principle states that the universe looks the same from every point in space and in every direction. This means that the laws of physics and the distribution of matter are the same throughout the universe.

2. What are co-moving coordinates?

Co-moving coordinates are a type of coordinate system used in cosmology that take into account the expansion of the universe. They are defined by the comoving distance, which is the distance between two points that is constant throughout the history of the universe.

3. How does the Perfect Cosmological Principle apply to co-moving coordinates?

In co-moving coordinates, the Perfect Cosmological Principle means that the universe looks the same from every point in space and at every point in time. This is because the comoving distance between any two points remains constant, regardless of the expansion of the universe.

4. What is the significance of the Perfect Cosmological Principle in cosmology?

The Perfect Cosmological Principle is a fundamental assumption in the study of the large-scale structure and evolution of the universe. It allows us to make predictions and understand the behavior of the universe on a grand scale.

5. What are some evidence for the validity of the Perfect Cosmological Principle?

Some evidence for the Perfect Cosmological Principle includes the observation of the cosmic microwave background radiation, which is nearly uniform in all directions, and the distribution of galaxies in the universe, which is consistent with the idea of a homogeneous and isotropic universe.

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