Critical density formula hides fundamental relationship?

In summary, the current density of the universe is close to the critical density. This implies that the universe is flat and linearly expanding.
  • #1
johne1618
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Observations show that the current density of the Universe is close to the critical density:

rho = 3 H_0^2 / 8 Pi G

Assuming a spherical observable Universe of constant density, together with the relation c = H_0 * R, one can rearrange the above equation to give the relation:

G * M / R = c^2 / 2

where M is the mass and R is the radius of the observable universe at the current cosmological time.

Perhaps this is a fundamental relationship that holds at all times. It seems to embody Mach's principle in that it says that half the mass/energy of any particle comes from the mutual gravitational potential energy between the particle and the rest of the observable Universe. (To see this multiply both sides by the particle mass m). In fact this relationship seems to provide a natural definition of the "observable" universe as the "gravitationally interacting" Universe.

If you plug the above relationship into the Friedmann equations one gets a linearly expanding model that behaves exactly like the massless Milne model!
 
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  • #2
johne1618 said:
If you plug the above relationship into the Friedmann equations one gets a linearly expanding model that behaves exactly like the massless Milne model!
If you do it properly, everything will cancel, because the equation you wrote down is the equivalent of the Friedmann equations.
 
  • #3
The equation defines a model of the Universe that is spatially flat and linearly expanding that obeys the Friedmann equations.

The first Friedmann equation says:

[(a' / a)^2 - 8/3 G Pi rho] a^2 = -kc^2

where a is the scale of the Universe, rho the density and k is the spatial curvature.

If I use the relationship G M / R = c^2 / 2 for a spherical observable universe of Mass M and radius R then I can get a formula for the density rho as

rho = M / V = (c^2 * R / 2 G) * 1 / (4/3 Pi R^3)

rho = 3 c^2 / 8 Pi G R^2

Now for the Hubble constant we have the formula:

c = H R

Therefore the term 8 /3 G Pi rho is actually H^2.

We also know the term (a' / a)^2 = H^2 by the definition of the Hubble constant.

Thus we find that this solution implies

-k c^2 / a^2 = H^2 - H^2 = 0

therefore the spatial curvature is zero. Notice we haven't set it to zero beforehand it came out naturally from the model.
 
  • #4
johne1618 said:
Now for the Hubble constant we have the formula:
c = H R
This is a linear approximation valid only below the curvature scale; so you are implicitly assuming a flat universe by using the Hubble relation.
 
  • #5
johne1618 said:
If I use the relationship G M / R = c^2 / 2 for a spherical observable universe of Mass M and radius R
And this is a spherical mass distribution embedded in flat space...
 

FAQ: Critical density formula hides fundamental relationship?

What is the critical density formula?

The critical density formula is a mathematical equation used in cosmology to determine the average density of matter in the universe. It is denoted as ρc and is equal to 3H^2/8πG, where H is the Hubble constant and G is the gravitational constant.

What is the significance of the critical density formula?

The critical density formula is significant because it allows us to understand the overall structure and evolution of the universe. It tells us whether the universe is expanding or contracting, and whether it contains enough matter to eventually stop its expansion and start contracting.

How does the critical density formula hide a fundamental relationship?

The critical density formula hides a fundamental relationship between the average density of the universe and the rate of its expansion. This relationship is known as the Friedmann equations, which describe the evolution of the universe and its expansion based on the amount and type of matter present.

Why is the critical density formula important in determining the fate of the universe?

The critical density formula is important because it helps us determine the fate of the universe. If the average density of the universe is equal to the critical density, it will eventually stop expanding and start contracting. If the average density is less than the critical density, the universe will continue to expand forever. And if it is greater than the critical density, the universe will eventually collapse in a "Big Crunch."

Can the critical density formula be used to accurately predict the future of the universe?

While the critical density formula can give us an idea of the overall structure and fate of the universe, it cannot accurately predict the exact future. This is because the formula is based on certain assumptions and does not take into account other factors such as dark matter and dark energy, which also affect the evolution of the universe.

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