Show me the math. All these words mean nothing without a model to test.
Again, worthless words without a working model. Link a model or an equation so we can play with it.
As an aside, I'm going to go on a tangent first by saying, I will be starting another thread because you said that we are not going to Mars because of mass extinction if we stay on Earth. Be sure to look for it. I'm not sure where you've been the last few decades.
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Cosmological relativity is an extension of the principles of Einstein's Special and General Relativity to cosmological scales. However, its starting point is the expansion of the Universe and not the propagation of light.
Cosmic Time
Cosmic time is the time that the universe would need to expand from a zero size point for a given red shift. In the Big Bang cosmology it would be the time since the
Big Bang. In any cosmology that starts with the universe as larger than a point, the universe would actually be younger than
cosmic time.
- t = Cosmic time.
- z= Red Shift.
- τ = Observed Cosmic time = 13.56 Gyr.
According to Cosmological Relativity τ is constant for all space and time such that at any place in the Universe and at any time in its history an observer would measure the same Current cosmic time. Also like Einsteinian Relativity the laws of nature are the same for all space and time. The result is that there is no absolute cosmic time; instead it is relative to the time and place of the observer just like velocity in
Special relativity. Also like velocity in
Special relativity cosmic time does not simply add from one observer to another. Instead cosmic time is added by the following formula:
- t = Cosmic time.
- τ = Observed Cosmic time = 13.56 Gyr.
The key to Cosmological Relativity is that there is no absolute cosmic time, although any observer at any point in space and at any time will see τ = 13.56 Gyr.
5D cosmology
Cosmological relativity’s line element for an expanding Universe in negligible gravity is:
ds2 = τ2
dν2 - (
dx2 +
dy2 +
dz2 )
- τ = H0-1 = Observed Cosmic time = 13.56 Gyr.
- ν = Is the space velocity at a given point in space.
- x,y,z = Normal 3d spatial dimensions.
This is similar to the
Special relativity line element.
ds2 = c2
dt2 - (
dx2 +
dy2 +
dz2 )
- t = time.
- c = the speed of light.
- x,y,z = Normal 3d spatial dimensions.
When time is added to Cosmological relativity’s line element we get:
ds2 = τ2
dν2 - (
dx2 +
dy2 +
dz2 ) + c2
dt2
- τ = H0-1 = Observed Cosmic time = 13.56 Gyr.
- ν = Is the space velocity at a given point in space.
- t = time.
- c = the speed of light.
- x,y,z = Normal 3d spatial dimensions.
The result is a theory of 5 dimensions.
- 1 of time.
- 1 of spatial expansion velocity.
- 3 normal spatial dimensions.
Special Relativity
Cosmological Special Relativity has much in common with
Einstein’s Special relativity. Both theories deal with the special case of no gravity forming the basis for the more general concept. The main difference is that cosmic time (t) replaces velocity (v) as the critical quantity and observed cosmic time (τ= 13.56 Gyr) replaces the velocity of light (c) as the constant. Both theories have essentially the same formulae, but Cosmological Special Relativity substitutes ”t” for “v” and “τ” for “c”.
In Cosmological Special Relativity τ = H0-1 = 13.56 Gyr, where H0 = Hubble’s constant.
Thus both theories have similar transformations between reference frames.
- Cosmological Special Relativity
Thus both theories have similar formulae for relative mass. (m)
- Cosmological Special Relativity
Similar formulae for relative length. (L)
- Cosmological Special Relativity.
It is in the area of time (t) and velocity (v) that the two theories are the most different, since they basically switch places. However, in Cosmological Special Relativity, the velocity referred to is the expansion of the universe and not the independent motion of the object.
- Cosmological Special Relativity.
In Cosmological Special Relativity we get an added relationship for the acceleration (a) of the expansion of the universe.
Cosmological Special Relativity also has relativistic formulae for the universes’ density (ρ) and temperature (T).
Even though both the universe's density (ρ) and its temperature (T) are shown to be larger in the past, it seems likely that these are purely relativistic affects and that at those times the measured values would be what they are today.
Cosmological Special Relativity and
Special relativity are not exclusive but work together, each being most significant under the right circumstances.
Special relativity as v approaches c and Cosmological Special Relativity as t approaches τ.
General Relativity
Cosmological General Relativity, like
Einstein’s General relativity, deals with the general case where gravity is present.
4D
In its 4D form of space-velocity, Cosmological General Relativity gives only the state of the universe in an instant of time.
While in Cosmological Special Relativity τ = H0-1, when gravity is considered as it is in Cosmological General Relativity, τ = h-1, and its relationship H0 becomes:
- Ωm =ρm/ρc = Cosmological General Relativity’s ratio of the mass density of the universe and the mass density that would result in a constant expansion rate.
- ρc = 3h2/8πG = 3/8πGτ2 = Cosmological General Relativity’s mass density at which a constant expansion rate occurs.
- ρm = measured mass density of the universe.
- z = ν /c = redshift.
- h = τ-1 = 72.17 km / s Mpc
- τ = Observed Cosmic time = 13.58 Gyr.
- G = Gravitational Constant
According to Cosmological General Relativity, the presence of gravity resulting from matter and energy reduces the vacuum pressure that tends to accelerate the expansion of the universe. This vacuum pressure (p) is denoted by:
As a result, the value of Ωm affects the expansion of the universe:
Ωm > 1
- This results in a decelerating expansion.
Ωm = 1
- This results in a constant expansion.
Ωm < 1
- This results in an accelerating expansion.
- Ωm = 0.245
When this is applied to the unbounded universe of the
Big bang, the result is that for the first 5.08 Gyr after the
Big bang there would be a decelerating expansion. At this point the expansion becomes constant for a brief time and then starts to accelerate as it is today.
Next we have ΩT which denotes the curvature of space on cosmic scales. The difference between ΩT and Ωm is ΩΛ. Such that:
ΩT = Ωm + ΩΛ
Now ΩΛ = (H0 / h)2 = 0.764
The result is: ΩT = Ωm + ΩΛ = 0.245 + 0.764 = 1.009 ≈ 1
This shows that the universe is flat ( Euclidean ) on a large scale
5D
When the time dimension is added to Cosmological General Relativity, the result is a 5D theory that reproduces all of the results of General Relativity with additional effects that solve a number of problems in cosmology. It results in a 5D space – time – velocity manifold that is an extension of General Relativity for cosmology.
Cosmological relativity - CreationWiki, the encyclopedia of creation science
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Cosmological Relativity: A New Theory of Cosmology
Cosmological Relativity: A New Theory ofCosmology1
Cosmological special relativity
Cosmological special relativity
Aspects of Cosmological Relativity
Aspects of Cosmological Relativity
Value of the Cosmological Constant in the Cosmological Relativity Theory
Value of the Cosmological Constant in the Cosmological Relativity Theory
On the Anomalous Acceleration of Pioneer Spacecrafts
On the Anomalous Acceleration of Pioneer Spacecrafts
Five-dimensional cosmological theory of unified space, time and velocity
Five-dimensional cosmological theory of unified space, time and velocity - ScienceDirect