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The Hubble parameter is defined by:
H(t) = a'(t) / a(t)
where a is the scale factor which is a function of cosmological time t.
This definition is equivalent to the Hubble relation:
v(t) = H(t) r(t)
where v(t) and r(t) are the proper velocity and distance of an object at cosmological time t.
I assume that this relationship is exact provided that we acknowledge that the Hubble parameter H(t) is constant only in space and *not* in time. It can be interpreted as simply asserting that space is expanding uniformly at a rate H(t).
Now let us assert that a universal speed limit exists, namely the velocity of light c. We know this is true observationally as the redshift diverges as v -> c.
This assumption allows us to define the Hubble radius R(t) by
c = H(t) R(t).
Then the Hubble radius, R_0, at the present time t_0 is given by:
c = H_0 R_0
where H_0 is the present Hubble parameter value.
As we have:
R(t) = R_0 a(t)
R(t) = (c / H_0) * a(t)
Therefore
a'(t) / a(t) = c / R(t)
a'(t)/ a(t) = H_0 / a(t)
So that finally
a(t) = H_0 * t
or equivalently
R(t) = c * t
Thus we seem to have derived a scale factor with a linear time dependence using only two facts:
1. Space is expanding uniformly.
2. A cosmological speed limit, namely c, exists.
Is this correct?
I expect I'm also assuming that space is flat.
This very simple scale factor time dependence, the so-called coasting cosmology, is actually close to what is observed.
H(t) = a'(t) / a(t)
where a is the scale factor which is a function of cosmological time t.
This definition is equivalent to the Hubble relation:
v(t) = H(t) r(t)
where v(t) and r(t) are the proper velocity and distance of an object at cosmological time t.
I assume that this relationship is exact provided that we acknowledge that the Hubble parameter H(t) is constant only in space and *not* in time. It can be interpreted as simply asserting that space is expanding uniformly at a rate H(t).
Now let us assert that a universal speed limit exists, namely the velocity of light c. We know this is true observationally as the redshift diverges as v -> c.
This assumption allows us to define the Hubble radius R(t) by
c = H(t) R(t).
Then the Hubble radius, R_0, at the present time t_0 is given by:
c = H_0 R_0
where H_0 is the present Hubble parameter value.
As we have:
R(t) = R_0 a(t)
R(t) = (c / H_0) * a(t)
Therefore
a'(t) / a(t) = c / R(t)
a'(t)/ a(t) = H_0 / a(t)
So that finally
a(t) = H_0 * t
or equivalently
R(t) = c * t
Thus we seem to have derived a scale factor with a linear time dependence using only two facts:
1. Space is expanding uniformly.
2. A cosmological speed limit, namely c, exists.
Is this correct?
I expect I'm also assuming that space is flat.
This very simple scale factor time dependence, the so-called coasting cosmology, is actually close to what is observed.
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