heusdens
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Originally posted by marcus
Hi heusdens, it is a nice try but doesn't work
I am replying to what you said in previous post:
"But what if our length unit would be choosen in such a way, that it does express some fundamental property of nature. As I suggest, the expansion of space itself, ..."
You have been given a bad misconception from popular accounts and the careless way astronomers talk
The rate that space is expanding is different in different places.
It is uneven.
Uniform expansion is not at all a "fundamental property" of space built into its nature.
When they talk about the expansion rate they mean a kind of temporary average.
The average is only strictly correct for the present moment (t=0) which is why they write the zero subscript on H0.
And it is only a rough estimate gotten by averaging the expansion in various places and directions from us, which rigorously speaking are all different.
The main equations of cosmology---Friedmann's two equations---are boiled down from Einsteins by ASSUMING that the distribution of energy in space is isotropic and homogeneous (same everywhere and in all directions) which it obviously is NOT.
However the Friedmann equations are simple and terribly useful and the work soooooo well! Even though predicated on obviously false assumptions. These equations contain the definition of the Hubble constant----the idealized expansion rate.
We have enough to worry about with the fundamental constants we already have. Please do not suggest that the expansion-rate of space is also a "fundamental constant"!
Compared with other things it is highly changeable.
One should really call it "Hubble parameter" (as some people are starting to do) and not call it Hubble "constant."
But cheers anyway, I sympathize with your interest in scales of measurement and foundations-issues
That's a good point!
And there is one other thing about the Hubble correlation parameter.
We can only observe this correlation in a very tiny spatial and temporal extent (namely: the temporal and spatial extend in which we know about, or since we do scientific cosmologic observations).
How do we know then that there is a distance - velocity ("virtual" recession speed) relation, it could as well be a time - velocity / virt. reces. speed relation.