I suspect you're conflating two vastly different things? Light from distant 
galaxies - what's used to measure the Hubble constant - was emitted WAY 
after the hypothetical inflationary era. The Hubble expansion only refers 
to the increasing separation between galaxies/clusters of galaxies/similar 
observable objects/groups. It isn't possible to make deductions about 
inflation (except indirectly, e.g. from the observed homogeneity of matter 
in the universe) from observable objects, which formed a lot later. The 
earliest directly observable thing in the universe (at present) is the 
microwave background. It's possible neutrinos or gravitational waves will 
let us observe earlier eventa, but none of these appraoch the inflationary 
era, which predates the quark-gluon plasma that became nuclei etc.

On Tuesday, 15 July 2025 at 14:30:28 UTC+12 Alan Grayson wrote:

> Given the fact that light from very distant galaxies is hugely 
> red-shifted, and the general belief that light we're observing today from 
> those distant galaxies, was emitted when the universe was very young, one 
> would conclude that the rate of expansion at that time was huge. But Clark 
> disputes this conclusion. He claims the opposite; that the rate of 
> expansion in the very early universe was exceedingly SLOW. If that's the 
> case, can we conclude that the theory of Inflation must be false, insofar 
> as it alleges a huge initial expansion rate to account for the observed 
> uniformity of the current universe? Moreover, Hubble's law confirms that as 
> we go back in time, the universe was expanding faster than it is today, 
> again apparently confirming the Inflation theory of a very high initial 
> rate of expansion (ignoring recent findings the the rate of expansion is 
> iagain ncreasing). AG

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