A Radically Conservative Solution for Cosmology’s Biggest Mystery
quantamagazine.org
quantamagazine.org
The tension has been there for a long time, but its only something like two years ago that the statistical errors got small enough you had to somewhat seriously consider there could be some important reason for the disagreement.
Gaia gives better Cepheid distances, decreasing the total uncertainty somewhat. But the big story is the calibration of the intrinsics supernova brightness (and its variation), so while better Cepheids help, its mostly by further closing a already unlikely avenue of explanation.
The big crime of the article is portraying the field as thinking the tension is due to new physics, when in fact the difference between the CMB and SN determinations has been known for something like 20 years and for all that time been mostly viewed as something experimentalists get sorted. For a long time the values agreed within their stated uncertainties, and its only rather recently that they have pushed their statistical errors down enough that the difference can be said to be real. So its a while yet until the difference is truly trusted as something to be explained by new physics rather than some calibration error.
I am not sure how to parse this quote, and seem unlikely that appropriate statistical models weren't available
It's also not obvious that there should be a statistical framework because combinations is usually something done carefully by people familiar with both experiments, so essentially it's on a case by case basis and not wholesale across the field.
General Relativity affords uniform expansion through the cosmological constant. Non-uniform expansion means new fields, so either dark matter or modified gravity.
The main problem with eternal inflation is it gets us attempting to make statements about regions outside what we can observe directly.