In the article version I looked at (see below) there were many uses of the word
tension. I was unable to find what this word means in these contexts. I would much appreciate someone explaining what the usage of
tension in the article means.
https://www.nature.com/articles/s41...10MNWY=&tracking_referrer=www.livescience.com
The following are a few examples.
Before evaluating the
tensions of the PL18 results with independent cosmological observables, we first check whether the PL18 power spectra can provide an unbiased and reliable estimate of the curvature of the Universe.
When log 10 I I is positive, then two datasets are in agreement, whereas they are in
tension if this parameter is negative.
A second
tension is present between PL18 power spectra and the constraints on the lensing potential derived from the four-point function of Planck CMB maps39 (hereafter, called CMB lensing).
This
tension is also present in the PL18 release 2 , and the inclusion of the A lens parameter removes this difference.
Even assuming these data points to be independent, the increase in χ2 when curvature is varied suggests there is
tension at the 95% CL, while there is no significant
tension in the case of flatness.
Fig. 4 |
Tension with BAO.
Fig. 5 |
Tension with CMB lensing.
Fig. 6 |
Tension with Cosmic shear measurements.