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- W3157401662 abstract "We use an up to date compilation of Tully-Fisher data to search for transitions in the evolution of the Tully-Fisher relation. Using an up to date data compilation, we find hints at $approx 3sigma$ level for a transition at critical distances $D_c simeq 9 Mpc$ and $D_c simeq 17 Mpc$. We split the full sample in two subsamples according to the measured galaxy distance with respect to a splitting distance $D_c$ and identify the likelihood of the best fit slope and intercept of one sample with respect to the best fit corresponding values of the other sample. For $D_c simeq 9 Mpc$ and $D_c simeq 17 Mpc$ we find a tension between the two subsamples at a level of $Delta chi^2 > 17; (3.5sigma)$. Using a Monte-Carlo simulation we demonstrate that this result is robust with respect to random statistical and systematic variations of the galactic distances. If the tension is interpreted as due to a gravitational strength transition, it would imply a shift of the effective gravitational constant to lower values for distances larger than $D_c$ by $frac{Delta G}{G}simeq -0.1$. Such a shift is of the anticipated sign and magnitude but at somewhat lower distance (redshift) than the gravitational transition recently proposed to address the Hubble and growth tensions ($frac{Delta G}{G}simeq -0.1$ at transition redshift $z_tlesssim 0.01$ ($D_clesssim 40 Mpc$))." @default.
- W3157401662 created "2021-05-10" @default.
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- W3157401662 date "2021-04-29" @default.
- W3157401662 modified "2023-09-27" @default.
- W3157401662 title "Hints for a gravitational constant transition in Tully-Fisher data" @default.
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