Strong constraints on the gravitational law from Gaia DR3 wide binaries

We Views Milgromian d Indranil Banik u Charalambos Pittordis s Will Sutherland ra Benoit Famaey k Rodrigo Ibata , Steffen Mieske lo Hongsheng Zhao ho Strong ceed the Newtonian prediction by |$\approx Gaia DR3 t asymptotically Monthly Notices of the Royal Astronomical Society el 2023 fec stad3393 < https://doi.org/10.1093/mnras/stad3393 - - Share Icon Share Abstract ss="summa Milgromian hLightText__NxlGi">Newtonian 2 − t 30 xt__NxlGi">Pittordi WB and Sutherland Newtonian ightText__NxlGi |$\approx 20\%$| pan class="summaryFeed_highLightText__NxlGi">Ne Galactic /span> \rm Gaia DR3 ghtText__ 8611 i">Monte Car 250 /span> Sun class="summaryFeed_highLightText__NxlGi">Markov Chain EFE _NxlGi">19σ Newtonian WB eed_highLightText__NxlGi">Mil Newtonian span> Milgromian ass="summaryFeed_highLightText__NxlGi">Newton 0 an < Newtonian s="summaryFeed_highLightText__NxlGi">1