Strong constraints on weak gravity from Gaia DR3 wide binaries

Testing Milgromian dynamics (MOND) with widely separated binary stars in the Solar neighbourhood, which due to their low accelerations should have their mutual gravity and thus their orbital velocity enhanced by 20% in MOND compared to Newtonian expectations. A priori protocol used as much as possible to mitigate possible bias in conducting such a critical test:

Slides are available here:

The recently accepted paper on this result is available here:

[synx]

so he shows how MOND actually works and is correct for the whole talk and then in the end he concludes that it doesn't work... not very helpfull.