Zitat:
Zitat von Timm
Was ist von diesem paper zu halten:
https://arxiv.org/pdf/2207.09736.pdf
In this paper, by using the well known weak field, low velocity gravitomagnetic formulation of GR, the expected rotation curves in GR are rigorously obtained for purely baryonic disk models with realistic density profiles, and compared with the predictions of newtonian gravity for the same disks in absence of Dark Matter. As expected, the resulting rotation curves are indistinguishable, with GR corrections at all radii of the order of v 2/c2 ? 10?6 |
Genau was ich schon immer sage. Die ART bringt Korrekturen in der Größenordnung 10e-6, weil wir es hier mit ganz, gamz schwachen Feldern zu tun haben.