Conformally-rescaled Schwarzschild metrics do not predict flat galaxy rotation curves
Abstract For conformally invariant gravity theories defined on Riemannian spacetime and having the Schwarzschild–de-Sitter (SdS) metric as a solution in the Einstein gauge, we consider whether one may conformally rescale this solution to obtain flat rotation curves, such as those observed in galaxie...
| المؤلفون الرئيسيون: | , |
|---|---|
| التنسيق: | مقال |
| اللغة: | English |
| منشور في: |
SpringerOpen
2022-07-01
|
| سلاسل: | European Physical Journal C: Particles and Fields |
| الوصول للمادة أونلاين: | https://doi.org/10.1140/epjc/s10052-022-10531-6 |