gravity is kicking and alive: the cases of Orion and NGC 3198
arXiv:1405.6314 · doi:10.1142/S021827181442005X
Abstract
We analyzed the Rotation Curves of two crucial objects, the Dwarf galaxy Orion and the low luminosity Spiral NGC 3198, in the framework of gravity. We surprisingly found that the no DM power-law f(R) case fits them well, performing much better than CDM Dark Matter halo models. The level of this unexpected success can be a boost for gravity.
arXiv commentThis essay received an honorable mention in the Gravity Research Foundation 2014 Essay Contest. 6 pg, 1 fig
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- Galactic rotation dynamics in a new gravity model
- Light deflection angle through velocity profile of galaxies in model
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- Palatini gravity tests in the weak field limit: Solar System, seismology and galaxies
- Static Spherically Symmetric solutions in a subclass of Horndeski theories of gravity
- Velocity dispersion of dark matter deficient ultra-diffuse galaxies: A case for modified gravity