Ab initio Calculation of Galactic Rotation Curves in vacuo

Details Ab initio Calculation of Galactic Rotation Curves in vacuo Ab initio Calculation of Galactic Rotation Curves in vacuo

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..apr.s1006m&link_type=abstract

American Physical Society, APS April Meeting, April 14-17, 2007, abstract #S1.006

Physics

Optics

Scientific paper

Galactic rotation curves appear to become asymptotically flat far from the core, a feature that can be explained with an optical model of gravitational forces. With the core as a central lens, gravity from one side of the galaxy can be focused by the core onto the oposite side, thereby increasing radial forces, above those expected from a central Newtonian model. Using basic optics, the asymptotic rotational features of galaxies are easily calculated. The need for dark matter in galaxies is obviated.

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