Galactic mass distribution without dark matter or modified Newtonian mechanics

Details Galactic mass distribution without dark matter or modified Newtonian mechanics Galactic mass distribution without dark matter or modified Newtonian mechanics

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..apry11008n&link_type=abstract

American Physical Society, APS April Meeting, April 14-17, 2007, abstract #Y11.008

Physics

Scientific paper

Given the dimensions (including thickness) of a galaxy, and its rotation profile, a method is arranged to find the mass and density distribution in the defined envelope that will cause that rotation profile with near-exact speed matches. Newton's law is unchanged. Surface-light intensity and dark matter are not needed. Results are presented in dimensionless plots allowing easy comparisons of galaxies.

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