Authors: Yuri Heymann
The dark matter problem in the context of spiral galaxies refers to the discrepancy between the galactic mass estimated from luminosity measurements of galaxies with a given mass-to-luminosity ratio and the galactic mass measured from the rotational speed of stars using the Newton’s law. Newton’s law fails when applied to a star in a spiral galaxy. The problem stems from the fact that Newton’s law is applicable to masses represented as points by their barycenter. As spiral galaxies have shapes similar to a disk, we shall correct Newton’s law accordingly. We found that the Newton’s force exerted by the interior mass of a disk on an adjacent mass shall be multiplied by the coefficient ηdisk estimated to be 7.44±0.83 at a 99% confidence level. The corrective coefficient for the gravitational force exerted by a homogeneous sphere at it’s surface is 1.00±0.01 at a 99% confidence level, meaning that Newton’s law is not modified for a spherical geometry. This result was proven a long time ago by Newton in the shell theorem.
Comments: 8 Pages. Accepted for publication in Progress in Physics
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[v1] 2016-07-19 23:11:49
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