Galaxy Dynamics Predictions in the Nonsymmetric Gravitational Theory
J. W. Moffat
Abstract
In the weak field approximation, the nonsymmetric gravitational theory has, in addition to the Newtonian gravitational potential, a Yukawa potential produced by the exchange of a spin 1+ boson between fermions. If the range r0 is of order 30 kpc, then the potential due to the interaction of known neutrinos in the halos of galaxies can explain the flat rotation curves of galaxies. The results are based on a physical linear approximation to the NGT field equations and they are consistent with equivalence principle observations, other solar system gravitational experiments and the binary pulsar data.
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