An attempt to do without dark matter
天体物理学
2015-06-24 v1
摘要
The discrepancy between dynamical mass measures of objects such as galaxies and the observed distribution of luminous matter in the universe is typically explained by invoking an unseen ``dark matter'' component. Dark matter must necessarily be non-baryonic. We introduce a simple hypothesis to do away with the necessity for dark matter by introducing an additional non-gravitational force coupled to baryon number as a charge. We compare this hypothesis to Milgrom's Modified Newtonian Dynamics. The model ultimately fails when confronted with observation, but it fails in an interesting way.
引用
@article{arxiv.astro-ph/0006453,
title = {An attempt to do without dark matter},
author = {William H. Kinney and Martina Brisudova},
journal= {arXiv preprint arXiv:astro-ph/0006453},
year = {2015}
}
备注
To appear in Proceedings of the 15th Florida Workshop in Nonlinear Astronomy and Physics, "The Onset of Nonlinearity" (8 pages, LaTeX, uses nyas.sty)