Newtonian mechanics & gravity fully model disk galaxy rotation curves without dark matter
| dc.creator | Banhatti, Dilip G. | |
| dc.date | 2008-06-06 | |
| dc.date | 2008-07-10 | |
| dc.date.accessioned | 2026-07-07T09:49:17Z | |
| dc.date.available | 2026-07-07T09:49:17Z | |
| dc.description | EGRET gamma-ray archival data used with GALPROP software show two ringlike structures in Milky Way Plane which roughly tally with distribution of stars ([1] & references therein). To understand fully the implications of this and similar results on detailed structure and rotation curve of especially Milky Way Disk as well as rotation curves of other galaxies as derived from spatially resolved spectroscopic data-cubes, a re-examination of the basis of the connection between mass density and rotation curve is warranted. Kenneth F. Nicholson's approach [2], which uses only Newtonian dynamics & gravity, is presented. | |
| dc.description | 6 pages, 5 figures, 1 table (Currently visiting Solid State Theory group at University of Muenster, Germany), For IAU Symposium 254 on Galaxy Disk in Cosmological Context, 9-14 June 2008, Copenhagen, Denmark | |
| dc.identifier | https://arxiv.org/abs/0806.1131 | |
| dc.identifier | http://arxiv.org/abs/0806.1131 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/164532 | |
| dc.subject | Astrophysics | |
| dc.title | Newtonian mechanics & gravity fully model disk galaxy rotation curves without dark matter | |
| dc.type | text |