- Conference date: 17-19 October 2006
- Location: Madrid (Spain)
Spiral galaxy rotation curves are described using Carmeli’s Cosmological General Relativity. A Tully‐Fisher type relation results and rotation curves are reproduced without the need for non‐baryonic halo dark matter. For accelerations larger than a critical value the Newtonian force law applies, but for accelerations less than the critical value the Carmelian force law applies.
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