Galaxy Rotation Curves without Dark Matter
Galaxy rotation curves are flat at large radii, which in ΛCDM requires dark matter halos. The τ-framework derives flat rotation curves from the boundary reading…
Physics
High impact frontier problem
ASTRO
Book V
Public
Manuscript
Physics cascade
In plain language
Galaxy rotation curves are flat at large radii, which in ΛCDM requires dark matter halos. The τ-framework derives flat rotation curves from the boundary reading…
Overview
Galaxy rotation curves are flat at large radii, which in ΛCDM requires dark matter halos. The τ-framework derives flat rotation curves from the boundary reading without dark matter particles.
Result Statement
Flat rotation curves from boundary reading of τ³. No dark matter halos needed. Status: Internally addressed.