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Toward a Zero-Parameter Model for Galaxy Rotation Curve Data
Sophia Cisneros, James O'Brien, Noah Oblath +3
Modeling the luminous mass components of spiral galaxies in standard gravity poses a challenge due to the missing mass problem. However, with the addition of cold dark matter, the…
The Luminous Convolution Model for spiral galaxy rotation curves
S. Cisneros, J. G. O'Brien, N. S. Oblath +1
The Luminous Convolution Model (LCM) is an empirical formula, based on a heuristic convolution of Relativistic transformations, which makes it possible to predict the observed rota…
The Luminous Convolution Model as an alternative to dark matter in spiral galaxies
S. Cisneros, N. S. Oblath, J. A. Formaggio +6
The Luminous Convolution Model (LCM) demonstrates that it is possible to predict the rotation curves of spiral galaxies directly from estimates of the luminous matter. We consider…