1 citations · 1 across the 3 of their papers we have counts for
3 papers
astro-ph.GA2016
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…
astro-ph.GA2015
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…
astro-ph.GA2014★ 1 cited
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…