Scalar Fields as Dark Matter in Spiral Galaxies
F. Siddhartha Guzman, Tonatiuh Matos

TL;DR
This paper proposes a scalar field model for dark matter in spiral galaxies based on Einstein-Dilaton theory, successfully matching observed rotation curves with a specific energy density profile.
Contribution
It introduces an exact static, axially symmetric solution of Einstein-Dilaton theory modeling dark matter as a scalar field with a potential, aligning with galaxy rotation observations.
Findings
Effective energy density scales as 1/(r^2 + r_c^2)
Circular velocity profiles match observed galaxy rotation curves
Model provides a new theoretical framework for dark matter in galaxies
Abstract
We present a model for the dark matter in spiral galaxies, which is a result of a static and axial symmetric exact solution of the Einstein-Dilaton theory. We suposse that dark matter is a scalar field endowed with a scalar potential. We obtain that a) the effective energy density goes like and b) the resulting circular velocity profile of tests particles is in good agreement with the observed one.
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