Testing noncommutativity-like model as a galactic density profile
  Noncommutative-like model (NC-like) is an interesting alternative inspired by
string theory to understand and describe the velocity rotation curves of
galaxies without the inclusion of dark matter particles. In a natural way, a
Gaussian density profile emerges and is characterized by a parameter {\theta},
called the NC-like parameter. Hence we aim to confront the NC-like model with a
galaxy sample of the SPARC catalogue to constrain the model parameters and
compare statistically with the Einasto density profile using the Akaike and
Bayesian information criteria. According to our results, some galaxies prefer
the NC-like over the Einasto model while others do not support NC-like.
