Modelando a matéria escura com campos escalares.

Abstract

Experimental data from probes and computational work are ways of detecting and measuring the concentration of dark matter in galaxies and clusters via astrophysical phenomena such as gravitational lensing, Big Bang nucleosynthesis ,cosmic background radiation, the rotation curves of spiral galaxies and more recently the merging of Bala Cluster are explored to explain the dark matter problem. Proposals of this matter constituents are discussed and we investigate a model of Bose-Einstein Condensate which describes dark matter as superfluid building a model to describe the galaxys halo and via the creation of an specific potential.