SANTOS, V. C. S.; http://lattes.cnpq.br/3246941835824922; SANTOS, Vivianni Cordeiro de Sousa.
Resumo:
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.