L. Arturo Ureña-López

Further analysis of a cosmological model with quintessence and scalar dark matter

We present the complete solution to a

New cosmological tracker solution for quintessence

95%

Quintessence and scalar dark matter in the Universe

scalar field cosmological model in which the dark matter is modeled by a scalar field

Gravitational cooling of self-gravitating Bose-Condensates

ensuremath{Phi}

Evolution of the Schrodinger-Newton system for a self-gravitating scalar field

with the scalar potential

Scalar field as dark matter in the universe

V(ensuremath{Phi}{)=V}_{0}[mathrm{cosh}(ensuremath{lambda}sqrt{{ensuremath{kappa}}_{0}}ensuremath{Phi})ensuremath{-}1]

Inflation, dark matter, and dark energy in the string landscape

and the dark energy is modeled by a scalar field ensuremath{Psi}, endowed with the scalar potential

Bose-Einstein condensation of relativistic Scalar Field Dark Matter

stackrel{ifmmode tilde{}else ~{}fi{}}{V}(ensuremath{Psi})={V}_{0}[mathrm{sinh}(ensuremath{alpha}sqrt{{ensuremath{kappa}}_{0}}ensuremath{Psi}){]}^{ensuremath{beta}}.

ON THE DYNAMICS OF A QUADRATIC SCALAR FIELD POTENTIAL

This model has only two free parameters, ensuremath{lambda} and the equation of state

Inflaton field as self-interacting dark matter in the braneworld scenario

{ensuremath{omega}}_{ensuremath{Psi}}.