89 citations · 340 across the 11 of their papers we have counts for
11 papers
Equation of state, universal profiles, scaling and macroscopic quantum effects in Warm Dark Matter galaxies
H. J. de Vega, N. G. Sanchez
The Thomas-Fermi approach to galaxy structure determines selfconsistently and nonlinearly the gravitational potential of the fermionic WDM particles given their quantum distributio…
Quantum WDM fermions and gravitation determine the observed galaxy structures
C. Destri, H. J. de Vega, N. G. Sanchez
Quantum mechanics is necessary to compute galaxy structures at kpc scales and below. This is so because near the galaxy center, at scales below 10 - 100 pc, warm dark matter (WDM)…
Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics
C. Destri, H. J. de Vega, N. G. Sanchez
We derive the main physical galaxy properties: mass, halo radius, phase space density and velocity dispersion from a semiclassical gravitational approach in which fermionic WDM is…
Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio r
C. Destri, H. J. de Vega, N. G. Sanchez
The MCMC analysis of the CMB+LSS data in the context of the Ginsburg-Landau approach to inflation indicated that the fourth degree double--well inflaton potential best fits the pre…
Model independent analysis of dark matter points to a particle mass at the keV scale
H. J. de Vega, N. G. Sanchez
We present a model independent analysis of dark matter (DM) both decoupling ultra relativistic (UR) and non-relativistic (NR) based in the phase-space density D = rho_{DM}/sigma^3_…
The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
D. Boyanovsky, C. Destri, H. J. de Vega +1
Inflation is part of the Standard Model of the Universe supported by CMB and large scale structure LSS datasets. This review presents new developments of inflation in three main ch…