activity
19932021
most citedPhase transitions in the early and the present Universe

148 citations · 1.1k across the 28 of their papers we have counts for

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hep-ph200612 cited

Non equilibrium dynamics of mixing, oscillations and equilibration: a model study

D. Boyanovsky, C. M. Ho

The non-equilibrium dynamics of mixing, oscillations and equilibration is studied in a field theory of flavored neutral mesons that effectively models two flavors of mixed neutrino…

astro-ph200663 cited

CMB quadrupole suppression: I. Initial conditions of inflationary perturbations

D. Boyanovsky, H. J. de Vega, N. G. Sanchez

We investigate the issue of initial conditions of curvature and tensor perturba- tions at the beginning of slow roll inflation and their effect on the power spectra. Renormalizabil…

astro-ph200660 cited

CMB quadrupole suppression: II. The early fast roll stage

D. Boyanovsky, H. J. de Vega, N. G. Sanchez

Within the effective field theory of inflation, an initialization of the classical dynamics of the inflaton with approximate equipartition between the kinetic and potential energy…

hep-ph200613 cited

Space-time propagation of neutrino wave packets at high temperature and density

C. M. Ho, D. Boyanovsky

We study the space-time evolution of ``flavor'' neutrino wave-packets at finite temperature and density in the early Universe prior to BBN. We implement non-equilibrium field theor…

hep-ph2006148 cited

Phase transitions in the early and the present Universe

D. Boyanovsky, H. J. de Vega, D. J. Schwarz

The evolution of the Universe is the ultimate laboratory to study fundamental physics across energy scales that span about 25 orders of magnitude: from the grand unification scale…

astro-ph2006

Clarifying Slow Roll Inflation and the Quantum Corrections to the Observable Power Spectra

D. Boyanovsky, H. J. de Vega, N. G. Sanchez

Slow-roll inflation can be studied as an effective field theory. The form of the inflaton potential consistent with the data is V(phi) = N M^4 w(phi/[sqrt{N} M_{Pl}]) where phi is…