Ratra has worked in a number of areas of cosmology and astroparticle and early universe physics. In 1988, Ratra and
Jim Peebles of Princeton University proposed the first dynamical
dark energy scalar field, or
quintessence, model.
Dark energy is the leading candidate for the mechanism that is responsible for causing the observed accelerated cosmological expansion. Ratra and his students and collaborators have pioneered measurements of the redshift of the transition between an earlier epoch when cosmological expansion decelerated because dark and baryonic (ordinary) matter dominated the cosmological energy budget and the current epoch where the cosmological expansion accelerates because dark energy dominates the current cosmological energy budget. Ratra and his students and collaborators have developed new cosmological probes and used these in conjunction with better-established ones to measure the Hubble constant (
Hubble's law), the geometry of space (
Shape of the universe), and
dark energy dynamics. Ratra's early universe research includes the first consistent semi-classical computation of the spectrum of energy density perturbations from
inflation. He collaborated with
Willy Fischler of the University of Texas at Austin and
Leonard Susskind of Stanford University on this computation. He has also computed the power spectrum of energy density perturbations in non-spatially-flat inflation models. Ratra also proposed the first inflation model that can generate, from quantum fluctuations, a large-enough primordial cosmological magnetic field to be able to explain observed galactic magnetic fields. == Honours ==