Eilat Glikman (Physics) has been awarded a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy on behalf of the National Aeronautics and Space Administration, to lead a research project titled Testing the Triggering Mechanism for Luminous, Radio-Quiet Red Quasars in the Clearing Phase: A Comparison to Radio-Loud Red Quasars. This three year project, involving collaborators from Yale University, the National Radio Astronomy Observatory, the University of California San Diego, and the Leibniz Institute of Astrophysics in Potsdam, Germany, is based on observations of radio-quiet dust-reddened quasars and involves a study of the relationship between radio emission and host galaxy morphology. Evidence for mergers would support a picture in which luminous quasars and galaxies co-evolve independent of their radio properties; whereas the absence of mergers would link radio emission to mergers and require an alternate explanation for the extreme properties of these radio-quiet dust-reddened quasars. If mergers do not dominate the evolution of radio-quiet quasars, then a new paradigm for black hole and galaxy growth will need to be established.