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Bradley E. Schaefer
Professor of Physics & Astronomy
Ph.D., 1983 - Massachusetts Institute of Technology
Office: 243-A Nicholson
Telephone: 0015-Office
E-mail:
RESEARCH INTERESTS
One primary thrust of research is to use photometry of exploding objects to get results of interest for cosmology:
For Gamma-Ray Bursts, the big advance has been the realization that the bursts are standard candles (like Type Ia Supernovae and Cepheids). With this, GRBs become tools for cosmology that can be seen out to red shifts from ~0.2 to around 20. This allows GRBs to be light sources for the first real detection of the Gunn-Peterson effect, to create a Hubble Diagram from 0.2<z<10, and to measure the star formation rate of our Universe out to z~20.
For supernovae, as part of the Supernova Cosmology Project, a Hubble Diagram was created with high accuracy out to a red shift of ~1.0. This demonstrated that the Cosmological Constant is non-zero and causes our Universe's expansion to accelerate.
For Recurrent Novae, the question is whether they are the progenitors of Type Ia supernovae, as the knowledge of the progenitor type is required for any evolution calculation such as is needed for the future precision cosmology with supernovae. To answer the progenitor question, extensive work is being pursued to get Recurrent Novae orbital periods, accretion rates, outburst dates, eruption light curves, and the average magnitudes between outbursts. A centerpiece of this work is the timing of eclipses from U Sco and CI Aql since 1897 to measure the orbital period change across the latest eruptions (in 1999 and 2000 respectively) to get the first measure of the ejected mass which allows for knowing whether the white dwarf is gaining or losing mass.
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Updated: Thu, 20-Sep-2007 3:27 PM