Richard F. Holman
Professor
Ph.D., Johns Hopkins University
Email: rh4a@andrew.cmu.edu
Phone: (412) 268-5159
FAX: (412)
681-0648
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My interests center mainly on the interface between cosmology and
particle physics. I have very strong interests in the quantum
mechanics/field theory involved in inflationary cosmologies. This has led
me to spending a great deal of time developing a formalism that can be used to
describe quantum fields in non-equilibrium environments, such as occur during
and immediately after an inflationary phase. This formalism has also had
very interesting applications to the so-called Dark Energy problem.
I am currently involved in trying to understand how current and future
measurements of the Cosmic Microwave Background Radiation could detect effects
coming from Planck-Scale physics, as well as constructing models that describe
the so-called Dark Energy component of the Universe.

Selected Publications
"Renormalization of Initial Conditions and the Trans-Planckian
Problem of Inflation," by Hael Collins and R. Holman, Phys. Rev. D 71
(2005) 085009.
"Dark Energy from Wet Dark Fluid," by R.Holman and
Siddhartha Naidu, submitted to JCAP (2004).
"The Fate of the Alpha-Vacuum," by Hael Collins, R.
Holman and Matthew R. Martin, Phys. Rev. D 68 (2003) 124012.
"Are Inflationary Predictions Sensitive to Very High
Energy Physics?," by C.P. Burgess, J.M. Cline, F. Lemieux, and R. Holman, JHEP
0302 (2003) 048.
"Radion Induced Brane Preheating," by Hael Collins, R.
Holman and Matthew R. Martin, Phys. Rev. Lett.
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