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Rupert Croft
Associate Professor
D. Phil., Oxford University
Email: rcroft@andrew.cmu.edu
Phone: (412) 268-8917
FAX: (412) 681-0648
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Cosmology has a "Standard Model", which includes the
Big Bang, Inflation, and Dark Matter. Using this framework, Physical
cosmologists are beginning to understand how structures form, how the
action of gravity amplifies initially tiny perturbations, giving rise to
galaxies, stars and ultimately our own planet. My research
uses as a tool computer simulation codes (running on
parallel computing facilities established in the Physics
department) which evolve model universes forwards in time,
subject to the laws of Physics which have been included:
gravity, gas dynamics, radiative cooling and so on. Our
analytical theories of how astrophysical processes take
place can be checked with these numerical experiments,
which also provide predictions to be compared with
observational data.
I study the Universe both at high and low redshift, using this approach, looking at structure traced by galaxy clusters, galaxies, and
intergalactic gaseous filaments seen as absorption features in the spectra
of quasars. By working closely with observational astrophysicists at
CMU I aim to make use of the enormous quantities of data from
new telescopes, satellites and surveys. Our Universe is the ultimate physics
laboratory, and these new data contain information which will
constrain not only our theories of structure formation within the Universe,
but also the physical processes and parameters which govern
its global evolution.

Selected Publications
Wang, Q. D., Yao, Y., Tripp, T.
M., Fang, T.-T., Cui, W., Nicastro, F., Mathur, S., Williams, R. J., Song, L., &
Croft, R. A. C., “Warm-Hot Gas in and around the Milky Way: Detection and
Implications of O VII Absorption toward LMC X-3”, Astrophys J., 635,
386, (2005).
Altay, G., Colberg, J.M., and
Croft, R. A. C., “The Influence of Large–Scale Structure on Halo Shapes and
Alignments” 2005, Mon. Not. R. astr. Soc., 370, 1422, (2006).
Croft, R. A. C., Banday, A.J.,
& Hernquist, L., “Lyman-alpha forest-CMB cross-correlation and the search for
the ionised baryons at high redshift”, Mon. Not. R. astr. Soc., 369,
1090, (2006).
Kim, Y-R., & Croft, R. A. C.,
“A potentially pure test of cosmic geometry: galaxy clusters and the real space
Alcock-Paczynski test” Mon. Not. R. astr. Soc., 374, 535, (2007).
De, S., & Croft, R. A.
C.,.“Peaks in the cosmological density field: sensitivity to initial power
spectrum, redshift distortions and galaxy halo occupation” Mon. Not. R. astr.
Soc., 382, 1591, (2007).
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