Postdoctoral Fellow
Canadian Institute for Theoretical Astrophysics
research interests: computational cosmology; first stars and
black holes; reionization; 21-cm observations of the EOR; galaxy
formation; physics of the IGM; large-scale structure
of the universe
Gallery
send questions, comments, or requests to: malvarez 'at' cita.utoronto.ca
Poster showing different aspects of reionization.
Poster by M. Alvarez Background visualization by M. Alvarez and T. Abel
See Alvarez et al. (2009) for more details.
Shows the vast range of length scales involved in the process of
reionization. On the left is shown the result of a large scale
semi-numerical calculation of reionization, while right panels
show the result of a small scale calculations on much smaller scales,
with a relatively dim flux as would occur when a patch is just
beginning to be reionized (top-right), and a much higher flux as would
occur near a number of bright galaxies (bottom-right).
Large scale (left) visualization by M. Alvarez, R. Kaehler, and T. Abel Small scale (right) visualization by J. Emberson and M. Alvarez Large scale (left) simulation by M. Alvarez and T. Abel Small scale (right) simulation by J. Emberson, R. Thomas, and M. Alvarez
left: Reionization redshift in a 0.5 Mpc/h-thick slice for a
reionization simulation with a mean free path of 256 Mpc/h (top)
and 8 Mpc/h (bottom). Clockwise beginning from top-left,
regions shown are 2 Gpc/h, 500 Mpc/h, and 125 Mpc/h across.
The radii of the circles correspond to the photon mean free path.
right: Same as left panels but for the projected ionized
fraction in a 5 Mpc/h-thick slice at a time when the mean
volume-weighted ionized fraction is 0.75. Note that the ionization
field contains considerably more small scale structure in the
8 Mpc/h mean free path case.