|Description||2013 Spring Physics Colloquium Series - Weighing and Measuring Galaxy Clusters, the Most|
Massive Objects in the Universe
Lindsay King, Ph.D.
Associate Professor, Department of Physics
University of Texas at Dallas
Galaxy clusters are the most massive bound objects in the universe, and most of
their mass is dark matter that cannot be seen directly with telescopes. Most of
their normal baryonic luminous matter is hot X-ray emitting gas, that enshrouds
clusters. Stars that shine in galaxies, seen using optical telescopes, account for a
smaller amount of this normal matter. Being able to map out the mass in
clusters allows key tests of our paradigm for structure formation in the
universe, and of the properties of dark matter itself. My talk will begin with an
outline of how strong and weak gravitational lensing signatures are used as a
tool to study cluster structure. I will then discuss facets of our theoretical and
observational research in this area.
One topic that we will consider is how the physics of baryonic matter impacts
on the distribution of mass (and hence lensing signatures) in clusters formed in
hydrodynamic computer simulations. In particular, I will discuss the importance
of the physics of supermassive black holes, hosted by cluster galaxies, in
shaping lensing signatures such as the number of giant arcs - highly magnified
and distorted images of distant galaxies.
Over the past few years, it has been discovered that "Bullet Clusters" offer a new
window on dark matter as well as testing gravity on large scales. These are the
most energetic events since the big bang, comprising two or more clusters that
have collided in the past - so violently that their dark matter and hot X-ray gas
have been separated. Only a handful of these events are known, and we will
focus on Abell 2146, a unique system that we are currently investigating.
Room E.125, Baylor Sciences Building
Reception at 3:40 p.m. in BSB D.311
For more information contact:
Dr. Anzhong Wang 254-710-2276