Physical Society Colloquium
Dark Matter and First Galaxies Light Up
Department of Physics UC Davis
The Bullet Cluster has been the subject of intense research in the last few
years. This system is remarkably well-suited to addressing outstanding issues
in both cosmology and fundamental physics. I will present measurements of the
composition of this system, show the evidence for existence of dark matter,
and describe limits that we placed on the intrinsic properties of dark matter
particles. I will also present results from a much larger sample of Bullet-like
clusters, MACSJ0025-1222, A520, and DLSCL J0916.2+2951 among others.
In the second part of my talk I will describe our recent endeavors with
Hubble Space Telescope, Spitzer Space Telescope, Keck, and ALMA that enabled
us to detect galaxies at the time when the Universe was only a few precent of
its current age. They are likely beacons of the epoch of reionization, which
marked the end of the so-called “Dark Ages” and signified
the transformation of the universe from opaque to transparent. Clusters of
galaxies, when used as cosmic telescopes, can greatly simplify the task of
studying and finding these galaxies. With a massive cluster one can gain
several magnitudes of magnification over a typical observing field, enabling
imaging and spectroscopic studies of intrinsically lower-luminosity galaxies
than would otherwise be observable, even with the largest telescopes. I will
present the newest results that seem to suggest that the galaxies have started
forming stars much earlier than previously thought.
Friday, October 28th 2016, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
|