Calendar
2012
September-December
Wed, Dec 12 - Fri, Dec 14 |
Cosmological Radiative Transfer Comparison Project Workshop IV 3-day Cosmology Workshop: click link, above, for details |
January-May
Mon, May 14 - Tues, May 15 |
TCC NIRB Workshop Near Infrared Background and the Epoch of Reionization [abstract] |
Mon, May 7 - Tues, May 8 |
TCC Gamma-Ray Workshop Dark Matter Signatures in the Gamma-Ray Sky [abstract] hosts: Eiichiro Komatsu & Can Kilic, University of Texas at Austin |
Tue, May 1 |
TCC / Colloquium Constraining Cosmology through the Growth of Structure: New Results from the South Pole Telescope [abstract] |
Mon, Apr 23 |
TCC / Astro Theory Seminar New Probes of Weak Lensing [abstract] |
Wed, Apr 18 |
TCC / Cosmos Seminar Constraining Dark Matter [abstract] Astrophysical and cosmological observations provide
compelling evidence for the existence of dark matter in the universe,
but its particle physics nature remains mysterious. In this talk, I
will discuss how hardron colliders and neutron stars can help us
understand dark matter properties. Using an effective field theory
approach, we show that mono-jet+missing energy searches at the
Tevatron and LHC can provide a probe of dark matter, which is
complementary to direct detection experiments, and in some cases the
colliders provide an even stronger constraint. Stellar systems are
natural laboratories
for exploring dark matter. We show dark matter particles accumulated
in old neutron stars can form mini black holes and lead to the
destruction of host stars. The observation of old neutron stars
actually excludes a class of dark matter models. In this talk, I will
also talk about self-interacting dark matter. |
Wed, Mar 28 |
TCC / Cosmos Seminar Cosmic Infrared Background and New Cosmological Populations [abstract] Alexander "Sasha" Kashlinsky, NASA, Goddard Space Flight Center |
Mon, Mar 26 |
TCC / Cosmos Seminar Measuring the Large-Scale Flow of X-ray Luminous Clusters from WMAP Data [abstract] Alexander "Sasha" Kashlinsky, NASA, Goddard Space Flight Center |