Calendar
2011
September-December
Mon, Dec 5 |
TCC Presentation / Theoretical Astrophysics Seminar Hydrogen and Helium Reionization [abstract] |
Fri, Dec 2 |
Special Astronomy/Physics Joint Colloquium Cosmic Information: IT from BIT, from BITs in IT [abstract] J. Richard Bond, Canadian Institute for Theoretical Astrophysics (CITA) |
Wed, Nov 30 |
TCC Presentation / Cosmos Seminar Giant Gamma-ray Bubbles in the Inner Galaxy: AGN Activity or Bipolar Galactic Wind? [abstract] |
Mon, Nov 21 |
PhD Defense Presentation / Theoretical Astrophysics Seminar Toward an Understanding of the Large Scale Structure of the Universe with Galaxy Surveys [abstract] |
Mon, Nov 14 |
TCC Presentation / Theoretical Astrophysics Seminar The Plasma Physics and Cosmological Implications of TeV Blazars [abstract] Philip Chang, University of Wisconsin, Milwaukee (formerly of CITA-ICAT) |
Wed, Nov 9 |
TCC Presentation / Cosmos Seminar Cosmology without Cosmic Variance [abstract] |
Wed, Nov 2 |
TCC Presentation / Cosmos Seminar The Mass Assembly History of Black Holes in the Universe [abstract] |
Wed, Oct 26 |
TCC Presentation / Cosmos Seminar New Results from the South Pole Telescope [abstract] |
Mon, Oct 24 |
TCC Presentation / Theoretical Astrophysics Seminar From OWLS to FiBY: Numerical Simulations of Galaxy Formation and Evolution [abstract] Claudio Dalla Vecchia, Max Planck Institute for Extraterrestrial Physics |
Mon, Oct 17 |
TCC Presentation / Theoretical Astrophysics Seminar Lyman-alpha in Three Dimensions [abstract] |
Thurs, Sep 29 |
TCC Presentation / Extragalactic Seminar Galaxy Mergers through Cosmic Time [abstract] |
Thurs, Sep 8 |
TCC Presentation / Extragalactic Seminar Galaxy Formation and Evolution through Metals [abstract] |
January-May
Mon, May 23 |
TCC Presentation / Special Seminar Galaxy-Galaxy Weak Lensing as a Tool to Correct Finger-of-God Effects in Redshift Power Spectrum Measurements [abstract] |
Thurs, May 12 |
TCC Presentation / Special Seminar Host vs. Subhalo-2D Density Profile Measured from Galaxy-Galaxy Lensing [abstract] |
Fri, May 6 |
TCC Presentation / Special Seminar Velocity Probe on Cosmology [abstract] |
Thurs, May 5 |
TCC Presentation / Extragalactic Seminar The Dark Matter Halo - Galaxy Connection in the Local Universe and Local Group [abstract] |
Thurs, Apr 28 |
TCC Presentation / Extragalactic Seminar Understanding the Global Course of Galaxy Evolution at z < 1 [abstract] |
Fri, Apr 22 |
TCC Presentation / Special Seminar Obscured Quasars at High Redshift [abstract] |
Tue, Apr 12 |
TCC Presentation / Weinberg Theory Seminar Screening Dark Energy [abstract] |
Wed, Mar 30 |
TCC Presentation / Cosmos Seminar The Influence of Structure Formation on the Interpretation of Dark Matter Experiments [abstract] |
Tues, Mar 8 |
TCC Presentation / Astronomy Colloquium DEEP2 and Beyond: Studying Galaxy Evolution and Large-Scale Structure with Deep Surveys [abstract] |
Tue, Feb 15 |
TCC Presentation / Astronomy Colloquium Is Inhomogeneity Important in Cosmology? [abstract] |
Wed, Feb 9 |
TCC Presentation / Cosmos Seminar High Resolution Imaging of the Sunyaev-Zel'dovich Effect in Galaxy Clusters [abstract] |
Wed, Feb 9 |
TCC Presentation / Stellar Seminar Observational Constraints on Dark Matter Heating in White Dwarf Stars [abstract] |
Mon, Jan 31 |
TCC Special Colloquium / Theoretical Astrophysics Seminar Dark Matter [abstract] All the matter and energy of our daily experience -- tables, chairs, people, air, planets, etc -- constitute only 4% of the total content of the Universe. The majority of the Universe resides in the Dark Side: Dark Matter and Dark Energy. This talk will examine the dark matter that comprises most of the mass of the Milky Way and all other galaxies. I will begin by reviewing the observational evidence for dark matter and then turn to what we think it is. Its existence was first noticed in clusters in the 1930s, and yet its nature remains a mystery still today. I will discuss proposed candidates for the dark matter, which is probably made of some new kind of fundamental particle. The best motivated dark matter particles are Weakly Interacting Massive Particles, or WIMPs, such as supersymmetric particles. A great deal of excitement currently pervades this field because of current and upcoming experiments that are finding hints of dark matter in the form of otherwise unexplained events. We first made these predictions twenty years ago, and it is very exciting that more and more signals are emerging that may in fact be signatures of dark matter detection. These particles have been powerful motivation for the LHC at CERN, the underground experiments such as XENON or CDMS, satellites such as FERMI or PAMELA, and neutrino detectors such as ICECUBE at the South Pole. The current status will be discussed. Dark Stars provide another potential avenue for discovery: we found that the first stars to form in the universe may be powered by WIMP dark matter heating rather than by fusion (a new phase of stellar evolution). Dark Stars may be detectable as well in the upcoming James Webb Space Telescope. Perhaps in the near future the dark matter mystery will be solved. |
Wed, Jan 26 |
TCC Presentation The Matching of the Cosmic Star Formation Rate and the Cosmic Supernova Rate [abstract] |
Wed, Jan 19 |
TCC / Cosmos Seminar Cosmological Imprints of f(R) Gravity [abstract] |
Tue, Jan 18 |
TCC / Colloquium (Tinsley Scholar) Dust in the Early Universe [abstract] |