Thursday, October 29
AT&T Conference Center, Classroom 105
[map]
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9:10-9:20
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Welcome & Texas Cosmology Center
Eiichiro Komatsu ~ UT Austin
pdf
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9:20-9:30
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Welcome
Mary Ann Rankin ~ Dean of the College of Natural Sciences
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DARK ENERGY
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9:30-9:50
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Supernovae and the Accelerating
Universe
Nick Suntzeff ~ Texas A&M
pdf ~
abstract
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9:50-10:10
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Cosmology with the SDSS II Supernova Survey
Craig Wheeler ~ UT Austin
pdf ~
abstract |
10:10-10:30
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Type Ia Supernovae
Kevin Krisciunas ~ Texas A&M
pdf
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10:30-11:00
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Break
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11:00-11:20
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Hobby-Eberly Dark
Energy Experiment
Karl Gebhardt or Gary Hill ~ UT Austin
pdf
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11:20-11:40
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The Dark Energy Survey
Darren DePoy ~ Texas A&M
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11:40-12:00
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Constraining dark energy with an improved measurement
of the Hubble constant
Lucas Macri ~ Texas A&M
pdf [13MB] ~
abstract
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12:00-1:30
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Lunch Tejas Dining Room
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1:30-2:00
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SPECIAL TALK Carbon Monoxide Line Emission as a CMB
Foreground: Tomography of the Star Forming Universe
Rashid Sunyaev ~ MPI
pdf
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2:00-3:00
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Poster Session
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3:00-3:20
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The growth rate index of large scale structure
as a probe of cosmic acceleration
Mustapha Ishak-Boushaki ~ UT Dallas
pdf ~
abstract |
3:20-3:40
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A transparent instance of how Lambda contributes to the bending of light
Wolfgang Rindler ~ UT Dallas
pdf ~
abstract |
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STRUCTURE FORMATION
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3:40-4:00
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Why does environment matter?
Kim-Vy Tran ~ Texas A&M
pdf ~
abstract
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4:00-4:30
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Break
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4:30-4:50
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Searching for the First Galaxies
Steve Finkelstein ~ Texas A&M
pdf ~
abstract
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4:50-5:10
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Cosmic Reionization
Paul Shapiro ~ UT Austin
pdf [7MB] ~
abstract
When the first stars began to form in the LCDM universe at high redshift,
they released ionizing and dissociating UV radiation into their surroundings
which influenced the formation of other stars and galaxies, near and far,
and left an observable imprint on the first billion years of
cosmic evolution. The theory and simulation of this process depends upon
combining elements of cosmological structure formation on scales large and
small with radiative transfer, gas and gravitational dynamics, to determine
the self-consistent history of cosmic star and galaxy formation, from the
cosmic dark ages thru the epoch of reionization (EOR). I will report on
some of the latest developments on this frontier,
including simulations and predictions of observable signatures,
like the fluctuating background of redshifted 21-cm line radiation, a
fluctuating near-IR background, the temperature and polarization anisotropy
of the CMB, and a distortion of the luminosity function and spatial
clustering observed for Lyman alpha emission-line galaxies during the EOR. |
5:10-5:30
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Simulating cosmological reionization
with Enzo
Daniel Reynolds ~ SMU
pdf ~
abstract
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5:30-7:00
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Reception M3 Pre-function
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7:00-9:00
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Dinner Salon DE
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Friday, October 30
AT&T Conference Center, Amphitheatre 204
[map]
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DARK ENERGY, INFLATION, AND STRINGS
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9:30-9:50
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F-ast Proton Decay
Dimitri Nanopoulos ~ Texas A&M
pdf
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9:50-10:10
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The Horava-Lifshitz and its Applications to Cosmology and Astrophysics
Anzhong Wang ~ Baylor
pdf ~
abstract
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10:10-10:30
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Investigations of the String Landscape
Gerald Cleaver ~ Baylor
abstract |
10:30-11:00
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Break
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11:00-11:20
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Asymptotically Safe Inflation
Steven Weinberg ~ UT Austin
pdf
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11:20-11:40
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String Theory and Inflation
Melanie Becker ~ Texas A&M
pdf ~
abstract
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DARK MATTER
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11:40-12:00
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Dark Matter at the LHC
Bhaskar Dutta ~ Texas A&M
pdf
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12:00-1:30
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Lunch Tejas Dining Room
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1:30-2:00
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SPECIAL TALK Bose-Einstein
Condensation of Dark Matter Axions
Pierre Sikivie ~ Univ. of Florida
pdf ~
abstract
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2:00-2:20
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The Texas Dark Matter Project:
Constraints on Dark Matter Axion Models from White Dwarf Evolution
Don Winget ~ UT Austin
pdf
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2:20
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Adjourn
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