|
|
WMAP-1: 2 years after
|
|
10/24/2005 12:00:00 PM
EST
|
37 Minutes 14 Seconds
|
|
|
Limits on non-gaussianities from WMAP data
|
|
10/24/2005 12:30:00 PM
EST
|
25 Minutes 32 Seconds
|
|
|
Large-scale structure from the Sloan Digital Sky Survey
|
|
10/24/2005 1:00:00 AM
EST
|
32 Minutes 7 Seconds
|
|
|
Cosmological Model Selection and the Inflationary Cosmology
|
|
10/24/2005 3:00:00 PM
EST
|
2 Hours 3 Minutes 35 Seconds
|
|
|
Reheating and Thermalization after inflation
|
|
10/24/2005 5:00:00 PM
EST
|
32 Minutes 10 Seconds
|
|
|
Singularities in String Theory
|
|
10/25/2005 9:30:00 AM
EST
|
2 Hours 1 Minute 3 Seconds
|
|
|
Density perturbations in singularity-free quantum cosmology
|
|
10/25/2005 12:00:00 PM
EST
|
27 Minutes 47 Seconds
|
|
|
String Pair Production in a Time-Dependent Gravitational Field
|
|
10/25/2005 12:30:00 PM
EST
|
25 Minutes 2 Seconds
|
|
|
Anthropic prediction for Lambda and the Q catastrophe
|
|
10/25/2005 1:00:00 PM
EST
|
35 Minutes 30 Seconds
|
|
|
Supernova observations and dark energy
|
|
10/25/2005 3:00:00 PM
EST
|
1 Hour 37 Minutes 25 Seconds
|
|
|
Dynamics of Dark Energy
|
|
10/25/2005 5:00:00 PM
EST
|
47 Minutes 9 Seconds
|
|
|
Laboratory tests of the Equivalence Principle and the Inverse Square Law
|
|
10/26/2005 9:30:00 AM
EST
|
1 Hour 12 Minutes 54 Seconds
|