|
CODE |
SPEAKER |
TITLE OF LECTURE |
| 8:45-9:00 |
WELCOME
|
| 9:00-10:00 |
AP.1 |
I. ANTONIADIS |
The Physics of Extra Dimensions |
| 10:00-11:00 |
AP.2 |
G. LAZARIDES |
Particle Physics Approach to Dark Matter |
| 11:00-11:30 |
COFFEE
|
| 11:30-12:30 |
OB.1 |
J. SILK |
Dark Matter and Galaxy Formation |
| 12:30-13:30 |
AP.3 |
A. LAHANAS |
LSP as Candidates for Dark Matter |
| 13:30-14:30 |
LUNCH
|
| 16:30-17:00 |
S.1 |
M. PLIONIS |
Constraining the Equation of State from High-Redshift AGN Clustering and the SN Ia |
| 17:00-17:30 |
S.2 |
I. AREFEVA |
String Field Model of Cosmological Dark Energy |
| 17:30-18:00 |
S.3 |
E. ABDALLA |
Strong Gravity: Perturbative and non Perturbative Aspects |
| 18:00-18:30 |
COFFEE
|
| 18:30-18:50 |
S.4 |
H. CULETU |
Is the Rindler Horizon Energy Nonvanishing? |
| 18:50-19:10 |
S.5 |
C. CARVALHO |
Cosmological Perturbations from the Brane-Bulk Interaction |
| 19:10-19:25 |
S.6 |
E. MAJEROTTO |
Observational Constraints on Interacting Dark Energy Models |
| 19:25-19:40 |
S.7 |
D. SAPORE |
Cosmological Observations through the Baryonic Oscillations on the Power Spectrum |
|
CODE |
SPEAKER |
TITLE OF LECTURE |
| 9:00-10:00 |
AP.1 |
I. ANTONIADIS |
The Physics of Extra Dimensions |
| 10:00-11:00 |
AP.2 |
G. LAZARIDES |
Particle Physics Approach to Dark Matter |
| 11:00-11:30 |
COFFEE
|
| 11:30-12:30 |
OB.1 |
J. SILK |
Dark Matter and Galaxy Formation |
| 12:30-13:30 |
TH.1 |
I. VERGADOS |
Methods of Direct Detection of Dark Matter |
| 13:30-14:30 |
LUNCH
|
| 16:30-17:00 |
S.8 |
K. TAMVAKIS |
Bulk Fields with Gauge Interactions |
| 17:00-17:30 |
S.9 |
C. MARTINS |
The Quest for Cosmological Scalar Fields |
| 17:30-18:00 |
S.10 |
J. CERVANTES-COTA |
The Influence of Scalar Fields on Galactic Dynamics |
| 18:00-18:30 |
COFFEE
|
| 18:30-18:45 |
S.11 |
C. MOUSTAKIDIS |
The Role of Ionization Electrons in Direct Dark Matter Detection |
| 18:45-19:00 |
S.12 |
B. CUADROS-MELGAR |
The Need of Dark Energy for Dynamical Compactification of Extra Dimensions on the Brane |
| 19:00-19:15 |
S.13 |
P. PASIPOULARIDES |
Stable Solutions for 5D Gravity with a non Minimally Coupled Scalar Field
|
| 19:15-19:30 |
S.14 |
M. WYMAN |
Unique Observational Signatures of Cosmic Superstrings |
| 19:30-19:45 |
S.15 |
A. AVGOUSTIDIS |
Cycloops: Dark Matter from Extra Dimensions? |
|
CODE |
SPEAKER |
TITLE OF LECTURE |
| 9:00-10:00 |
OB.2 |
R. CRITTENDEN |
Dark Energy in the Cosmic Background |
| 10:00-11:00 |
TH.2 |
M. BRUNI |
Cosmological Perturbations and Dark Energy |
| 11:00-11:30 |
COFFEE
|
| 11:30-12:30 |
TH.3 |
M. SAMI |
Cosmological Models for Dark Energy |
| 12:30-13:30 |
OB.3 |
W. PERCIVAL |
Large Scale Structure and Cosmological Parameters |
| 13:30-14:30 |
LUNCH
|
| 16:30-17:00 |
S.16 |
C. CHARMOUSIS |
Higher Dimensional Gravity |
| 17:00-17:30 |
S.17 |
M. FAIRBAIRN |
Photon Mixing in Domain Walls and the Cosmic Coincidence Problem
|
| 17:30-18:00 |
S.18 |
A. PAPAZOGLOU |
Constraints in the Cosmology of Conical Branes
|
| 18:00-18:30 |
COFFEE
|
| 18:30-18:50 |
S.19 |
G. KOFINAS |
Braneworld Cosmologies from Six Dimensions
|
| 18:50-19:05 |
S.20 |
V. ZAMARIAS |
Avoidance of Early-Time Singularity and no Late-Time Dark Energy in Braneworlds |
| 19:05-19:20 |
S.21 |
WONG WAN YAN |
Spectral Distortions to the CMB from the Recombination of H and He |
| 19:20-19:35 |
S.22 |
T. GIANNANTONIO |
Integrated Sachs-Wolfe Effect and Dark Energy |
| 19:35-19:50 |
S.23 |
T. SOTIRIOU |
f(R) Theories of Gravity and their Newtonian Limit |
21:00 |
BANQUET |
|
CODE |
SPEAKER |
TITLE OF LECTURE |
| 9:00-10:00 |
OB.4 |
P. TOZZI |
Cosmological Parameters from Galaxy Clusters |
| 10:00-11:00 |
TH.4 |
R. MAARTENS |
Dark Energy from Modified Gravity |
| 11:00-11:30 |
COFFEE
|
| 11:30-12:30 |
TH.5 |
R. SANDERS |
Modified Gravity without Dark Matter |
| 12:30-13:30 |
TH.6 |
R. WOODARD |
Avoiding Dark Energy with 1/R Modifications of Gravity |
| 13:30-14:30 |
LUNCH
|
| 16:30-17:00 |
S.24 |
L. PERIVOLAROPOULOS |
Reconstruction of Extended Quintessence Potentials |
| 17:00-17:30 |
S.25 |
S. TSUJIKAWA |
A Unified Analysis for Cosmological Scaling Solutions and its Application to Dark Energy
|
| 17:30-18:00 |
S.26 |
A. TOPORENSKY |
Cosmological Dynamics in Induced Gravity Brane Models
|
| 18:00-18:30 |
COFFEE
|
| 18:30-19:00 |
S.27 |
SARBEN SARKAR |
Decoherence from Noncritical Strings
|
| 19:00-19:30 |
S.28 |
B. WANG |
Constraints on the Dark Energy from the Holographic Connection to the small l CMB suppression
|
