School Program
Date & Time |
09:00-10:30 | 10:30-11:00 | 11:00-12:30 | 12:30-16:30 | 16:30-18:00 | 18:00-18:30 | 18:30-20:00 | |
Sunday, Jan. 16th | SF - Inf | Break | GL | Lunch | SF - Inf | Break | T | |
Monday, Jan. 17th | GL | BC | SF - Inf | T/S1 | ||||
Tuesday, Jan. 18th | BRCP | BC | CMB-SA | S2 | ||||
Wednesday, Jan. 19th | BC | SF - Inf | CMB-SA | T/S3 | ||||
Thursday, Jan. 20th | CMB | CMB-SA | WL | CMB-SA | ||||
Friday, Jan. 21st | E X C U R S I O N | |||||||
Saturday, Jan. 22nd | WL | Break | HzU | Lunch | CMB | Break | S4/S5 | Reception |
Sunday, Jan. 23rd | WL | CMB | HzU | HzU | ||||
Monday, Jan. 24th | HzU | S6 / S7 | EXCURSION |
Topics Abbreviation | Related Lecturers |
SF = Structure Formation
Inf = Inflation
GL = Gravitational Lensing
BC = Brane Cosmology
CMB = Cosmic Microwave Background
SA = Secondary Anisotropies
HzU = High Z Universe
WL = Weak-Lensing
BRCP= Back-Reaction of Cosmological Perturbations
T = Tutorial
S = Seminar
|
SF : R. Brandenberger
Inf : R. Brandenberger
GL : S. Rahvar
CMB-SA: N. Afshordi BC : R. Maartens
HzU : B. Mobasher
WL : U. Seljak
BRCP: G. Geshnizjani
CMB: U. Seljak
|
Seminars
Topics Abbreviation | Related Speaker |
S1 = Rotational symmetries of the CMB statistics
S2 = Dynamics of Compact Objects
S3 = Varying light speed theories & cosmology
S4 = Iranian National Observatory, Status review of an exciting project S5 = Spherical symmetric thick domain wall S6 = Vaccum quantum effects for branes on Ad S7 = Magellanic stream |
S1: A. Hajian S2: Y. Sobouti S3: N. Jafari
S4: S. Arbabi S5: S. Khosravi S6: A. Saharian S7: H. Haghi |