Astronomical Solutions to Galactic Dark Matter Will Sutherland Institute of Astronomy, Cambridge.
Dark energy by david spergel
Eloisa Menegoni ICRA and INFN, University of Rome “La Sapienza” Cosmological constraints on variations of fundamental constants Miami2010, Fort Lauderdale,
Hydrogen 21cm Cosmology Tzu-Ching Chang (ASIAA) Ue-Li Pen, Kiyo Masui (CITA) Jeff Peterson, Kevin Bandura, Tabitha Voytek, Aravind Natarajan (CMU) Pat.
SOME LIKE IT HOT: dynamical suppression of vacuum configurations in cosmology, and hot CMB A.O.Barvinsky Theory Department, Lebedev Physics Institute,
ACFI-FRIBM. Horoi CMU Double-beta decay and BSM physics: shell model nuclear matrix elements for competing mechanisms Mihai Horoi Department of Physics,
2008/3/13 1 Application of Michelson type bolometric interferometer to CMB B mode polarization observations Makoto Hattori Astronomical Institute Tohoku.
Some Problems in String Cosmology Miao Li Institute of Theoretical Physics Academia Sinica.
Scalar dispersion forces, BE condensation and scalar dark matter J A Grifols, UAB Valparaíso, December 11-15, 2006.
1 What is the Dark Energy? David Spergel Princeton University.
Speaker : Cheon Hwa Sung Yonsei University
Clustering in the Sloan Digital Sky Survey Bob Nichol (ICG, Portsmouth) Many SDSS Colleagues.