Big Bang
Chris Clarkson - Testing the Copernican Principle
Evolution of universe
If the universe were perfectly uniform, then how come the microwave background isn’t uniform? Where did all the structure(galaxies, clusters, etc.) come.
Quantum vacuum and the gravitational repulsion between matter and antimatter: a key for the understanding of the Universe? D.S. Hajdukovic GBAR Collaboration.
The next decade of weak lensing science Rachel Mandelbaum, CMU.
1 1 Dark Energy in Dark Antarctica Dark Energy in Dark Antarctica Eric Linder 21 July 2009 Berkeley Center for Cosmological Physics, UC Berkeley & Berkeley.
D.S. Hajdukovic GBAR Collaboration Meeting 18 th April 2012
The next decade of weak lensing science
C luster L ensing A nd S upernova survey with H ubble
