Slide 1 CHALLENGES OF RELATIVISTIC ASTROPHYSICS Reuven Opher (Univ. of Sao Paulo/Cornell. Univ.) Slide 2 WHAT ARE THE BIGGEST PROBLEMS THAT NEED TO BE SOLVED IN RELATIVISTIC…
Cosmological Constraints from the maxBCG Cluster Sample Eduardo Rozo October 12, 2006 In collaboration with: Risa Wechsler, Benjamin Koester, Timothy McKay, August Evrard,…
The formation of galactic disks An overview of Mo Mao & White 1998 MNRAS 295 319 Introduction Disk formation in hierarchical cosmogonies Two component theory: dark matter…
The sdss galaxies at redshift 0.1 What can we learn from the luminosity function and color studies? The sdss galaxies at redshift 0.1 1 OUTline Scientific Questions SDSS…
Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster.. Structure of Massive Star at End of HS Burning Delayed Explosions Neutrino…
The Fate of the Universe The cosmological principle The simplest universes is: Homogenous â the same everywhere you go Isotropic â the same in all directions Discussion…
Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster.. Structure of Massive Star at End of HS Burning Neutrinos Arrive from SN1987A…
Impact of Early Dark Energy on non-linear structure formation Margherita Grossi MPA, Garching Advisor : Volker Springel 3rd Biennial Leopoldina Conference on Dark Energy…
The sdss galaxies at redshift 0.1 What can we learn from the luminosity function and color studies? The sdss galaxies at redshift 0.1 1 OUTline Scientific Questions SDSS…