All
Energy Frontier
Cosmic Frontier
Intensity Frontier Physics
Theoretical Physics
Particle Data Group
Detector R & D
Affiliates
Staff
Postdocs/Visiting Scholars
Graduate Students
Alumni
The SCP is conducting a search for very distant (redshifts greater than 1.2) Type Ia supernovae using the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope.
The Nearby Supernova Factory (SNfactory) is designed to address a wide range of supernova issues using detailed observations of low-redshift SN.
The LUX experiment is a 350 kg liquid xenon time-projection chamber that aims to directly detect galactic dark matter in an underground laboratory 1 mile under the earth, in the Black Hills of South Dakota, USA.
The most conclusive and carefully examined evidence for The Big Bang is the existence of an isotropic radiation bath that permeates the entirety of the universe known as the cosmic microwave background (CMB).
DESI will measure the effect of dark energy on the expansion of the universe. It will obtain spectra for tens of millions of galaxies and quasars, constructing a 3D map of the universe to 10 billion light years.
The Baryon Oscillation Spectroscopic Survey (BOSS) will map the spatial distribution of luminous red galaxies (LRGs) to detect the scale imprinted by early universe oscillations.
This page
Other pages
Account
