Precision Studies of Dark Energy with LSST
arXiv:astro-ph/0609516 · doi:10.1063/1.2402596
Abstract
Starting around 2013, data from the Large Synoptic Survey Telescope (LSST) will be analyzed for a wide range of phenomena. By separately tracing the development of mass structure and rate of expansion of the universe, these data will address the physics of dark matter and dark energy, the possible existence of modified gravity on large scales, large extra dimensions, the neutrino mass, and possible self interaction of dark matter particles.
9 pages, 3 figures, Talk given at CIPANP 2006, 9th Conference on the Intersections of Particle and Nuclear Physics, May 30-June 3, 2006, Rio Grande, Puerto Rico
Cited by in corpus (7)
- Reconstructing Redshift Distributions with Cross-Correlations: Tests and an Optimized Recipe
- Nonlinear growth in modified gravity theories of dark energy
- Axion constraints in non-standard thermal histories
- Re-capturing cosmic information
- Observational Constraints on Exponential Gravity
- The Northern Sky Optical Cluster Survey III: A Cluster Catalog Covering Pi Steradians
- Magnification Bias Corrections to Galaxy-Lensing Cross-Correlations