Research @ KICP
The most striking recent development in cosmology was the discovery that the expansion of the universe is speeding up. Initially discovered by observations of distant Type Ia supernovae, this effect has now been confirmed by observations of the CMB anisotropy, the large-scale galaxy distribution, and the evolution of the galaxy cluster abundance. While the existence of cosmic acceleration is now firmly established, its physical origin remains a deep mystery. Within General Relativity, Einstein's theory of gravity, vacuum energy (i.e. the Cosmological Constant) smooth compared with the dark matter could be responsible. Alternatively, General Relativity may need to be modified or replaced to correctly explain the acceleration.
Identifying the physical cause of the cosmic acceleration is a key challenge for fundamental physics in the coming decade. Answering this question requires multiple astrophysical and cosmological techniques, analysis of multiple, large-volume data sets, and synergy between theory and observations. The Dark Energy MA was created to take on this challenge. The goals of the MA are to address whether or not cosmic acceleration requires a modification of Einstein's theory of gravity, General Relativity, and if not, to probe the nature of the dark energy that is driving acceleration and that makes up 75% of the universe.
In order to meet these goals, the MA will seek to measure the dark energy equation of state parameter to high precision and accuracy and to test the consistency of General Relativity with cosmic acceleration by measuring the cosmic expansion history and growth rate of large-scale structure. The MA is engaging in the following specific activities to achieve its plans:
Joint Analysis Hub
The Joint Analysis Hub will spearhead efforts to bring together the major dark energy/cosmic acceleration experiments and teams to combine datasets in a consistent and powerful way.
High redshift observations of Type Ia Supernovae (SN) provided the first convincing evidence for the existence of Dark Energy (DE). These observations remain one of the most useful tools for constraining cosmological parameters. Despite numerous advances in observational and theoretical techniques towards understanding Type Ia SN, there remain many potential systematic uncertainties that can limit the cosmological precision obtainable from SN surveys. These systematic uncertainties have become the limiting factor in SN constraints on DE. It is the goal of the Supernova Hub to carry out a research program to understand and reduce these potential systematic errors, thereby improving SN as cosmological probes.