Report of the Dark Energy Task Force
Abstract
Dark energy appears to be the dominant component of the physical Universe, yet there is no persuasive theoretical explanation for its existence or magnitude. The acceleration of the Universe is, along with dark matter, the observed phenomenon that most directly demonstrates that our theories of fundamental particles and gravity are either incorrect or incomplete. Most experts believe that nothing short of a revolution in our understanding of fundamental physics will be required to achieve a full understanding of the cosmic acceleration. For these reasons, the nature of dark energy ranks among the very most compelling of all outstanding problems in physical science. These circumstances demand an ambitious observational program to determine the dark energy properties as well as possible.
Cite
@article{arxiv.astro-ph/0609591,
title = {Report of the Dark Energy Task Force},
author = {Andreas Albrecht and Gary Bernstein and Robert Cahn and Wendy L. Freedman and Jacqueline Hewitt and Wayne Hu and John Huth and Marc Kamionkowski and Edward W. Kolb and Lloyd Knox and John C. Mather and Suzanne Staggs and Nicholas B. Suntzeff},
journal= {arXiv preprint arXiv:astro-ph/0609591},
year = {2007}
}
Comments
The Dark Energy Task Force (DETF) was established by the Astronomy and Astrophysics Advisory Committee (AAAC) and the High Energy Physics Advisory Panel (HEPAP) as a joint sub-committee to advise the Department of Energy, the National Aeronautics and Space Administration, and the National Science Foundation on future dark energy research