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Report

Report of the Dark Energy Task Force

Andreas AlbrechtUniv. of California, Davis, CA (United States)Gary BernsteinUniv. of Pennsylvania, Philadelphia, PA (United States)R. N. CahnLawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)Wendy L. FreedmanCarnegie Inst. of Washington, Washington, DC (United States). ObservatoriesJacqueline HewittMassachusetts Inst. of Technology (MIT), Cambridge, MA (United States)Wayne HuUniv. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)John HuthHarvard Univ., Cambridge, MA (United States)Marc KamionkowskiCalifornia Inst. of Technology (CalTech), Pasadena, CA (United States)Edward W. KolbFermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Astronomy Astrophysics CenterLloyd KnoxUniv. of California, Davis, CA (United States)John C. MatherNASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)Suzanne T. StaggsPrinceton Univ., NJ (United States)N. B. SuntzeffTexas A & M Univ., College Station, TX (United States)
2006en
ABI

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.

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Citations and references

Cited by 60 references