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Phys. Rev. Lett. 100, 241302 (2008) [4 pages]

Beyond Two Dark Energy Parameters

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Devdeep Sarkar1, Scott Sullivan1, Shahab Joudaki1, Alexandre Amblard1, Daniel E. Holz2,3, and Asantha Cooray1
1Department of Physics and Astronomy, University of California, Irvine, California 92697, USA
2Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
3Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA

Received 6 September 2007; revised 6 April 2008; published 19 June 2008

Our ignorance of dark energy is generally described by a two-parameter equation of state. In these approaches, a particular ad hoc functional form is assumed, and only two independent parameters are incorporated. We propose a model-independent, multiparameter approach to fitting dark energy and show that next-generation surveys will constrain the equation of state in three or more independent redshift bins to better than 10%. Future knowledge of dark energy will surpass two numbers (e.g., [w0,w1] or [w0,wa]), and we propose a more flexible approach to the analysis of present and future data.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.100.241302
DOI:
10.1103/PhysRevLett.100.241302
PACS:
95.36.+x, 98.62.Py, 98.80.Es