Two new diagnostics of dark energy

Varun Sahni, Arman Shafieloo, and Alexei A. Starobinsky
Phys. Rev. D 78, 103502 – Published 3 November 2008

Abstract

We introduce two new diagnostics of dark energy (DE). The first, Om, is a combination of the Hubble parameter and the cosmological redshift and provides a null test of dark energy being a cosmological constant Λ. Namely, if the value of Om(z) is the same at different redshifts, then DEΛ, exactly. The slope of Om(z) can differentiate between different models of dark energy even if the value of the matter density is not accurately known. For DE with an unevolving equation of state, a positive slope of Om(z) is suggestive of phantom (w<1) while a negative slope indicates quintessence (w>1). The second diagnostic—acceleration probe q¯—is the mean value of the deceleration parameter over a small redshift range. It can be used to determine the cosmological redshift at which the universe began to accelerate, again without reference to the current value of the matter density. We apply the Om and q¯ diagnostics to the Union data set of type Ia supernovae combined with recent data from the cosmic microwave background (Wilkinson Microwave Anisotropy Probe 5) and baryon acoustic oscillations.

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  • Received 29 July 2008

DOI:https://doi.org/10.1103/PhysRevD.78.103502

©2008 American Physical Society

Authors & Affiliations

Varun Sahni1, Arman Shafieloo1, and Alexei A. Starobinsky2

  • 1Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, India
  • 2Landau Institute for Theoretical Physics, Kosygina 2, Moscow 119334, Russia

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Issue

Vol. 78, Iss. 10 — 15 November 2008

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