Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-05-18
Phys.Rev.Lett.87:141302,2001
Astronomy and Astrophysics
Astrophysics
5 pages, 3 figures, revtex4, submitted to PRL
Scientific paper
10.1103/PhysRevLett.87.141302
Dark energy models which alter the relative scaling behavior of dark energy and matter could provide a natural solution to the cosmic coincidence problem - why the densities of dark energy and dark matter are comparable today. A generalized class of dark energy models is introduced which allows non-canonical scaling of the ratio of dark matter and dark energy with the Robertson-Walker scale factor a(t). Upcoming observations, such as a high redshift supernova survey, application of the Alcock-Paczynski test to quasar pairs, and cluster evolution, will strongly constrain the relative scaling of dark matter and dark energy as well as the equation of state of the dark energy. Thus, whether there actually is a coincidence problem, and the extent of cosmic coincidence in the universe's recent past can be answered observationally in the near future. Determining whether today is a special time in the history of the universe will be a SNAP.
Abazajian Kevork
Dalal Neal
Jenkins Elizabeth
~Manohar Aneesh V.
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