The quadratic approximation for quintessence with arbitrary initial conditions

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Vanderbilt University. Department of Physics and Astronomy

Abstract

We examine models of quintessence in which a minimally-coupled scalar field phi evolves near a local extremum of its potential V ( phi) at phi_. Assuming that (1/V )(dV/dphi) is small and w ~ -1, we Taylor expand the potential about phi_ and derive a general expression for w(a). The dynamics of this field are determined by the initial and final equation of state parameters w_i and w_0, the quantity V''( phi_)/V(phi_), and the direction of \dot\phi_i in relation to \dot\phi 0. This approximation is then tested for six values of V''( phi)/V(phi_) and shown to lie within 2% of the exact solution for five of these cases. However, the model becomes less precise near certain values of V''( phi_)/V(phi_) where \dot\phi becomes very large.

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Dark energy, Quintessence, w(a)

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Except where otherwised noted, this item's license is described as CC0 1.0 Universal