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Gradient instability for w < -1

Stephen D. H. Hsu, Alejandro Jenkins, Mark B. Wise

Abstract

We show that in single scalar field models of the dark energy with equations of state satisfying $w \equiv p / ρ< -1$, the effective Lagrangian for fluctuations about the homogeneous background has a wrong sign spatial kinetic term. In most cases, spatial gradients are ruled out by microwave background observations. The sign of $w+1$ is not connected to the sign of the time derivative kinetic term in the effective Lagrangian.

Gradient instability for w < -1

Abstract

We show that in single scalar field models of the dark energy with equations of state satisfying , the effective Lagrangian for fluctuations about the homogeneous background has a wrong sign spatial kinetic term. In most cases, spatial gradients are ruled out by microwave background observations. The sign of is not connected to the sign of the time derivative kinetic term in the effective Lagrangian.

Paper Structure

This paper contains 16 equations, 1 figure.

Figures (1)

  • Figure 1: The effective couplings of two gravitons to several quanta of the scalar field. The shaded region represents interactions involving only scalars.