Emergence of ghosts in Horndeski theory
arXiv:2001.11784 · doi:10.1007/JHEP07(2020)038
Abstract
We show that starting from initial conditions with stable perturbations, evolution of a galileon scalar field results in the appearance of a ghost later on. To demonstrate this, we consider a theory with k-essence and cubic galileon Lagrangians on a fixed Minkowski background. Explicit analytical solutions of simple waves are constructed, on top of which a healthy scalar degree of freedom is shown to be converted onto a ghost. Such a transformation is smooth and moreover perturbations remain hyperbolic all the time (until a caustic forms). We discuss a relation between the ghost and the appearance of closed causal curves for such solutions.
14 pages, 4 figures; v2: clarifications added, matches published version
References in corpus (5)
Cited by in corpus (8)
- No evidence of kinetic screening in simulations of merging binary neutron stars beyond general relativity
- Dynamics of Screening in Modified Gravity
- UV completions, fixing the equations and nonlinearities in -essence
- Gravitational Collapse in Cubic Horndeski Theories
- K-dynamics: well-posed 1+1 evolutions in K-essence
- Scalar-tensor cosmologies without screening
- Large black-hole scalar charges induced by cosmology in Horndeski theories
- Caustic formation in DBI models: Wave propagation on planar domain walls