Jeans' Ghost
arXiv:1606.00618 · doi:10.1103/PhysRevD.94.064001
Abstract
We show that a massless canonical scalar field minimally coupled to general relativity can become a tachyonic ghost at low energies around a background in which the scalar's gradient is spacelike. By performing a canonical transformation we demonstrate that this low energy ghost can be recast, at the level of the action, in a form of a fluid that undergoes a Jeans-like instability affecting only modes with large wavelength. This illustrates that low-energy tachyonic ghosts do not lead to a catastrophic quantum vacuum instability, unlike the usual high-energy ghost degrees of freedom.
7 pages
Cited by in corpus (44)
- A new relativistic theory for Modified Newtonian Dynamics
- The Viability of Phantom Dark Energy: A Brief Review
- Cosmological parameter constraints for Horndeski scalar-tensor gravity
- Instabilities in Mimetic Matter Perturbations
- Higher Derivative Mimetic Gravity
- A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
- Stable solutions of inflation driven by vector fields
- Novel matter coupling in general relativity via canonical transformation
- Anisotropic cosmological reconstruction in gravity
- Built-in scordatura in U-DHOST
- Hamiltonian analysis of mimetic scalar gravity revisited
- Bouncing Models in an Extended Gravity Theory
- Phantom cosmology in an Extended Theory of Gravity
- Stability of scalar perturbations in scalar-torsion gravity theories in the presence of a matter fluid
- COSMOS-- soft Higgsotic attractors
- On the stability conditions for theories of modified gravity in presence of matter fields
- Gauge Field Mimetic Cosmology
- Two-field disformal transformation and mimetic cosmology
- The role of the tachyonic instability in Horndeski gravity
- Stealth dark energy in scordatura DHOST theory
- Aether scalar tensor theory: Linear stability on Minkowski space
- Cosmological Perturbation Theory in Metric-Affine Gravity
- Stealth magnetic field in de Sitter spacetime
- Cosmology and gravitational waves in consistent Einstein-Gauss-Bonnet gravity
- Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity
- Anisotropic Mimetic Cosmology
- Mimetic Inflation
- Extending applicability of bimetric theory: chameleon bigravity
- Generalized Brans-Dicke theories in light of evolving dark energy
- Stable cosmology in chameleon bigravity
- Role of matter in extended quasidilaton massive gravity
- Conformally and Disformally Coupled Vector field Models of Dark Energy
- Cosmological Instabilities and the Role of Matter Interactions in Dynamical Dark Energy Models
- Avoiding instabilities in antisymmetric tensor field driven inflation
- Aether scalar tensor theory: Hamiltonian Formalism
- Multi-field Mimetic Gravity
- On tachyonic stability priors for dark energy
- Big Bang Nucleosynthesis constraints on the cosmological evolution in a Universe with a Weylian Boundary
- Revisiting linear stability of black hole odd-parity perturbations in Einstein-Aether gravity
- A de Sitter limit analysis for dark energy and modified gravity models
- Stability of stealth magnetic field in de Sitter spacetime
- The Ogievetsky-Polubarinov massive gravity and the benign Boulware-Deser mode
- Scalar and vector modes in inflation with antisymmetric tensor field
- Positivity vs. Lorentz-violation: an explicit example