Formation of caustics in k-essence and Horndeski theory
arXiv:1602.00735 · doi:10.1007/JHEP04(2016)129
Abstract
We study propagation of waves and appearance of caustics in k-essence and galileon theories. First we show that previously known solutions for travelling waves in k-essence and galileon models correspond to very specific fine-tuned initial conditions. On the contrary, as we demonstrate by the method of characteristics, generic initial conditions leads to a wave in k-essence which ends up with formation of caustics. Finally, we find that any wave solution in pure k-essence is also a solution for a galileon theory with the same k-essence term. Thus in the Horndeski theory with a k-essence term formation of caustics is generic. We discuss physical consequences of the caustics formation and possible ways to cure the problem.
17 pages, 3 figures, v3: References added, appendix added with a tentative approach to resolve the caustic problem; v4: typos corrected, matches published version
References in corpus (17)
- Covariant Galileon
- Healthy theories beyond Horndeski
- Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensors
- Avoiding Dark Energy with 1/R Modifications of Gravity
- Exploring gravitational theories beyond Horndeski
- Cosmology with Mimetic Matter
- Unifying framework for scalar-tensor theories of gravity
- Global topological k-defects
- On causality and superluminal behavior in classical field theories. Applications to k-essence theories and MOND-like theories of gravity
- Hamiltonian analysis of spatially covariant gravity
- Gauge k-vortices
- Escaping from the black hole?
- Hamiltonian structure of scalar-tensor theories beyond Horndeski
- On the quasi-linearity of the Einstein- "Gauss-Bonnet" gravity field equations
- Many Faces of Mimetic Gravity
- Formation of caustics in Dirac-Born-Infeld type scalar field systems
- Plane waves in the generalized Galileon theory
Cited by in corpus (36)
- Black holes and stars in Horndeski theory
- Covariant Horava-like and mimetic Horndeski gravity: cosmological solutions and perturbations
- Recovering a MOND-like acceleration law in mimetic gravity
- Black holes in a cubic Galileon universe
- Living with ghosts in Horava-Lifshitz gravity
- Healthy imperfect dark matter from effective theory of mimetic cosmological perturbations
- Dynamics of Screening in Modified Gravity
- Caustics for Spherical Waves
- Recovering P(X) from a canonical complex field
- UV completions, fixing the equations and nonlinearities in -essence
- Gravitational Collapse in Cubic Horndeski Theories
- Spacetime and dark matter from spontaneous breaking of Lorentz symmetry
- Gravitational focusing of Imperfect Dark Matter
- Plebanski-Demianski solutions in Quadratic gravity with conformally coupled scalar fields
- K-dynamics: well-posed 1+1 evolutions in K-essence
- Is the DBI scalar field as fragile as other -essence fields?
- Raychaudhuri equation in -essence geometry: conditional singular and non-singular cosmological models
- Field Theories and Fluids for an Interacting Dark Sector
- Inflation and late-time accelerated expansion driven by -essence degenerate dynamics
- Cosmological constraints on a unified dark matter-energy scalar field model with fast transition
- The Phantom of the New Oscillatory Cosmological Phase
- Some disquisitions on cosmological 2-form dualities
- Critical collapse in K-essence models
- Generalized unimodular gravity as a form of k-essence
- K-essence in Horndeski models
- Emergence of ghosts in Horndeski theory
- A new nonlinear instability for scalar fields
- Two-body problem in theories with kinetic screening
- Instabilities Appearing in Cosmological Effective Field theories: When and How?
- Caustic Formation upon Shift Symmetry Breaking
- Dynamical dimensional reduction in multi-valued Hamiltonians
- A new instability in clustering dark energy?
- Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
- Caustic formation in DBI models: Wave propagation on planar domain walls
- Positivity vs. Lorentz-violation: an explicit example
- Cherenkov radiation as ghost instability