On causality and superluminal behavior in classical field theories. Applications to k-essence theories and MOND-like theories of gravity
arXiv:gr-qc/0607055 · doi:10.1103/PhysRevD.75.085013
Abstract
Field theories whose full action is Lorentz invariant (or diffeomorphism invariant) can exhibit superluminal behaviors through the breaking of local Lorentz invariance. Quantum induced superluminal velocities are well-known examples of this effect. The issue of the causal behavior of such propagations is somewhat controversial in the literature and we intend to clarify it. We provide a careful analysis of the meaning of causality in classical relativistic field theories, and we stress the role played by the Cauchy problem and the notions of chronology and time arrow. We show that superluminal behavior threaten causality only if a prior chronology on spacetime is chosen. In the case where superluminal propagations occur, however, there is at least two non conformally related metrics on spacetime and thus two available notions of chronology. These two chronologies are on equal footing and it would thus be misleading to choose \textit{ab initio} one of them to define causality. Rather, we provide a formulation of causality in which no prior chronology is assumed. We argue this is the only way to deal with the issue of causality in the case where some degrees of freedom propagate faster than others. We actually show that superluminal propagations do not threaten causality. As an illustration of these conceptual issues, we consider two field theories, namely k-essences scalar fields and bimetric theories of gravity, and we derive the conditions imposed by causality. We discuss various applications such as the dark energy problem, MOND-like theories of gravity and varying speed of light theories.
15 pages, 2 figures; minor changes, references added, submitted to Phys.Rev.D
References in corpus (7)
- Dynamics of dark energy
- Causality, Analyticity and an IR Obstruction to UV Completion
- Can dark energy evolve to the Phantom?
- Correspondence between kinematical backreaction and scalar field cosmologies - the `morphon field'
- No-go theorem for k-essence dark energy
- Escaping from the black hole?
- Could the Pioneer anomaly have a gravitational origin?
Cited by in corpus (54)
- Beyond the Cosmological Standard Model
- Imperfect Dark Energy from Kinetic Gravity Braiding
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- The Tensor-Vector-Scalar theory and its cosmology
- Kinetic k-essence and Quintessence
- Causality and the speed of sound
- Stability and superluminality of spherical DBI galileon solutions
- Black holes in the presence of dark energy
- Time-dependent spherically symmetric covariant Galileons
- Vacuum structure for scalar cosmological perturbations in Modified Gravity Models
- DHOST Bounce
- Speedy sound and cosmic structure
- Pure kinetic k-essence as the cosmic speed-up
- TeVeS gets caught on caustics
- Potential-driven Galileon inflation
- Attractor scenarios and superluminal signals in k-essence cosmology
- Fab Four: When John and George play gravitation and cosmology
- Cosmological tachyon condensation
- -essence Gravity Inflation
- Information-Entropic for Travelling Solitons in Lorentz and CPT Breaking Systems
- Constraints on Kinetically Modified Inflation from WMAP5
- Galileon accretion
- Cuscuton gravity as a classically stable limiting curvature theory
- Emergent Universe and Genesis from the DHOST Cosmology
- Non-Gaussianity in single field models without slow-roll
- Caustics for Spherical Waves
- Constant-roll in the Palatini- models
- Phase-space analysis of a class of k-essence cosmology
- Thermodynamics of k-essence
- Constant-roll -Inflation Dynamics
- Slow-Roll Inflation at N3LO
- Suppressing Quantum Fluctuations in Classicalization
- Scalar mode propagation in modified gravity with a scalar field
- Disforming to Conformal Symmetry
- Stability and Quasinormal Modes of Black holes in Tensor-Vector-Scalar theory: Scalar Field Perturbations
- Dynamics of generalized tachyon field
- -Inflation-corrected Einstein-Gauss-Bonnet Gravity with Massless Primordial Gravitons
- New Dynamical Degrees of Freedom from Invertible Transformations
- Adiabatic regularisation of power spectra in -inflation
- Cosmology in 5D and 4D Einstein-Gauss-Bonnet gravity
- The Phantom of the New Oscillatory Cosmological Phase
- Solitons in generalized galileon theories
- Chaotic Inflation and Reheating in Generalized Scalar-Tensor Gravity
- Acausality in Superfluid Dark Matter and MOND-like Theories
- Three problems of superfluid dark matter and their solution
- Causal Modifications of Gravity and Their Observational Bounds
- Causality and Stability from Acoustic Geometry
- Potential-driven Inflation with Disformal Coupling to Gravity
- Two-body problem in theories with kinetic screening
- A Critique of Covariant Emergent Gravity
- The K-essence flow seen from the preferred frame . A scalar field theory with Landau superfluid structure
- A Bit Rate Bound on Superluminal Communication
- Non-parametric exploration of minimally coupled gravity with phantom crossing
- Kinetically-driven ekpyrosis