Apparent ghosts and spurious degrees of freedom in non-local theories
arXiv:1311.3421 · doi:10.1016/j.physletb.2014.04.024
Abstract
Recent work has shown that non-local modifications of the Einstein equations can have interesting cosmological consequences and can provide a dynamical origin for dark energy, consistent with existing data. At first sight these theories are plagued by ghosts. We show that these apparent ghost-like instabilities do not describe actual propagating degrees of freedom, and there is no issue of ghost-induced quantum vacuum decay.
18 pages, 3 figures. v2: cross-reference to 1311.3435 added
References in corpus (14)
- Resummation of Massive Gravity
- Avoiding Dark Energy with 1/R Modifications of Gravity
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- Degravitation of the Cosmological Constant and Graviton Width
- Non-Local Modification of Gravity and the Cosmological Constant Problem
- Dynamics of Nonlocal Cosmology
- Accelerating cosmologies from non-local higher-derivative gravity
- Phantom and non-phantom dark energy: The cosmological relevance of non-locally corrected gravity
- Predictive Power of Strong Coupling in Theories with Large Distance Modified Gravity
- Newtonian limit of nonlocal cosmology
- A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
- Inflation in (Super-)renormalizable Gravity
- Fading Gravity and Self-Inflation
- Reconstruction Procedure in Nonlocal Cosmological Models
Cited by in corpus (44)
- Massive Gravity
- Beyond CDM: Problems, solutions, and the road ahead
- Super-renormalizable & Finite Gravitational Theories
- Cosmological perturbations and structure formation in nonlocal infrared modifications of general relativity
- Non-local gravity and dark energy
- Nonlocal gravity. Conceptual aspects and cosmological predictions
- Super-renormalizable or Finite Lee-Wick Quantum Gravity
- Nonlocal Models of Cosmic Acceleration
- Weak lensing by voids in modified lensing potentials
- Universally Finite Gravitational & Gauge Theories
- Nonlocal quantum gravity and M-theory
- Non-local gravity and comparison with observational datasets
- Nonlinear structure formation in Nonlocal Gravity
- Cosmological dynamics and dark energy from non-local infrared modifications of gravity
- Changing the prior: absolute neutrino mass constraints in nonlocal gravity
- Spherically symmetric static solutions in a non-local infrared modification of General Relativity
- Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with CDM
- Testing nonlocal gravity with Lunar Laser Ranging
- Field equations and cosmology for a class of nonlocal metric models of MOND
- Perturbative loop corrections and nonlocal gravity
- Gravity in the infrared and effective nonlocal models
- Cosmological perturbations and observational constraints on nonlocal massive gravity
- Galaxy cluster lensing masses in modified lensing potentials
- Dynamical analysis of cosmology: Impact of initial conditions and constraints from supernovae
- Non-local gravity with a Weyl-square term
- Acausality in Nonlocal Gravity Theory
- Nonlocal Metric Realizations of MOND
- Stability analysis and future singularity of the model of non-local gravity
- Revival of the Deser-Woodard nonlocal gravity model: Comparison of the original nonlocal form and a localized formulation
- A Caveat on Building Nonlocal Models of Cosmology
- Conformal symmetry and nonlinear extensions of nonlocal gravity
- Non-local formulation of ghost-free bigravity theory
- Removing Ostrogradski ghost from degenerate gravity theories
- On nonlocally interacting metrics, and a simple proposal for cosmic acceleration
- Growth of perturbations in nonlocal gravity with non-CDM background
- Noether symmetry in a nonlocal f(T) Gravity
- Ghosts in classes of non-local gravity
- Dark energy and dimensional transmutation in gravity
- Hamiltonian Formalism for Nonlocal Gravity Models
- Classical and Quantum Nonlocal Supergravity
- Cosmological evolution of generalized non-local gravity
- An Improved Cosmological Model
- The Case for Nonlocal Modifications of Gravity
- Stability issues of nonlocal gravity during primordial inflation