Tuning the Cosmological Constant, Broken Scale Invariance, Unitarity
arXiv:1603.07101 · doi:10.1088/1475-7516/2016/06/028
Abstract
We study gravity coupled to a cosmological constant and a scale but not conformally invariant sector. In Minkowski vacuum, scale invariance is spontaneously broken. We consider small fluctuations around the Minkowski vacuum. At the linearised level we find that the trace of metric perturbations receives a positive or negative mass squared contribution. However, only for the Fierz-Pauli combination the theory is free of ghosts. The mass term for the trace of metric perturbations can be cancelled by explicitly breaking scale invariance. This reintroduces fine-tuning. Models based on four form field strength show similarities with explicit scale symmetry breaking due to quantisation conditions.
17 pages, v2: typo corrected and reference added, v3: references and comments added, estimate of ghost mass added, version accepted for publication
References in corpus (44)
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Dynamics of dark energy
- Resummation of Massive Gravity
- Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant
- Generalization of the Fierz-Pauli Action
- Modeling the fifth dimension with scalars and gravity
- Massive Gravity
- Theoretical Aspects of Massive Gravity
- Symmetries and Strings in Field Theory and Gravity
- Resolving the Ghost Problem in non-Linear Massive Gravity
- Effective Field Theory for Massive Gravitons and Gravity in Theory Space
- Confirmation of the Secondary Constraint and Absence of Ghost in Massive Gravity and Bimetric Gravity
- A Small Cosmological Constant from a Large Extra Dimension
- Self-tuning flat domain walls in 5d gravity and string theory
- The -theorem and the Asymptotics of 4D Quantum Field Theory
- General Properties of the Self-tuning Domain Wall Approach to the Cosmological Constant Problem
- TASI Lectures on the Cosmological Constant
- Sequestering the Standard Model Vacuum Energy
- Categorizing Different Approaches to the Cosmological Constant Problem
- Scale invariance, new inflation and decaying Lambda terms
- A Comment on Self-Tuning and Vanishing Cosmological Constant in the Brane World
- The Cosmological Constant and the String Landscape
- The Cosmological Constant Problem from a Brane-World Perspective
- Limit Cycles and Conformal Invariance
- Lectures on the Cosmological Constant Problem
- Self-tuning vacuum variable and cosmological constant
- On Scale and Conformal Invariance in Four Dimensions
- Vacuum Energy Sequestering: The Framework and Its Cosmological Consequences
- Model for self-tuning the cosmological constant
- Self-tuning solution of the cosmological constant problem with antisymmetric tensor field
- Scale Symmetry Breaking From Total Derivative Densities and the Cosmological Constant Problem
- Brane singularities and their avoidance
- The Big Constant Out, The Small Constant In
- Brane singularities with mixtures in the bulk
- Nontrival Cosmological Constant in Brane Worlds with Unorthodox Lagrangians
- More self-tuning solutions with
- Why trust a theory? Some further remarks (part 1)
- Metamorphosis of the Cosmological Constant and 5D Origin of the Fiducial Metric
- Vacuum energy sequestering and conformal symmetry
- Ghosts and Tachyons in the Fifth Dimension
- Dynamical Instability of Self-Tuning Solution with Antisymmetric Tensor Field
- Dual Description of Brane World Cosmological Constant with
- General self-tuning solutions and no-go theorem