The Effective Theory of Gravity and Dynamical Vacuum Energy
arXiv:2205.04703 · doi:10.1007/JHEP11(2022)037
Abstract
Gravity and general relativity are considered as an Effective Field Theory at low energies and macroscopic distances. The effective action of the conformal anomaly of light or massless quantum fields has significant effects on macroscopic scales, due to associated light cone singularities that are not captured by an expansion in local curvature invariants. A compact local form for the WZ effective action of the conformal anomaly and stress tensor is given, requiring the introduction of a new light scalar field, which it is argued should be included in the low energy effective action for gravity. The scalar conformalon couples to the conformal part of the spacetime metric and allows the effective value of the vacuum energy, described as a condensate of a 4-form abelian gauge field strength F=dA, to change in space and time. This is achieved by the identification of the torsion dependent part of the Chern-Simons 3-form of the Euler class with the gauge potential A, which enters the effective action of the conformal anomaly as a J.A interaction analogous to electromagnetism. The conserved 3-current J describes the worldtube of 2-surfaces that separate regions of differing vacuum energy. The resulting EFT thus replaces the fixed constant Lambda of classical gravity, and its apparently unnaturally large sensitivity to UV physics, with a dynamical condensate whose ground state value in empty flat space is Lambda = 0 identically. By allowing Lambda to vary rapidly near the 2-surface of a black hole horizon, the proposed EFT of dynamical vacuum energy provides an effective Lagrangian for gravitational condensate stars, as the final state of complete gravitational collapse consistent with quantum theory. The possible consequences of dynamical vacuum dark energy for cosmology, the cosmic coincidence problem, and the role of conformal invariance for other fine tuning issues in the SM are discussed.
arXiv comment41 pages, Revised Version published in JHEP 2022, 37 (2022). Previous Sec. 2 expanded to Secs. 2-3. The role of the torsional part of the Chern-Simons 3-form and source current for the 4-form field strength clarified in Secs. 5-7. Previous Sec. 5 moved to Appendix B and modified to discuss torsional susceptibility kappa. Previous Sec. 6 eliminated as unnecessary. Conclusions are unchanged
References in corpus (45)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Confrontation between General Relativity and Experiment
- Black Holes: Complementarity or Firewalls?
- General relativity as an effective field theory: The leading quantum corrections
- The information paradox: A pedagogical introduction
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Gravitational Vacuum Condensate Stars
- Quantum Gravity in Everyday Life: General Relativity as an Effective Field Theory
- Physical Aspects of the Space-Time Torsion
- Jerusalem Lectures on Black Holes and Quantum Information
- On the Foundations of Chiral Perturbation Theory
- A Quartic Conformally Covariant Differential Operator for Arbitrary Pseudo-Riemannian Manifolds (Summary)
- De Sitter Space and Eternity
- Introduction to Effective Field Theory
- First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters
- Weyl Cohomology and the Effective Action for Conformal Anomalies
- Black Hole Evaporation in the Presence of a Short Distance Cutoff
- The effective field theory treatment of quantum gravity
- Surface Tension and Negative Pressure Interior of a Non-Singular `Black Hole'
- Cosmological Dark Energy: Prospects for a Dynamical Theory
- Effective Action, Conformal Anomaly and the Issue of Quadratic Divergences
- Conformal Symmetry and Central Charges in 4 Dimensions
- On the Instability of Global de Sitter Space to Particle Creation
- The Trace Anomaly and Massless Scalar Degrees of Freedom in Gravity
- Macroscopic Effects of the Quantum Trace Anomaly
- The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
- Renormalised 3-point functions of stress tensors and conserved currents in CFT
- Quantum Vacuum Instability of 'Eternal' de Sitter Space
- Cosmology and the Standard Model
- Linear Response, Validity of Semi-Classical Gravity, and the Stability of Flat Space
- Physical States of the Quantum Conformal Factor
- Some more remarks on the Witten-Veneziano formula for the mass
- TTT in CFT: Trace Identities and the Conformal Anomaly Effective Action
- Cosmological Horizon Modes and Linear Response in de Sitter Spacetime
- The cosmological constant as a manifestation of the conformal anomaly?
- Decay of the de Sitter Vacuum
- Anomaly Poles as Common Signatures of Chiral and Conformal Anomalies
- Structure of Lanczos-Lovelock Lagrangians in Critical Dimensions
- Towards a solution of the cosmological constant problem
- Slowly rotating gravastars
- Asymptotic Scale Invariance and its Consequences
- Condition for directly testing scalar modes of gravitational waves by four detectors
- Surface Stress Tensor and Junction Conditions on a Rotating Null Horizon
- Fermion Pairing and the Scalar Boson of the 2D Conformal Anomaly
Cited by in corpus (13)
- Gravitational Condensate Stars: An Alternative to Black Holes
- Possible Causes of False General Relativity Violations in Gravitational Wave Observations
- Running vacuum in QFT in FLRW spacetime: The dynamics of from the quantized matter fields
- Gravitational Vacuum Condensate Stars
- Rotating black holes in semiclassical gravity
- Regular Black Holes and Horizonless Ultra-Compact Objects in Lorentz-Violating Gravity
- Notes on conformal anomaly, nonlocal effective action and the metamorphosis of the running scale
- Quantum Effects of the Conformal Anomaly in a 2D Model of Gravitational Collapse
- Effective approach to the Antoniadis-Mottola model: quantum decoupling of the higher derivative terms
- Embedding Unimodular Gravity in String Theory
- Overspinning a rotating black hole in semiclassical gravity with type-A trace anomaly
- Trace anomaly contributions to semi-classical wormhole geometries
- Macroscopic backreaction of the trace anomaly on classical vacuum backgrounds