On the initial value problem for semiclassical gravity without and with quantum state collapses
arXiv:2205.11671 · doi:10.1088/1475-7516/2023/01/040
Abstract
We explore how the initial value problem may be formulated for globally hyperbolic, Hadamard, solutions of the semiclassical Einstein-Klein-Gordon equations. Given a set of data on an initial 3-surface, consisting of the values on the surface of a spacetime metric and its first 3 time derivatives off the surface, we introduce a notion of 'surface Hadamard' state on the CCR algebra of the surface. We conjecture that, for a given such set of classical Cauchy data with a surface Hadamard state satisfying the semiclassical constraint equations, the initial value problem will be well posed. We present similar conjectures for a semiclassical scalars model and semiclassical electrodynamics. Moreover, partly inspired by work of Parker and Simon in 1993, we define semiclassical gravity `physical solutions' to be those that are (jointly smooth) functions of and of coordinates continuous in at . We conjecture that for such solutions the second and third time derivatives of the metric off the surface need not be specified, but rather will be determined by that continuity condition. Assuming the initial value conjecture for such physical solutions holds, and that a stochastic rule were available which leads to quantum state collapses occurring on (non-intersecting) random Cauchy surfaces, we discuss the well-posedness of semiclassical gravity with stochastic quantum state collapses. We also discuss two notions of approximate physical semiclassical solutions (both with and without collapses): Namely solutions to order (first discussed by Parker and Simon in 1993) and solutions to order . We point out that the latter do not require higher derivative terms or Hadamard subtractions, but that nevertheless order semiclassical gravity is a distinct theory from classical general relativity capable of incorporating quantum interference phenomena.
arXiv comment47 pages. Corrections implemented, notably Def 11 (preliminary surface Hadamard condition) and certain equations on p. 33. Explanations improved and typos fixed. This version corresponds largely to the published version in JCAP
References in corpus (61)
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Dynamical Reduction Models
- The generally covariant locality principle -- A new paradigm for local quantum physics
- Does backreaction enforce the averaged null energy condition in semiclassical gravity?
- Local Wick Polynomials and Time Ordered Products of Quantum Fields in Curved Spacetime
- Averaged Energy Conditions and Quantum Inequalities
- Existence of Local Covariant Time Ordered Products of Quantum Fields in Curved Spacetime
- Is Quantum Gravity Necessary?
- Semiclassical Gravity Theory and Quantum Fluctuations
- Einstein Equation with Quantum Corrections Reduced to Second Order
- Quantum Field Theory Constrains Traversable Wormhole Geometries
- Relativistic state reduction dynamics
- Conservation of the stress tensor in perturbative interacting quantum field theory in curved spacetimes
- Hadamard renormalization of the stress-energy tensor for a quantized scalar field in a general spacetime of arbitrary dimension
- A general worldline quantum inequality
- Can Bohmian mechanics be made relativistic?
- Lectures on the Cosmological Constant Problem
- Quantum Instability of the Cauchy Horizon in Reissner-Nordström-deSitter Spacetime
- Quantum Field Theory on Spacetimes with a Compactly Generated Cauchy Horizon
- Evaporation of Two Dimensional Black Holes
- Measurement Analysis and Quantum Gravity
- Algebraic QFT in Curved Spacetime and quasifree Hadamard states: an introduction
- Quantum effects in the Alcubierre warp drive spacetime
- A Relativistic Dynamical Collapse Model
- The Necessity of the Hadamard Condition
- Stable cosmological models driven by a free quantum scalar field
- The BTZ black hole violates strong cosmic censorship
- Singularity theorems from weakened energy conditions
- Towards a formal description of the collapse approach to the inflationary origin of the seeds of cosmic structure
- On the initial conditions and solutions of the semiclassical Einstein equations in a cosmological scenario
- Quantum stress tensor at the Cauchy horizon of Reissner-Nordström-deSitter spacetime
- Lectures on quantum energy inequalities
- Semiclassical instability of dynamical warp drives
- Quantum Inequalities and Singular Energy Densities
- Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities
- Simple Refutation of the Eppley-Hannah argument
- Strong cosmic censorship in the BTZ black hole
- Quantum-corrected black holes and naked singularities in (2+1)-dimensions
- Global Existence of Solutions of the Semiclassical Einstein Equation for Cosmological Spacetimes
- Higher Derivative Scalar Quantum Field Theory in Curved Spacetime
- Quantum strong energy inequalities
- Semiclassical theories as initial value problems
- Semi-classical gravity in de Sitter spacetime and the cosmological constant
- Generally covariant dynamical reduction models and the Hadamard condition
- Stress-Energy Must be Singular on the Misner Space Horizon even for Automorphic Fields
- Dynamical Backreaction in Robertson-Walker Spacetime
- Static symmetric solutions of the semi-classical Einstein-Klein-Gordon system
- Constraining quantum collapse inflationary models with current data: The semiclassical approach
- Spacetime in Semiclassical Gravity
- Hadamard renormalization for a charged scalar field
- The thermal and two-particle stress-energy must be ill-defined on the 2-d Misner space chronology horizon
- Semiclassical Self Consistent Treatment of the Emergence of Seeds of Cosmic Structure. The second order construction
- Evaporation of four-dimensional dynamical black holes sourced by the quantum trace anomaly
- Towards a novel approach to semi-classical gravity
- Special cosmological models derived from the semiclassical Einstein equation on flat FLRW space-times
- Scale-Invariant Curvature Fluctuations from an Extended Semiclassical Gravity
- Semiclassical gravity with a conformally covariant field in globally hyperbolic spacetimes
- Linear stability of semiclassical theories of gravity
- Hadamard states on spherically symmetric characteristic surfaces, the semi-classical Einstein equations and the Hawking effect
- Can a particle detector cross a Cauchy horizon?
- Collapse of the wavefunction, the information paradox and backreaction
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