Quantum initial conditions for inflation and canonical invariance
arXiv:2002.07042 · doi:10.1103/PhysRevD.102.023507
Abstract
We investigate the transformation of initial conditions for primordial curvature perturbations under two types of transformations of the associated action: simultaneous redefinition of time and the field to be quantised, and the addition of surface terms. The latter encompasses all canonical transformations, whilst the time- and field-redefinition is a distinct, non-canonical transformation since the initial and destination systems use different times. Actions related to each other via such transformations yield identical equations of motion and preserve the commutator structure. They further preserve the time-evolution of expectation values of quantum operators unless the vacuum state also changes under the transformation. These properties suggest that it is of interest to investigate vacuum prescriptions that also remain unchanged under canonical transformations. We find that initial conditions derived via minimising the vacuum expectation value of the Hamiltonian and those obtained using the Danielsson vacuum prescription are not invariant under these transformations, whereas those obtained by minimising the local energy density are. We derive the range of physically distinct initial conditions obtainable by Hamiltonian diagonalisation, and illustrate their effect on the scalar primordial power spectrum and the Cosmic Microwave Background under the just enough inflation model. We also generalise the analogy between the dynamics of a quantum scalar field on a curved, time-dependent spacetime and the gauge-invariant curvature perturbation. We argue that the invariance of the vacuum prescription obtained by minimising the renormalised stress--energy tensor should make it the preferred procedure for setting initial conditions for primordial perturbations. All other procedures reviewed in this work yield ambiguous initial conditions, which is problematic both in theory and practice.
arXiv commentRevisions after review added. 17 pages, 8 figures. Accepted to PRD
References in corpus (41)
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Planck 2018 results. V. CMB power spectra and likelihoods
- The Trans-Planckian Problem of Inflationary Cosmology
- The Cold Dark Matter Density Perturbation
- Semiclassicality and Decoherence of Cosmological Perturbations
- How long before the end of inflation were observable perturbations produced?
- PolyChord: nested sampling for cosmology
- The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
- PolyChord: next-generation nested sampling
- A note on inflation and transplanckian physics
- The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics
- TASI Lectures on Inflation
- A generic estimate of trans-Planckian modifications to the primordial power spectrum in inflation
- On the Dependence of the Spectra of Fluctuations in Inflationary Cosmology on Trans-Planckian Physics
- A Horizon Ratio Bound for Inflationary Fluctuations
- Cosmological Perturbations from a New-Physics Hypersurface
- WMAP data and the curvature of space
- A note on alpha-vacua and interacting field theory in de Sitter space
- Closed Universes, de Sitter Space and Inflation
- Hamilton's approach in cosmological inflation with an exponential potential and its observational constraints
- TASI Lectures on Inflation
- The Coherent State Representation of Quantum Fluctuations in the Early Universe
- Kinetic Initial Conditions for Inflation
- Vacuum Choices and the Predictions of Inflation
- Trans-Planckian footprints in inflationary cosmology
- Primordial power spectra for curved inflating universes
- Canonical transformations and squeezing formalism in cosmology
- Predictions of just-enough inflation
- Bayesian inflationary reconstructions from Planck 2018 data
- Low power on large scales in just enough inflation models
- Inflation in the closed FLRW model and the CMB
- Minimal Theoretical Uncertainties in Inflationary Predictions
- Novel quantum initial conditions for inflation
- Constraining the kinetically dominated Universe
- An efficient method for solving highly oscillatory ordinary differential equations with applications to physical systems
- Dynamics of Inflationary Universes with Positive Spatial Curvature
- Optimal polarisation equations in FLRW universes
- A case for kinetically dominated initial conditions for inflation
- Causality in Inflationary Universes with Positive Spatial Curvature
- Which part of the stress-energy tensor gravitates?
Cited by in corpus (7)
- Constraining Quantum Initial Conditions before Inflation
- Rapid numerical solutions for the Mukhanov-Sasaki equation
- Quantum initial conditions for curved inflating universes
- New formalism to define vacuum states for scalar fields in curved space-times
- Inclusive probability of particle creation on classical backgrounds
- Quantum Fisher information of a cosmic qubit undergoing non-Markovian de Sitter evolution
- Finite inflation in curved space