Four-mode squeezed states: two-field quantum systems and the symplectic group
arXiv:2104.14942 · doi:10.1140/epjc/s10052-021-09922-y
Abstract
We construct the four-mode squeezed states and study their physical properties. These states describe two linearly-coupled quantum scalar fields, which makes them physically relevant in various contexts such as cosmology. They are shown to generalise the usual two-mode squeezed states of single-field systems, with additional transfers of quanta between the fields. To build them in the Fock space, we use the symplectic structure of the phase space. For this reason, we first present a pedagogical analysis of the symplectic group and its Lie algebra, from which we construct the four-mode squeezed states and discuss their structure. We also study the reduced single-field system obtained by tracing out one of the two fields. This procedure being easier in the phase space, it motivates the use of the Wigner function which we introduce as an alternative description of the state. It allows us to discuss environmental effects in the case of linear interactions. In particular, we find that there is always a range of interaction coupling for which decoherence occurs without substantially affecting the power spectra (hence the observables) of the system.
arXiv comment38 pages without appendices (total 49 pages), matches published version in EPJC
References in corpus (27)
- Area laws for the entanglement entropy - a review
- Towards Inflation in String Theory
- Semiclassicality and Decoherence of Cosmological Perturbations
- Squeezed states of light and their applications in laser interferometers
- The Real Symplectic Groups in Quantum Mechanics and Optics
- Inflation and squeezed quantum states
- Symplectic invariants, entropic measures and correlations of Gaussian states
- Quantum-to-classical transition for fluctuations in the early Universe
- Quantum-to-classical Transition of Cosmological Perturbations for Non-vacuum Initial States
- String Theory and Inflation
- Quantum Discord of Cosmic Inflation: Can we Show that CMB Anisotropies are of Quantum-Mechanical Origin?
- Inflation and String Theory
- Inflationary Perturbations: the Cosmological Schwinger Effect
- Squeezed States in the de Sitter Vacuum
- Obstructions to Bell CMB Experiments
- Observational constraints on quantum decoherence during inflation
- Chasing Brane Inflation in String-Theory
- Canonical transformations and squeezing formalism in cosmology
- Bell's Inequalities for Continuous-Variable Systems in Generic Squeezed States
- Non Gaussianities from Quantum Decoherence during Inflation
- Quantum entanglement in de Sitter space from Stringy Axion: An analysis using vacua
- Leggett-Garg Inequalities for Squeezed States
- Bipartite temporal Bell inequalities for two-mode squeezed states
- Two-mode squeezed states as Schrodinger-cat-like states
- Wigner function for SU(1,1)
- Squeezing for Bloch Four-Hyperboloid via The Non-Compact Hopf Map
- The symplectic group in Polymer Quantum Mechanics
Cited by in corpus (19)
- Minimal decoherence from inflation
- Discord and Decoherence
- Benchmarking the cosmological master equations
- The Open Effective Field Theory of Inflation
- Hamiltonian formalism for cosmological perturbations: the separate-universe approach
- Decoherence out of fire: Purity loss in expanding and contracting universes
- Comparing quantumness criteria
- The Early Universe as an Open Quantum System: Complexity and Decoherence
- Real-space Bell inequalities in de Sitter
- Entanglement and Expansion
- In-in formalism for the entropy of quantum fields in curved spacetimes
- Entanglement in Cosmology
- Density matrix formalism for interacting quantum fields
- Entanglement masquerading in the CMB
- Quantum Echo in Two-Component Bose-Einstein Condensates
- The Quantum Dynamics of Two-component Bose-Einstein Condensate: an Symmetry Approach
- Classical and Quantum Dynamics of Gyroscopic Systems and Dark Energy
- Probing the self-coherence of primordial quantum fluctuations with complexity
- Understanding Squeezed States of Light Through Wigner's Phase-Space