New class of exact coherent states: Enhanced quantization of motion on the half line
- 1. Institut des Sciences Moléculaires d'Orsay (ISMO), UMR 8214 CNRS, Université Paris-Saclay, 91405 Orsay Cedex, France
- 2. Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- 3. National Centre for Nuclear Research, Pasteura 7, 02-093 Warszawa, Poland
- 4. 𝒢ℝϵℂ𝒪—Institut d'Astrophysique de Paris, CNRS and Sorbonne Université, UMR 7095 98 bis boulevard Arago, 75014 Paris, France
Description
We have discovered a class of dynamically stable coherent states for motion on the half line. The regularization of the half line boundary and the consequent quantum motion are expounded within the framework of covariant affine quantization, although alternative approaches are also feasible. The former approach is rooted in affine coherent states and offers a consistent semiclassical representation of quantum motion. However, this method has been known to possess two shortcomings: (a) the dependence of affine coherent states on the choice of a vector, denoted as the "fiducial vector" (which remains unspecified), introduces significant arbitrariness in boundary regularization, and (b) regardless of the choice of fiducial vector, affine coherent states fail to evolve parametrically under the Schrödinger equation, thus limiting the accuracy of the semiclassical description. This limitation, in particular, hampers their suitability for approximating the evolution of compound observables. We demonstrate that a distinct and more refined definition of affine coherent states can simultaneously address both of these issues. In other words, these new affine coherent states exhibit parametric evolution only when the fiducial vector, denoted as , possesses a highly specific character, such as being an eigenstate of a well-defined Hamiltonian. Our discovery holds significant relevance in the field of quantum cosmology, particularly in scenarios where the positive variable is the scale factor of the universe, and its regularized motion plays a crucial role in avoiding the big-bang singularity.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.109.023516;
- arXiv
- arXiv:2310.16868;
- Crossref Funder ID
- 10.13039/501100004281;
Publishing Information
- Journal Title
- Physical Review D
- Journal Volume
- 109
- Journal Issue
- 2
- Journal Page Range
- 15 pgs.
- ISSN
- 1089-4918
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S97: MATHEMATICAL METHODS AND COMPUTING;
- Descriptors DEI
- ACCURACY; ANNIHILATION OPERATORS; COSMOLOGICAL MODELS; COSMOLOGY; EIGENFUNCTIONS; EQUATIONS OF MOTION; EVOLUTION; HAMILTONIANS; INTEGRABLE SYSTEMS; MOTION; QUANTIZATION; QUANTUM COSMOLOGY; SCHROEDINGER EQUATION; SEMICLASSICAL APPROXIMATION; SINGULARITY; UNIVERSE
- Descriptors DEC
- APPROXIMATIONS; CALCULATION METHODS; COSMOLOGY; DIFFERENTIAL EQUATIONS; DYNAMICAL SYSTEMS; EQUATIONS; FUNCTIONS; MATHEMATICAL MODELS; MATHEMATICAL OPERATORS; PARTIAL DIFFERENTIAL EQUATIONS; QUANTUM OPERATORS; WAVE EQUATIONS
Optional Information
- Copyright
- © 2024 American Physical Society
- Contract/Grant/Project number
- 2018/30/E/ST2/00370
- Notes
- Contact Email: herve.bergeron@universite-paris-saclay.fr; Contact Email: gazeau@apc.in2p3.fr; Contact Email: Przemyslaw.Malkiewicz@ncbj.gov.pl; Contact Email: patrick.peter@iap.fr; Record automatically processed
- Funding organization
- Narodowe Centrum Nauki