Pointer states for primordial fluctuations in inflationary cosmology
Open accessAbstract
Primordial fluctuations in inflationary cosmology acquire classical properties through decoherence when their wavelengths become larger than the Hubble scale. Although decoherence is effective, it is not complete, so a significant part of primordial correlations remains up to the present moment. We address the issue of the pointer states which provide a classical basis for the fluctuations with respect to the influence by an environment (other fields). Applying methods from the quantum theory of open systems (the Lindblad equation), we show that this basis is given by narrow Gaussians that approximate eigenstates of field amplitudes. We calculate both the von Neumann and linear entropy of the fluctuations. Their ratio to the maximal entropy per field mode defines a degree of partial decoherence in the entropy sense. We also determine the time of partial decoherence making the Wigner function positive everywhere which, for super-Hubble modes during inflation, is virtually independent of coupling to the environment and is only slightly larger than the Hubble time. On the other hand, assuming a representative environment (a photon bath), the decoherence time for sub-Hubble modes is finite only if some real dissipation exists.
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The entropy of the primordial fluctuations increases with increase in the scale factor a.
“The resulting entropy increases with increase in the scale factor a .”
From On a quantum Weyl curvature hypothesis (2022) · cites this paper as Kiefer et al. (2007)
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Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377253 · Cited by 4,860 · see citing works
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Bojowald, M. (2015) · Reports on Progress in Physics · doi:10.1088/0034-4885/78/2/023901 · Cited by 174 · see citing works
On a quantum Weyl curvature hypothesis
Kiefer, C. (2022) · AVS Quantum Science · doi:10.1116/5.0076811 · Cited by 10 · see citing works
“Detailed calculations of decoherence and entanglement for the primordial fluctuations can be found in Kiefer et al. (2007).”
BackgroundSelf-citation
- Authors
- Kiefer, C., Lohmar, I., Polarski, D., & Starobinsky, A. A.
- Affiliations
- University of Cologne (DE)
- Centre National de la Recherche Scientifique (FR)
- Landau Institute for Theoretical Physics (RU)
- Venue
- Classical and Quantum Gravity
- Publisher
- IOP Publishing
- Published
- 2007-03-13
- Volume
- 24
- Issue
- 7
- Pages
- 1699-1718
- ISSN
- 0264-9381 (ISSN-L)
- 1361-6382
- OpenAlex
- W2116905728
- Cited by
- 160
- References
- 1
- Citations by year
- 2026: 6 · 2025: 19 · 2024: 9 · 2023: 12 · 2022: 7 · 2021: 6 · 2020: 9 · 2019: 3 · 2018: 7 · 2017: 7 · 2016: 7 · 2015: 6 · 2014: 5 · 2013: 9 · 2012: 8
- FWCI
- 5.79
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Classical and Quantum Gravity (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- HAL (publishedVersion)
- arXiv (Cornell University)
- Funders
- Russian Foundation for Basic Research
- Centre Elile Borel, Institut Henri-Poincaré
- Institut Henri Poincaré
- Russian Academy of Sciences
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Quantum Mechanics and Applications
- Keywords
- primordial perturbations, inflation (cosmology), decoherence, pointer states, open quantum systems, Lindblad master equation, von Neumann entropy, linear entropy, Wigner function, energy dissipation, quantum-to-classical transition
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