Quantum geometric information flows and relativistic generalizations of G. Perelman thermodynamics for nonholonomic Einstein systems with black holes and stationary solitonic hierarchies
arXiv:1907.03541 · doi:10.1007/s11128-021-03287-7
Abstract
We investigate classical and quantum geometric information flow theories (respectively, GIFs and QGIFs) when the geometric flow evolution and field equations for nonholonomic Einstein systems, NES, are derived from Perelman-Lyapunov type entropic type functionals. In this work, the term NES encodes models of gravitational and matter fields interactions and their geometric flow evolution subjected to nonholonomic (equivalently, non-integrable, anholonomic) constraints. There are used canonical geometric variables which allow a general decoupling and integration of systems of nonlinear partial differential equations describing GIFs and QGIFs and (for self-similar geometric flows) Ricci soliton type configurations. Our approach is different from the methods and constructions elaborated for special classes of solutions characterized by area--hypersurface entropy, related holographic and dual gauge--gravity models, and conformal field theories, involving generalizations of the Bekenstein-Hawking entropy and black hole thermodynamics. We formulate the theory of QGIFs which in certain quasi-classical limits encodes GIFs and models with flow evolution of NES. There are analysed the most important properties (inequalities) for NES and defined and computed QGIF versions of the von Neumann, relative and conditional entropy; mutual information, (modified) entanglement and Rényi entropy. We construct explicit examples of generic off-diagonal exact and parametric solutions describing stationary solitonic gravitational hierarchies and deformations of black hole configurations. Finally, we show how Perelman's entropy and geometric thermodynamic values, and extensions to GIF and QGIF models can be computed for various new classes of exact solutions which cannot be described following the Bekenstein-Hawking approach.
latex2e 11pt, 51 pages, v5 with minor modifications for the title and some references corresponding to the published version
References in corpus (13)
- Towards a derivation of holographic entanglement entropy
- Deformation Quantization of Almost Kahler Models and Lagrange-Finsler Spaces
- Nonholonomic Ricci Flows, Exact Solutions in Gravity, and Symmetric and Nonsymmetric Metrics
- Curve Flows in Lagrange-Finsler Geometry, Bi-Hamiltonian Structures and Solitons
- Ricci Flows and Solitonic pp--Waves
- Fractional Curve Flows and Solitonic Hierarchies in Gravity and Geometric Mechanics
- Heterotic Supergravity with Internal Almost-Kähler Spaces, Instantons for , or , Gauge Groups, and Deformed Black Holes with Soliton, Quasiperiodic and/or Pattern-forming Structures
- Geometric information flows and G. Perelman entropy for relativistic classical and quantum mechanical systems
- Classical and quantum geometric information flows and entanglement of relativistic mechanical systems
- Entropy functionals and thermodynamics of relativistic geometric flows, stationary quasi-periodic Ricci solitons, and gravity
- Nonassociative black ellipsoids distorted by R-fluxes and four dimensional thin locally anisotropic accretion disks
- Kaluza--Klein gravity & cosmology emerging from G. Perelman's entropy functionals and quantum geometric information flows
- Off-diagonal cosmological solutions in emergent gravity theories and Grigory Perelman entropy for geometric flows
Cited by in corpus (5)
- Geometric Flow of Bubbles
- Dark energy and dark matter configurations for wormholes and solitionic hierarchies of nonmetric Ricci flows and gravity
- Nonassociative Ricci flows, star product and R-flux deformed black holes, and swampland conjectures
- Local Conformal Instability and Local Non-Collapsing in the Ricci flow of Quantum Spacetime
- The Anholonomic Frame and Connection Deformation Method for constructing off-diagonal solutions in (modified) Einstein gravity and nonassociative geometric flows and Finsler-Lagrange-Hamilton theories