Results 31 to 40 of about 156,624 (168)

Dynamical Signature: Complex Manifolds, Gauge Fields and Non-Flat Tangent Space

open access: yesUniverse, 2022
Theoretical possibilities of models of gravity with dynamical signature are discussed. The different scenarios of the signature change are proposed in the framework of Einstein-Cartan gravity.
Sergey Bondarenko
doaj   +1 more source

Ricci soliton and Ricci almost soliton within the framework of Kenmotsu manifold

open access: yesKarpatsʹkì Matematičnì Publìkacìï, 2019
First, we prove that if the Reeb vector field $\xi$ of a Kenmotsu manifold $M$ leaves the Ricci operator $Q$ invariant, then $M$ is Einstein. Next, we study Kenmotsu manifold whose metric represents a Ricci soliton and prove that it is expanding ...
A. Ghosh
doaj   +1 more source

Projective compactifications and Einstein metrics [PDF]

open access: yesJournal für die reine und angewandte Mathematik (Crelles Journal), 2014
Abstract For complete affine manifolds we introduce a definition of compactification based on the projective differential geometry (i.e. geodesic path data) of the given connection. The definition of projective compactness involves a real parameter α called the order of projective compactness.
Cap, Andreas, Gover, A. Rod
openaire   +4 more sources

Rigidity of Weak Einstein-Randers Spaces [PDF]

open access: yesSahand Communications in Mathematical Analysis
The Randers metrics are popular metrics similar to the Riemannian metrics, frequently used in physical and geometric studies. The weak Einstein-Finsler metrics are a natural generalization of the Einstein-Finsler metrics.
Behnaz Lajmiri   +2 more
doaj   +1 more source

Metrics With Vanishing Quantum Corrections

open access: yes, 2008
We investigate solutions of the classical Einstein or supergravity equations that solve any set of quantum corrected Einstein equations in which the Einstein tensor plus a multiple of the metric is equated to a symmetric conserved tensor $T_{\mu \nu ...
A A Coley   +21 more
core   +1 more source

Spectral metric and Einstein functionals

open access: yesAdvances in Mathematics, 2023
We define bilinear functionals of vector fields and differential forms, the densities of which yield the metric and Einstein tensors on even-dimensional Riemannian manifolds. We generalise these concepts in non-commutative geometry and, in particular, we prove that for the conformally rescaled geometry of the noncommutative two-torus the Einstein ...
Ludwik Dabrowski   +2 more
openaire   +3 more sources

On Bochner Flat Kähler B-Manifolds

open access: yesAxioms, 2023
We obtain on a Kähler B-manifold (i.e., a Kähler manifold with a Norden metric) some corresponding results from the Kählerian and para-Kählerian context concerning the Bochner curvature. We prove that such a manifold is of constant totally real sectional
Cornelia-Livia Bejan   +2 more
doaj   +1 more source

Geometry for the accelerating universe [PDF]

open access: yes, 2006
The Lorentzian spacetime metric is replaced by an area metric which naturally emerges as a generalized geometry in quantum string and gauge theory. Employing the area metric curvature scalar, the gravitational Einstein-Hilbert action is re-interpreted as
C. Rovelli   +5 more
core   +2 more sources

Construction of the cosmological model with periodically distributed inhomogeneities with growing amplitude

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
We construct an approximate solution to the cosmological perturbation theory around Einstein–de Sitter background up to the fourth-order perturbations. This could be done with the help of the specific symmetry condition imposed on the metric, from which ...
Szymon Sikora, Krzysztof Głód
doaj   +1 more source

Distances of qubit density matrices on Bloch sphere

open access: yes, 2011
We recall the Einstein velocity addition on the open unit ball $\B$ of $\R^{3}$ and its algebraic structure, called the Einstein gyrogroup. We establish an isomorphism between the Einstein gyrogroup on $\B$ and the set of all qubit density matrices ...
Einstein A.   +3 more
core   +1 more source

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