Abstract:We apply the method of moving anholonomic frames, with associated nonlinear
connections, in (pseudo) Riemannian spaces and examine the conditions when
various types of locally anisotropic (la) structures (Lagrange, Finsler like
and more general ones) could be modeled in general relativity. New classes of
solutions of the Einstein equations with generic local anisotropy are
constructed. We formulate the theory of nearly autoparallel (na) maps and
introduce the tensorial na-integration as the inverse operation t… Show more
“…The equation (33) contains only derivatives on y 4 = v and allows us to define h 4 (x i , v) for a given h 5 (x i , v), or inversely, for h * 4,5 = 0. Having defined h 4 and h 5 , we can compute the coefficients (36), which allows us to find w i from algebraic equations (34) and to compute n i by integrating two times on v as follow from equations (35). Similar properties hold true for equations on higher order shells.…”
Section: The System Of N-adapted Einstein Equationsmentioning
confidence: 99%
“…In explicit form, the (super) gravitational gauge field equations and conservations laws were analyzed in Refs. [33,34,35,36].…”
Section: Higher Order Nonholonomic Manifoldsmentioning
confidence: 99%
“…• Having defined h 4 and h 5 and computed γ from (36), we can solve the equation (35) by integrating on variable "v" the equation n * * i + γn * i = 0. The exact solution is…”
Section: Exact Solutions With Killing Symmetriesmentioning
confidence: 99%
“…Such constructions are similar to those presented in above Theorems and in Refs. [1,2,3,4,30,31,32,6,7,8,9,34,35,36]. Some additional necessary formulas are given in Appendices.…”
We prove that the Einstein equations can be solved in a very general form for arbitrary spacetime dimensions and various types of vacuum and non-vacuum cases following a geometric method of anholonomic frame deformations for constructing exact solutions in gravity. The main idea of this method is to introduce on (pseudo) Riemannian manifolds an alternative (to the Levi-Civita connection) metric compatible linear connection which is also completely defined by the same metric structure. Such a canonically distinguished connection is with nontrivial torsion which is induced by some nonholonomy frame coefficients and generic off-diagonal terms of metrics. It is possible to define certain classes of adapted frames of reference when the Einstein equations for such an alternative connection transform into a system of partial differential equations which can be integrated in very general forms. Imposing nonholonomic constraints on generalized metrics and connections and adapted frames (selecting Levi-Civita configurations), we generate exact solutions in Einstein gravity and extra dimension generalizations.
“…The equation (33) contains only derivatives on y 4 = v and allows us to define h 4 (x i , v) for a given h 5 (x i , v), or inversely, for h * 4,5 = 0. Having defined h 4 and h 5 , we can compute the coefficients (36), which allows us to find w i from algebraic equations (34) and to compute n i by integrating two times on v as follow from equations (35). Similar properties hold true for equations on higher order shells.…”
Section: The System Of N-adapted Einstein Equationsmentioning
confidence: 99%
“…In explicit form, the (super) gravitational gauge field equations and conservations laws were analyzed in Refs. [33,34,35,36].…”
Section: Higher Order Nonholonomic Manifoldsmentioning
confidence: 99%
“…• Having defined h 4 and h 5 and computed γ from (36), we can solve the equation (35) by integrating on variable "v" the equation n * * i + γn * i = 0. The exact solution is…”
Section: Exact Solutions With Killing Symmetriesmentioning
confidence: 99%
“…Such constructions are similar to those presented in above Theorems and in Refs. [1,2,3,4,30,31,32,6,7,8,9,34,35,36]. Some additional necessary formulas are given in Appendices.…”
We prove that the Einstein equations can be solved in a very general form for arbitrary spacetime dimensions and various types of vacuum and non-vacuum cases following a geometric method of anholonomic frame deformations for constructing exact solutions in gravity. The main idea of this method is to introduce on (pseudo) Riemannian manifolds an alternative (to the Levi-Civita connection) metric compatible linear connection which is also completely defined by the same metric structure. Such a canonically distinguished connection is with nontrivial torsion which is induced by some nonholonomy frame coefficients and generic off-diagonal terms of metrics. It is possible to define certain classes of adapted frames of reference when the Einstein equations for such an alternative connection transform into a system of partial differential equations which can be integrated in very general forms. Imposing nonholonomic constraints on generalized metrics and connections and adapted frames (selecting Levi-Civita configurations), we generate exact solutions in Einstein gravity and extra dimension generalizations.
“…An extensive and general treatment of the notion of non-linear connection, allowing for connections in associated bundles that are g-compatible, can be found in the work of Vacaru et al (for example [12] and [14]) in the contest of Lagrange spaces and other generalizations. In this general framework, the coefficients of an alternative non-linear connection are given by:…”
Caianiello's derivation of Quantum Geometry through an isometric embedding of the spacetime (M,g) in the pseudo-Riemannian structure (T * M, g * AB ) is reconsidered. In the new derivation, a non-linear connection and the bundle formalism induce a Lorentzian-type structure in the 4-dimensional manifold M that is covariant under arbitrary local coordinate transformations in M. If models with maximal acceleration are required to be non-trivial, gravity should be supplied with other interactions in a unification framework.
We study the fractional gravity for spacetimes with non-integer fractional derivatives. Our constructions are based on a formalism with the fractional Caputo derivative and integral calculus adapted to nonholonomic distributions. This allows us to define a fractional spacetime geometry with fundamental geometric/physical objects and a generalized tensor calculus all being similar to respective integer dimension constructions. Such models of fractional gravity mimic the Einstein gravity theory and various Lagrange-Finsler and Hamilton-Cartan generalizations in nonholonomic variables. The approach suggests a number of new implications for gravity and matter field theories with singular, stochastic, kinetic, fractal, memory etc processes. We prove that the fractional gravitational field equations can be integrated in very general forms following the anholonomic deformation method for constructing exact solutions. Finally, we study some examples of fractional black hole solutions, ellipsoid gravitational configurations and imbedding of such objects in solitonic backgrounds.
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