Abstract:We present an introduction to the geometry of higher-order vector and covector bundles (including higher-order generalizations of the Finsler geometry and Kaluza-Klein gravity) and review the basic results on Clifford and spinor structures on spaces with generic local anisotropy modeled by anholonomic frames with associated nonlinear connection structures. We emphasize strong arguments for application of Finsler-like geometries in modern string and gravity theory, noncommutative geometry and noncommutative fie… Show more
“…We have to state certain boundary/ symmetry/ topology conditions and define in explicit form the integration functions and systems of first order partial differential equations of type (8). This is necessary when we are interested to construct some explicit classes of exact solutions of Einstein equations (3) which are related to some physically important four and higher dimensional metrics.…”
Section: Introduction and Formulation Of Main Resultsmentioning
confidence: 99%
“…In this section, we outline the geometry of higher order nonholonomic manifolds which, for simplicity, will be modelled as (pseudo) Riemannian manifolds with higher order "shell" structure of dimensions k n = n + m + 1 m + ... + k m. Certain geometric ideas and constructions originate from the geometry of higher order Lagrange-Finsler and Hamilton-Cartan spaces defined on higher order (co) tangent classical and quantum bundles [10,11,12,13]. Such nonholonomic structures were investigated for models of (super) strings in higher order anisotropic (super) spaces [6] and for anholonomic higher order Clifford/ spinor bundles [7,8,9]. In explicit form, the (super) gravitational gauge field equations and conservations laws were analyzed in Refs.…”
Section: Higher Order Nonholonomic Manifoldsmentioning
confidence: 99%
“…It should be noted that for general coordinate transforms on k V, there is a mixing of coefficients and coordinates. 8 For simplicity, we can work with adapted coordinates when some sets of coordinates on a shell of lower order are contained in a subset of coordinates on shells of higher order by trivial extensions like u k−s α → u k−s+1 α = (u k−s α , y k−s+1 a ).…”
Section: Higher Order N-adapted Frames and Metricsmentioning
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.
“…We have to state certain boundary/ symmetry/ topology conditions and define in explicit form the integration functions and systems of first order partial differential equations of type (8). This is necessary when we are interested to construct some explicit classes of exact solutions of Einstein equations (3) which are related to some physically important four and higher dimensional metrics.…”
Section: Introduction and Formulation Of Main Resultsmentioning
confidence: 99%
“…In this section, we outline the geometry of higher order nonholonomic manifolds which, for simplicity, will be modelled as (pseudo) Riemannian manifolds with higher order "shell" structure of dimensions k n = n + m + 1 m + ... + k m. Certain geometric ideas and constructions originate from the geometry of higher order Lagrange-Finsler and Hamilton-Cartan spaces defined on higher order (co) tangent classical and quantum bundles [10,11,12,13]. Such nonholonomic structures were investigated for models of (super) strings in higher order anisotropic (super) spaces [6] and for anholonomic higher order Clifford/ spinor bundles [7,8,9]. In explicit form, the (super) gravitational gauge field equations and conservations laws were analyzed in Refs.…”
Section: Higher Order Nonholonomic Manifoldsmentioning
confidence: 99%
“…It should be noted that for general coordinate transforms on k V, there is a mixing of coefficients and coordinates. 8 For simplicity, we can work with adapted coordinates when some sets of coordinates on a shell of lower order are contained in a subset of coordinates on shells of higher order by trivial extensions like u k−s α → u k−s+1 α = (u k−s α , y k−s+1 a ).…”
Section: Higher Order N-adapted Frames and Metricsmentioning
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.
“…[ 26,19,20,21,31,32,33,34]) functions. Lifts of Sasaki type, or another ones, allow us to define canonical (Finsler type and generalizations) metric, F g, and N-connection, c N, structures.…”
Section: On "Well Defined" Finsler Gravity Theories and Cosmological mentioning
I do not agree with the authors of papers arXiv: 0806.2184 and 0901.1023v1 (published in Phys. Lett., respectively, B668 (2008) 453 and B676 (2009) 173). They consider that "In Finsler manifold, there exists a unique linear connection -the Chern connection ... It is torsion freeness and metric compatibility ... ". There are well known results (for example, presented in monographs by H. Rund and R. Miron and M. Anastasiei) that in Finsler geometry there exist an infinite number of linear connections defined by the same metric structure and that the Chern and Berwald connections are not metric compatible. For instance, the Chern's one (being with zero torsion and "weak" compatibility on the base manifold of tangent bundle) is not generally compatible with the metric structure on total space. This results in a number of additional difficulties and sophistication in definition of Finsler spinors and Dirac operators and in additional problems with further generalizations for quantum gravity and noncommutative/string/brane/gauge theories. I conclude that standard physics theories can be generalized naturally by gravitational and matter field equations for the Cartan and/or any other Finsler metric compatible connections. This allows us to construct more realistic models of Finsler spacetimes, anisotropic field interactions and cosmology.
“…[2,8] and for connection with spaces with torsion [9][10][11][12][13][14]). In a previous work, the above construction was extended to the case in which, alongside the diffeomorphisms and SO(4) rotations, local N = 1 supersymmetry transformations have been taken into account [15].…”
Abstract:We generalize previous works on the Dirac eigenvalues as dynamical variables of Euclidean gravity and N = 1 D = 4 supergravity to on-shell N = 2 D = 4 Euclidean supergravity. The covariant phase space of the theory is defined as the space of the solutions of the equations of motion modulo the on-shell gauge transformations. In this space we define the Poisson brackets and compute their value for the Dirac eigenvalues.
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