Modified Einstein and Finsler like theories on tangent Lorentz bundles

Author:

Stavrinos Panayiotis1,Vacaru Olivia2,Vacaru Sergiu I.34

Affiliation:

1. Department of Mathematics, University of Athens, Ilissia, Athens 15784, Greece

2. National College of Iaşi, 4 Arcu Street, Iaşi 700125, Romania

3. Theory Division, CERN, CH-1211, Geneva 23, Switzerland

4. University "Al. I. Cuza" Iaşi, Rector's Office, 14 Alexandru Lapuşneanu Street, Corpus R, UAIC, Office 323, Iaşi 700057, Romania

Abstract

In this paper, we study modifications of general relativity, GR, with nonlinear dispersion relations which can be geometrized on tangent Lorentz bundles. Such modified gravity theories, MGTs, can be modeled by gravitational Lagrange density functionals f(R, T, F) with generalized/modified scalar curvature R, trace of matter field tensors T and modified Finsler like generating function F. In particular, there are defined extensions of GR with extra dimensional "velocity/momentum" coordinates. For four-dimensional models, we prove that it is possible to decouple and integrate in very general forms the gravitational fields for f(R, T, F)-modified gravity using nonholonomic 2 + 2 splitting and nonholonomic Finsler like variables F. We study the modified motion and Newtonian limits of massive test particles on nonlinear geodesics approximated with effective extra forces orthogonal to the four-velocity. We compute the constraints on the magnitude of extra-accelerations and analyze perihelion effects and possible cosmological implications of such theories. We also derive the extended Raychaudhuri equation in the framework of a tangent Lorentz bundle. Finally, we speculate on effective modeling of modified theories by generic off-diagonal configurations in Einstein and/or MGTs and Finsler gravity. We provide some examples for modified stationary (black) ellipsoid configurations and locally anisotropic solitonic backgrounds.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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