On Singularities and Instability for Different Couplings between Scalar Field and Multidimensional Geometry
U. BLEYER, M. RAINER
Abstract
We consider a multidimensional model of the universe given as a D-dimensional geometry, represented by a Riemannian manifold (M,g) with arbitrary signature of g, M= × M1× ·s × Mn, where the Mi of dimension di are Einstein spaces, compact for i>1. For Lagrangian models L(R,ϕ) on M which depend only on the Ricci curvature R and a scalar field ϕ, there exists a conformal equivalence with minimal coupling models. For certain nonminimal models we study classical solutions and their relation to solutions in the equivalent minimal coupling model. The domains of equivalence are separated by certain critical values of the scalar field ϕ. Furthermore, the coupling constant ξ of the coupling between ϕ and R is critical at both, the minimal value ξ=0 and the conformal value ξc=D-24(D-1). In different noncritical regions of ξ the solutions behave qualitatively different. Instability can occure only in certain ranges of ξ. This paper is dedicated to Prof. D. D. Ivanenko.
Create a lesson
Related papers
Gravitational-Wave Constraints on R2 Gravity
Pawan Kumar Gupta, Laura Sagunski
Axial black hole perturbations in purely-metric Horndeski theories
Héloïse Delaporte, Hugo Roussille
Inflationary attractors in metric-affine gravity
Ilaria Andrei, Christian Dioguardi
Born-Infeld black holes in bumblebee gravity
A. A. Araújo Filho, E. M. Siquieri, N. Heidari et al.
Quasi-equilibrium tidal folds of white dwarfs around rotating black holes in shift-symmetric Einstein--scalar--Gauss--Bonnet gravity
Shoupan Liu, Meilin Liu, Yu Wang et al.
Dipolar boson stars as static two-body systems: an effective-one-body description
Thibault Damour, Romain Gervalle, Tamanna Jain