6533b829fe1ef96bd128a418
RESEARCH PRODUCT
Anisotropic deformations in a class of projectively-invariant metric-affine theories of gravity
Daniel De AndrésJose Beltrán JiménezAdrià Delhomsubject
PhysicsPhysics and Astronomy (miscellaneous)Spacetime010308 nuclear & particles physicsIsotropyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)16. Peace & justiceSpecial class01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciencesHomogeneous spaceAffine transformationAnisotropy010303 astronomy & astrophysicsRicci curvaturedescription
Among the general class of metric-affine theories of gravity, there is a special class conformed by those endowed with a projective symmetry. Perhaps the simplest manner to realise this symmetry is by constructing the action in terms of the symmetric part of the Ricci tensor. In these theories, the connection can be solved algebraically in terms of a metric that relates to the spacetime metric by means of the so-called deformation matrix that is given in terms of the matter fields. In most phenomenological applications, this deformation matrix is assumed to inherit the symmetries of the matter sector so that in the presence of an isotropic energy-momentum tensor, it respects isotropy. In this work we discuss this condition and, in particular, we show how the deformation matrix can be anisotropic even in the presence of isotropic sources due to the non-linear nature of the equations. Remarkably, we find that Eddington-inspired-Born-Infeld theories do not admit anisotropic deformations, but more general theories do. However, we find that the anisotropic branches of solutions are generally prone to a pathological physical behaviour.
year | journal | country | edition | language |
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2020-10-21 | Classical and Quantum Gravity |