In this paper we propose a geometrically motivated formulation of gravity in an invariant Weyl--Integrable space-time (IWIST), in which the background geometry is not imposed a priori but is dynamically determined through the Palatini variational principle. For a scalar field non-minimally coupled to gravity action, the resulting compatibility condition defines a Weyl--Integrable geometry which is preserved by a local Weyl transformation of the metric and the geo\-me\-tri\-cal scalar field. We construct an action invariant under both diffeomorphisms and Weyl transformations and introduce a Weyl-covariant variational procedure based on an invariant extension of the divergence theorem. The corresponding field equations are obtained for the metric, the Weyl scalar, and the Weyl gauge field. We further formulate the theory in the Einstein--Riemann frame, where the effective metric is Riemannian and the scalar field is re\-inter\-pre\-ted as a phy\-si\-cal degree of freedom of geometric origin. Finally, we propose a geometrical mechanism for the explicit breaking of Weyl symmetry by introducing a coupling between the Weyl gauge field and a current constructed from the scalar sector. The resulting theory remains diffeomorphism covariant while departing from local Weyl invariance. The Einstein--Riemann representation of the broken theory contains an additional generally covariant interaction, making the Weyl-invariant model a particular limit of a more general gravitational theory.
Weyl geometry, in which the length scale can be chosen independently at each point of spacetime, provides a natural framework for extending general relativity through Weyl invariance, that is, local scale symmetry. We construct a gravitational theory whose Lagrangian is an arbitrary function of the scalar curvature in...
We study the conformal coupling in the torsion-free Palatini formulation with an ordinary scalar kinetic term. Tuning the curvature coupling cannot restore Weyl invariance in a Palatini theory with an ordinary scalar kinetic term because, for an independent and inert connection, the scalar-curvature term is separately...
We develop a non-commutative extension of pre-geometric gravity based on a BF theory with gauge group SO(1, 4) or SO(2, 3). The theory is formulated on a topological manifold without presupposing any spacetime metric, with coordinates promoted to non-commutative operators via the Moyal star product. Four constrained BF...
A. Addazi· International Journal of Mod...· 0 citations
We present the canonical quantization of Weyl-invariant gravity in a specific conformal gauge. Fixing the scale factor as a(η)=1/(H0η) yields an effective geometric cosmological term M(η)=α/η2 on the left-hand side of the Einstein equations, guaranteeing an equation of state w=−1 by construction. The Bianchi identity r...
Jorge Meza-Domínguez, Tonatiuh Matos· Classical and quantum gravit...· 0 citations
We describe a family of two-dimensional metric deformations that preserve integrability. The seeds are (classically) conformal integrable field theories and the deformations are directly related to different classes of auxiliary field sigma models. We introduce a master action connecting deformations by Lie-algebra-val...
N. Baglioni, Daniele Bielli, Parita Shah et al.· 0 citations
We investigate asymptotically Weyl-invariant gravity in the Palatini formulation, defined by an exponent that interpolates between an Einstein-like infrared regime, where n→1, and a Weyl-invariant ultraviolet regime, where n→2. In four dimensions, we show that exact Weyl invariance within the minimal scalar Palatini f(...
D. Coumbe· Classical and quantum gravit...· 1 citation
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