Curvature-matter couplings in modified gravity: from linear models to conformally invariant theories
arXiv:2203.03295 · doi:10.1142/S0218271822400107
Abstract
In this proceeding, we review modified theories of gravity with a curvature-matter coupling between an arbitrary function of the scalar curvature and the Lagrangian density of matter. This explicit nonminimal coupling induces a non-vanishing covariant derivative of the energy-momentum tensor, that implies non-geodesic motion and consequently leads to the appearance of an extra force. Here, we explore the physical and cosmological implications of the nonconservation of the energy-momentum tensor by using the formalism of irreversible thermodynamics of open systems in the presence of matter creation/annihilation. The particle creation rates, pressure, and the expression of the comoving entropy are obtained in a covariant formulation and discussed in detail. Applied together with the gravitational field equations, the thermodynamics of open systems lead to a generalization of the standard CDM cosmological paradigm, in which the particle creation rates and pressures are effectively considered as components of the cosmological fluid energy-momentum tensor. Furthermore, we also briefly present the coupling of curvature to geometry in conformal quadratic Weyl gravity, by assuming a coupling term of the form , where is the ordinary matter Lagrangian, and is the Weyl scalar. The coupling explicitly satisfies the requirement of the conformal invariance of the theory. Expressing with the use of an auxiliary scalar field and of the Weyl scalar, the gravitational action can be linearized in the Ricci scalar, leading in the Riemann space to a conformally invariant type theory, with the matter Lagrangian nonminimally coupled to geometry.
20 pages, no figures; based on a plenary talk in the 4th PU International Conference on Gravitation and Cosmology, 22-25 Nov., 2021; accepted for published in IJMPD (proceedings)
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Cited by in corpus (11)
- Palatini formulation of the conformally invariant gravity theory
- Cosmological tests of the osculating Barthel-Kropina dark energy model
- Constraining viscous dark energy equation of state in gravity
- Exploring wormhole solutions in curvature-matter coupling gravity supported by noncommutative geometry and conformal symmetry
- Compact stellar structures in Weyl geometric gravity
- Dynamical reconstruction of the CDM model in scalar-tensor gravity
- Cosmological implications of the Weyl geometric gravity theory
- Dynamical reconstruction of the CDM model in the scalar-tensor representation of gravity
- Irreversible Geometrothermodynamics of Open Systems in Modified Gravity
- Dissipative quintessence, and its cosmological implications
- Observational tests of the conformal osculating Barthel-Kropina cosmological model