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The corrections to the cosmological models induced by non-minimal coupling between scalar field and torsion are considered. To determine these corrections in explicit form, the power-law parametrization of these corrections are proposed.…

广义相对论与量子宇宙学 · 物理学 2025-03-25 I. V. Fomin , S. V. Chervon , L. K. Duchaniya , B. Mishra

In general relativity the affine connection is required to be symmetric so torsion is zero while according to the Einsten- Cartan's theory torsion is connected to the spin tensor as expressed by the Cartan's equations. We consider the…

广义相对论与量子宇宙学 · 物理学 2022-11-24 Elisa Varani

We study the holographic dual description of a superconductor in which the gravity sector consists of a Maxwell field and a charged scalar field which except its minimal coupling to gravity it is also coupled kinematically to Einstein…

高能物理 - 理论 · 物理学 2016-09-02 Xiao-Mei Kuang , Eleftherios Papantonopoulos

We explore a novel cosmological model based on coupled fields in the framework of scalar tensor theories, considering the specific interplay between gravity and scalar fields. The model further extends a recent axion-dilaton system by…

广义相对论与量子宇宙学 · 物理学 2025-11-25 Mihai Marciu

We consider gravity from the quantum field theory point of view and introduce a natural way of coupling gravity to matter by following the gauge principle for particle interactions. The energy-momentum tensor for the matter fields is shown…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Yuan K. Ha

We compute the spectrum of scalar models with a general coupling to the scalar curvature. We find that the perturbative states of these theories are given by two massive spin-0 modes in addition to one massless spin-2 state. This latter…

广义相对论与量子宇宙学 · 物理学 2020-02-12 Ismael Ayuso , Jose A. R. Cembranos

We study accelerating Universes with power-law scale-factors. We include shear and vorticity, a cosmological "constant" term, and spin from torsion, as in Einstein-Cartan's theory when a scalar-field of Brans-Dicke type acts in the model.…

综合物理 · 物理学 2009-01-14 Marcelo Samuel Berman

We make it precise what it means to have a connection with torsion as solution of the Einstein equations. While locally the theory remains the same, the new formulation allows for topologies that would have been excluded in the standard…

高能物理 - 理论 · 物理学 2011-08-02 M. A. Lledo , L. Sommovigo

We consider the scale-invariant inflationary model studied in [1]. The Lagrangian includes all the scale-invariant operators that can be built with combinations of $R$, $R^2$ and one scalar field. The equations of motion show that the…

广义相对论与量子宇宙学 · 物理学 2017-03-14 Giovanni Tambalo , Massimiliano Rinaldi

A propagating torsion model is derived from the requirement of compatibility between minimal action principle and minimal coupling procedure in Riemann-Cartan spacetimes. In the proposed model, the trace of the torsion tensor is derived…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Alberto Saa

The field equations for gravitation and electromagnetism with sources in four dimensions can be interpreted as arising from the vacuum Einstein equations in five dimensions. Gauge invariance of the electromagnetic potentials leads to a…

高能物理 - 理论 · 物理学 2007-05-23 Tomas Liko

We consider Lorentz invariant scalar-tensor teleparallel gravity theories with a Lagrangian built from the torsion scalar, a scalar field, its kinetic term and a derivative coupling between the torsion and the scalar field. The field…

广义相对论与量子宇宙学 · 物理学 2018-09-12 Manuel Hohmann , Christian Pfeifer

We investigate the cosmological dynamics of a homogeneous scalar field non-minimally coupled to torsion gravity, which also interacts with cold dark matter through energy and momentum transfer. The matter and radiation perfect fluids are…

广义相对论与量子宇宙学 · 物理学 2025-02-05 Carlos Rodriguez-Benites , Manuel Gonzalez-Espinoza , Giovanni Otalora , Manuel Alva-Morales

The Horndeski Lagrangian brings together all possible interactions between gravity and a scalar field that yield second-order field equations in four-dimensional spacetime. As originally proposed, it only addresses phenomenology without…

广义相对论与量子宇宙学 · 物理学 2017-10-18 José Barrientos , Fabrizio Cordonier-Tello , Fernando Izaurieta , Perla Medina , Daniela Narbona , Eduardo Rodríguez , Omar Valdivia

We study the Poincar\'e gauge theory of gravity with the most general Lagrangian quadratic in curvature and torsion, focusing on the possible interaction of the axial torsion with the electromagnetic field. From the analysis of the closed…

广义相对论与量子宇宙学 · 物理学 2024-10-03 Mariya Iv. Trukhanova , Yu. N. Obukhov

In this study we explore the cosmological behavior of a non-minimally coupled scalar field that is linked to torsion gravity. We demonstrate the Sorkin-Schutz formalism with general power law teleparallel torsion coupling. The autonomous…

广义相对论与量子宇宙学 · 物理学 2025-04-08 S. A. Kadam

Cosmologies based on General Relativity encompassing an anti-symmetric connection (torsion) can display nice desirable features as the absence of the initial singularity and the possibility of inflation in the early stage of the universe.…

广义相对论与量子宇宙学 · 物理学 2018-12-12 Sergio Bravo Medina , Marek Nowakowski , Davide Batic

It has been known for a long time that the presence of torsion is in conflict with gauge invariance of the the electromagnetic field in curved Riemann-Cartan space if the Maxwell field is minimally coupled to the curved gravitational space…

广义相对论与量子宇宙学 · 物理学 2017-01-31 H. T. Nieh

A new class of gravity-matter models defined in terms of two independent non-Riemannian volume forms (alternative generally covariant integration measure densities) on the space-time manifold are studied in some detail. These models involve…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Eduardo Guendelman , Ramón Herrera , Pedro Labraña , Emil Nissimov , Svetlana Pacheva

We consider a possible (parity conserving) interaction between the electromagnetic field $F$ and a torsion field $T^\alpha$ of spacetime. For generic elementary torsion, gauge invariant coupling terms of lowest order fall into two classes…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Yakov Itin , Friedrich W. Hehl
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