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The perfect dilaton-spin fluid (as a model of the dilaton matter, the particles of which are endowed with intrinsic spin and dilaton charge) is considered as the source of the gravitational field in a Weyl-Cartan spacetime. The variational…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Olga V. Babourova , Boris N. Frolov

According to the model ($\Lambda$CDM), based on deep cosmological observations, the current universe is constituted of 5$\%$ baryonic matter and 25 $\%$ non-baryonic cold dark matter (of speculative origin). These include quanta of scalar…

高能物理 - 唯象学 · 物理学 2022-01-19 Ankur Chaubey , Manoj K. Jaiswal , Damini Singh , Venktesh Singh , Avijit K. Ganguly

We show how Einstein-Cartan gravity can accommodate both global scale and local scale (Weyl) invariance. To this end, we construct a wide class of models with nonpropagaing torsion and a nonminimally coupled scalar field. In…

高能物理 - 理论 · 物理学 2021-12-08 Georgios K. Karananas , Mikhail Shaposhnikov , Andrey Shkerin , Sebastian Zell

In the framework of generally covariant (pre-metric) electrodynamics (``charge & flux electrodynamics''), the Maxwell equations can be formulated in terms of the electromagnetic excitation $H=({\cal D}, {\cal H})$ and the field strength…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Friedrich W. Hehl , Yuri N. Obukhov , Guillermo F. Rubilar

We reformulate the general theory of relativity in the language of Riemann-Cartan geometry. We start from the assumption that the space-time can be described as a non-Riemannian manifold, which, in addition to the metric field, is endowed…

广义相对论与量子宇宙学 · 物理学 2015-06-12 J. B. Fonseca-Neto , C. Romero , S. P. G. Martinez

We consider spacetime to be a 4-dimensional differentiable manifold that can be split locally into time and space. No metric, no linear connection are assumed. Matter is described by classical fields/fluids. We distinguish electrically…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Friedrich W. Hehl , Yuri N. Obukhov

In supersymmetric theories, the Peccei-Quinn symmetry has a complex extension as a symmetry of the superpotential, so that the scalar potential always has an almost flat direction, the dilaton. We discuss how coherent oscillation of the…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Hashimoto , K. -I. Izawa , M. Yamaguchi , T. Yanagida

In this paper we first show that any coupled system consisting of a gravitational plus a free electromagnetic field can be described geometrically in the sense that both Maxwell equations and Einstein equation having as source term the…

数学物理 · 物理学 2011-12-20 J. Fernando T. Giglio , Waldyr A. Rodrigues

Dipole charge conservation forces isolated charges to be immobile fractons. These couple naturally to spatial two-index symmetric tensor gauge fields that resemble a spatial metric. We propose a spacetime Lorentz covariant version of dipole…

高能物理 - 理论 · 物理学 2024-03-12 Evangelos Afxonidis , Alessio Caddeo , Carlos Hoyos , Daniele Musso

The main aim of the paper is to give a full classification (up to isometry) of all metric spaces X with the following two properties: X contains a compact set with non-empty interior; and for any three distinct points a, b and c of X there…

度量几何 · 数学 2025-01-08 Piotr Niemiec

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

The quotient of the conformal group of Euclidean 4-space by its Weyl subgroup results in a geometry possessing many of the properties of relativistic phase space, including both a natural symplectic form and non-degenerate Killing metric.…

广义相对论与量子宇宙学 · 物理学 2015-07-02 Jeffrey S Hazboun , James T Wheeler

Using the Schwarzschild coordinate frame for a static cyclic symmetric metric in 2 + 1 Einstein gravity coupled to a electric Maxwell field and a dilaton logarithmically depending on the radial coordinate in the presence of an exponential…

广义相对论与量子宇宙学 · 物理学 2014-12-19 A. A. Garcia-Diaz , G. Gutierrez Cano

Supersymmetric Peccei-Quinn symmetry and string theory predict a complex scalar field comprising a dilaton and an axion. These fields are massless at high energies, but it is known since long that the axion is stabilized in an instanton…

高能物理 - 唯象学 · 物理学 2016-10-26 R. Dick , M. Gaul

Following Kottler, \'E.Cartan, and van Dantzig, we formulate the Maxwell equations in a metric independent form in terms of the field strength $F=(E,B)$ and the excitation $H=({\cal D}, {\cal H})$. We assume a linear constitutive law…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Friedrich W. Hehl , Yuri N. Obukhov , Guillermo F. Rubilar

We study the Brans-Dicke model in the presence of an axion. The dynamical equations are solved when the fields are space independent and the metric is spatially flat. It is found that at late time the scale factor undergoes decelerated…

高能物理 - 理论 · 物理学 2009-10-30 Sudipta Mukherji

In this paper we intend to complement the identification given in Kuerten & Fernandes-Silva [1] (Mod. Phys. Lett. A. Vol. 33, No. 16) which relates the axion to a metric spinor phase by means of Maxwell's theory in the Infeld-van der…

高能物理 - 理论 · 物理学 2023-02-22 André Martorano Kuerten

The Maxwell equations are formulated on an arbitrary (1+3)-dimensional manifold. Then, imposing a (constrained) linear constitutive relation between electromagnetic field $(E,B)$ and excitation $({\cal D},{\cal H})$, we derive the metric of…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Yuri N. Obukhov , Friedrich W. Hehl

We start from the pure Einstein-Hilbert action in Metric Affine Gravity, with the orthonormal metric. We get an effective Levi-Civita Dilaton gravity theory in which the Dilaton field is related to the scaling of the gravitational coupling.…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Roberto Scipioni

In pregeometry a metric arises as a composite object at large distances. We investigate if its signature, which distinguishes between time and space, could be a result of the dynamics rather than being built in already in the formulation of…

广义相对论与量子宇宙学 · 物理学 2022-06-29 C. Wetterich
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