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We replace the usual Hamiltonian constraint of quantum gravity H|psi>=0 by a weaker one <psi|H|psi>=0. This allows |psi> to satisfy the time-dependent functional Schrodinger equation. In general, only the phase of the wave function appears…

广义相对论与量子宇宙学 · 物理学 2007-05-23 H. Nikolic

Hamiltonian perturbation theory is used to analyse the stability of f(R) models. The Hamiltonian equations for the metric and its momentum conjugate are written for f(R) Lagrangian in the presence of perfect fluid matter. The perturbations…

广义相对论与量子宇宙学 · 物理学 2010-04-29 Tuomas Multamäki , Jaakko Vainio , Iiro Vilja

We deal with the problem of identifying a background structure and its perturbation in tetrad theories of gravity. Starting from a peculiar trivial principal bundle we define a metric which depends only on the gauge connection. We find the…

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

The evolution of a generally covariant theory is under-determined. One hundred years ago such dynamics had never before been considered; its ramifications were perplexing, its future important role for all the fundamental interactions under…

广义相对论与量子宇宙学 · 物理学 2016-11-23 James M. Nester , Chiang-Mei Chen

In the recently introduced gauge theory of translations, dubbed Coincident General Relativity, gravity is described with neither torsion nor curvature in the spacetime affine geometry. The action of the theory enjoys an enhanced symmetry…

广义相对论与量子宇宙学 · 物理学 2020-01-08 Jose Beltrán Jiménez , Lavinia Heisenberg , Tomi S. Koivisto

A straightforward method to compute Hamilton's density for theories that are linear in the spacetime curvature is provided. It is shown that the lapse function and shift vector still give rise to primary constraints, while the induced…

广义相对论与量子宇宙学 · 物理学 2022-06-23 Yuri Bonder

We discuss the interplay between standard canonical analysis and canonical discretization in three-dimensional gravity with cosmological constant. By using the Hamiltonian analysis, we find that the continuum local symmetries of the theory…

广义相对论与量子宇宙学 · 物理学 2015-05-19 J. Berra-Montiel , J. E. Rosales-Quintero

The Hamiltonian structure of General Relativity (GR), for both metric and tetrad gravity in a definite continuous family of space-times, is fully exploited in order to show that: i) the "Hole Argument" can be bypassed by means of a specific…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Luca Lusanna , Massimo Pauri

We describe a class of modified gravity theories that deform general relativity in a way that breaks time reversal invariance and, very mildly, locality. The algebra of constraints, local physical degrees of freedom, and their linearized…

广义相对论与量子宇宙学 · 物理学 2015-08-12 Marina Cortes , Henrique Gomes , Lee Smolin

The Hamiltonian formulation of the teleparallel equivalent of general relativity (TEGR) is developed from an ordinary second-order Lagrangian, which is written as a quadratic form of the coefficients of anholonomy of the orthonormal frames…

广义相对论与量子宇宙学 · 物理学 2016-11-30 Rafael Ferraro , María José Guzmán

We study a version of the recently proposed modified $F(R)$ Ho\v{r}ava-Lifshitz gravity that abandons the projectability condition of the lapse variable. We discovered that the projectable version of this theory has a consistent Hamiltonian…

高能物理 - 理论 · 物理学 2012-06-07 Masud Chaichian , Markku Oksanen , Anca Tureanu

Starting from a self-dual formulation of gravity, we obtain a noncommutative theory of pure Einstein theory in four dimensions. In order to do that, we use Seiberg-Witten map. It is shown that the noncommutative torsion constraint is solved…

高能物理 - 理论 · 物理学 2009-11-10 H. Garcia-Compean , O. Obregon , C. Ramirez , M. Sabido

Deformed Reissner-Nordstr\"om, as well as Reissner-Nordstr\"om de Sitter, solutions are obtained in a noncommutative gauge theory of gravitation. The gauge potentials (tetrad fields) and the components of deformed metric are calculated to…

高能物理 - 理论 · 物理学 2008-11-26 M. Chaichian , M. R. Setare , A. Tureanu , G. Zet

We develop a semiclassical theory of modified gravity with nontrivial spacetime torsion. In particular, we show that the semiclassical treatment can be axiomatized in the case of Einstein--Cartan theory with a nonminimally coupled, free…

广义相对论与量子宇宙学 · 物理学 2026-02-26 R. Morales-Cabrera , Y. Bonder

A well-defined regularized path integral for Lorentzian quantum gravity in three and four dimensions is constructed, given in terms of a sum over dynamically triangulated causal space-times. Each Lorentzian geometry and its associated…

高能物理 - 理论 · 物理学 2009-10-31 J. Ambjorn , J. Jurkiewicz , R. Loll

We construct a well-defined lattice-regularized quantum theory formulated in terms of fundamental fermion and gauge fields, the same type of degrees of freedom as in the Standard Model. The theory is explicitly invariant under local Lorentz…

高能物理 - 理论 · 物理学 2013-05-30 Alexey A. Vladimirov , Dmitri Diakonov

This is the first of a couple of papers in which, by exploiting the capabilities of the Hamiltonian approach to general relativity, we get a number of technical achievements that are instrumental both for a disclosure of \emph{new} results…

广义相对论与量子宇宙学 · 物理学 2014-11-17 L. Lusanna , M. Pauri

In gravity theories derived from a f(R) Lagrangian, matter is usually supposed to be minimally coupled to the metric, which hence defines a ``Jordan frame.'' However, since the field equations are fourth order, gravity possesses an extra…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Nathalie Deruelle , Misao Sasaki , Yuuiti Sendouda

Using the Ashtekar formulation, it is shown that the G_{Newton} --> 0 limit of Euclidean or complexified general relativity is not a free field theory, but is a theory that describes a linearized self-dual connection propagating on an…

高能物理 - 理论 · 物理学 2010-04-06 Lee Smolin

We study the canonical structure of the real first order formulation of general relativity on a null foliation. We use a tetrad decomposition which allows to elegantly encode the nature of the foliation in the norm of a vector in the fibre…

广义相对论与量子宇宙学 · 物理学 2015-03-25 Sergei Alexandrov , Simone Speziale