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Boundary effects in General Relativity with tetrad variables

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In this paper, the authors study general boundary variations using tetrads instead of the metric and show that the spin-1 momentum coincides with the rotational 1-form of isolated horizons.
Abstract
Varying the gravitational Lagrangian produces a boundary contribution that has various physical applications. It determines the right boundary terms to be added to the action once boundary conditions are specified, and defines the symplectic structure of covariant phase space methods. We study general boundary variations using tetrads instead of the metric. This choice streamlines many calculations, especially in the case of null hypersurfaces with arbitrary coordinates, where we show that the spin-1 momentum coincides with the rotational 1-form of isolated horizons. The additional gauge symmetry of internal Lorentz transformations leaves however an imprint: the boundary variation differs from the metric one by an exact 3-form. On the one hand, this difference helps in the variational principle: gluing hypersurfaces to determine the action boundary terms for given boundary conditions is simpler, including the most general case of non-orthogonal corners. On the other hand, it affects the construction of Hamiltonian surface charges with covariant phase space methods, which end up being generically different from the metric ones, in both first and second-order formalisms. This situation is treated in the literature gauge-fixing the tetrad to be adapted to the hypersurface or introducing a fine-tuned internal Lorentz transformation depending non-linearly on the fields. We point out and explore the alternative approach of dressing the bare symplectic potential to recover the value of all metric charges, and not just for isometries. Surface charges can also be constructed using a cohomological prescription: in this case we find that the exact 3-form mismatch plays no role, and tetrad and metric charges are equal. This prescription leads however to different charges whether one uses a first-order or second-order Lagrangian, and only for isometries one recovers the same charges.

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Edge modes of gravity. Part I. Corner potentials and charges

TL;DR: In this article, the classical and quantum nature of edge modes and symmetries in gravity systems is investigated. But the main focus of this paper is to understand how different formulations of gravity provide non-trivial representations of different sectors of the corner symmetry algebra, and set the foundations of a new proposal for states of quantum geometry as representation states of this corner algebra.
Journal ArticleDOI

Edge modes of gravity -- I: Corner potentials and charges

TL;DR: In this paper, the classical and quantum nature of edge modes and symmetries in gravity systems has been investigated and a new proposal for states of quantum geometry as representation states of the corner symmetry algebra has been made.
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The Weyl BMS group and Einstein’s equations

TL;DR: Weyl BMSW as mentioned in this paper is an extension of the BMS group, which includes super-translations, local Weyl rescalings and arbitrary diffeomorphisms of the 2D sphere metric.
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Edge modes of gravity. Part II. Corner metric and Lorentz charges

TL;DR: In this paper, a new program for quantum gravity, grounded in the notion of corner symmetry algebra and its representations, was proposed, where the dynamical variables of the tetrad gravity corner phase space are the internal normal to the spacetime foliation, which is conjugated to the boost generator.
Journal ArticleDOI

Edge modes of gravity -- II: Corner metric and Lorentz charges

TL;DR: In this paper, a new program for quantum gravity, grounded in the notion of corner symmetry algebra and its representations, was proposed, where the dynamical variables of the tetrad gravity corner phase space are the internal normal to the spacetime foliation, which is conjugated to the boost generator.
References
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Journal ArticleDOI

General Relativity with Spin and Torsion: Foundations and Prospects

TL;DR: In this article, a generalization of Einstein's gravitational theory is discussed in which the spin of matter as well as its mass plays a dynamical role, and the theory which emerges from taking this coupling into account, the ${U}_{4}$ theory of gravitation, predicts, in addition to the usual infinite-range gravitational interaction medicated by the metric field, a new, very weak, spin contact interaction of gravitational origin.
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Gravitational Waves in General Relativity. VII. Waves from Axi-Symmetric Isolated Systems

TL;DR: In this paper, it is shown that the flow of information to infinity is controlled by a single function of two variables called the news function, together with initial conditions specified on a light cone, which fully defines the behaviour of the system.
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Some properties of Noether charge and a proposal for dynamical black hole entropy

TL;DR: It is proved that the first law of black hole mechanics holds for arbitrary perturbations of a stationary black hole, and a local, geometrical prescription is proposed for the entropy, $S_{dyn}$, of a dynamical black hole.
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The Dynamics of General Relativity

TL;DR: This article appeared as Chapter 7 of an often cited compendium edited by L. Witten in 1962 as mentioned in this paper, which is now long out of print and is intended to provide contemporary accessibility to the flavor of the original ideas.
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Republication of: The dynamics of general relativity

TL;DR: The Golden Oldie as discussed by the authors is an unretouched version of the Witten formulation of General Relativity, originally published as Chap. 7, pp. 227-264, in Gravitation: an introduction to current research, L. Witten, ed.
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