Multisymplectic unified formalism for Einstein-Hilbert gravity

We present a covariant multisymplectic formulation for the Einstein-Hilbert model of General Relativity. As it is described by a second-order singular Lagrangian, this is a gauge field theory with constraints. The use of the unified Lagrangian-Hamiltonian formalism is particularly interest- ing when...

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Bibliographic Details
Authors: Gaset Rifà, Jordi, Román Roy, Narciso|||0000-0003-3663-9861
Format: article
Publication Date:2018
Country:España
Institution:Universitat Politècnica de Catalunya (UPC)
Repository:UPCommons. Portal del coneixement obert de la UPC
Language:English
OAI Identifier:oai:upcommons.upc.edu:2117/117223
Online Access:https://hdl.handle.net/2117/117223
https://dx.doi.org/10.1063/1.4998526
Access Level:Open access
Keyword:Symplectic geometry
Fiber spaces (Mathematics)
Field theory (Physics)
General relativity (Physics)
2nd-order classical field theories
Higher-order jet bundles
Multisymplectic forms
Hilbert- Einstein action
Einstein equations.
Geometria simplèctica
Espais fibrats (Matemàtica)
Camps, Teoria dels (Física)
Relativitat general (Física)
Classificació AMS::53 Differential geometry::53D Symplectic geometry, contact geometry
Classificació AMS::55 Algebraic topology::55R Fiber spaces and bundles
Classificació AMS::70 Mechanics of particles and systems::70S Classical field theories
Classificació AMS::83 Relativity and gravitational theory::83C General relativity
Àrees temàtiques de la UPC::Matemàtiques i estadística::Geometria
Àrees temàtiques de la UPC::Matemàtiques i estadística::Matemàtica aplicada a les ciències
Description
Summary:We present a covariant multisymplectic formulation for the Einstein-Hilbert model of General Relativity. As it is described by a second-order singular Lagrangian, this is a gauge field theory with constraints. The use of the unified Lagrangian-Hamiltonian formalism is particularly interest- ing when it is applied to these kinds of theories, since it simplifies the treatment of them; in particular, the implementation of the constraint algorithm, the retrieval of the Lagrangian description, and the construction of the covariant Hamiltonian formalism. In order to apply this algorithm to the co- variant field equations, they must be written in a suitable geometrical way, which consists of using integrable distributions, represented by multivector fields of a certain type. We apply all these tools to the Einstein-Hilbert model without and with energy-matter sources. We obtain and explain the geometrical and physical meaning of the Lagrangian constraints and we construct the multimomen- tum (covariant) Hamiltonian formalisms in both cases. As a consequence of the gauge freedom and the constraint algorithm, we see how this model is equivalent to a first-order regular theory, without gauge freedom. In the case of presence of energy-matter sources, we show how some relevant geo- metrical and physical characteristics of the theory depend on the type of source. In all the cases, we obtain explicitly multivector fields which are solutions to the gravitational field equations. Finally, a brief study of symmetries and conservation laws is done in this context.