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Boundary terms of the Einstein-Hilbert action

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arxiv 1607.05986 v3 pith:AEAD3VUO submitted 2016-07-19 gr-qc hep-th

classification gr-qchep-th
keywords actionboundaryeinstein-hilbertwellgeneralwilldynamicalposed
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abstract

The Einstein-Hilbert action for general relativity is not well posed in terms of the metric $g_{ab}$ as a dynamical variable. There have been many proposals to obtain an well posed action principle for general relativity, e.g., addition of the Gibbons-Hawking-York boundary term to the Einstein-Hilbert action. These boundary terms are dependent on what one fixes on the boundary and in particular on spacetime dimensions as well. Following recent works of Padmanabhan we will introduce two new variables to describe general relativity and the action principle with these new dynamical variables will turn out to be well posed. Then we will connect these dynamical variables and boundary term obtained thereof to existing literature and shall comment on a few properties of Einstein-Hilbert action which might have been unnoticed earlier in the literature. Before concluding with future prospects and discussions, we will perform a general analysis of the boundary term of Einstein-Hilbert action for null surfaces as well.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Covariant virtual work and the d'Alembert-Lagrange formulation of general relativity

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    A covariant virtual work and d'Alembert-Lagrange formulation is introduced for general relativity, recovering the Einstein equations from vanishing virtual work and the cosmological constant from an isoperimetric admi...

  2. Boundary Term in the Gravitational Action is the Heat Content of the Null surfaces

    gr-qc 2019-08 accept novelty 5.0 of 10

    The gravitational boundary term on any null surface equals the heat density Ts, and its flow variation equals T ds.

  3. Motion of Particles in Solar and Galactic Systems by Using Neumann Boundary Condition

    astro-ph.GA 2019-09 reject novelty 4.0 of 10

    A modified equation of motion with a fitted constant acceleration is shown to reproduce LSB galaxy rotation curves and predict a dark-matter-like mass profile, while also predicting large solar-system perihelion precessions.

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