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Hamiltonian approach to GR - Part 1: covariant theory of classical gravity

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F17%3AA0000016" target="_blank" >RIV/47813059:19240/17:A0000016 - isvavai.cz</a>

  • Result on the web

    <a href="https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-4854-1" target="_blank" >https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-4854-1</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1140/epjc/s10052-017-4854-1" target="_blank" >10.1140/epjc/s10052-017-4854-1</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Hamiltonian approach to GR - Part 1: covariant theory of classical gravity

  • Original language description

    A challenging issue in General Relativity concerns the determination of the manifestly covariant continuum Hamiltonian structure underlying the Einstein field equations and the related formulation of the corresponding covariant Hamilton-Jacobi theory. The task is achieved by adopting a synchronous variational principle requiring distinction between the prescribed deterministic metric tensor (g) over cap (r) equivalent to {(g) over cap _(mu nu) (r)} solution of the Einstein field equations which determines the geometry of the background spacetime and suitable variational fields x equivalent to {g, pi} obeying an appropriate set of continuum Hamilton equations, referred to here as GR-Hamilton equations. It is shown that a prerequisite for reaching such a goal is that of casting the same equations in evolutionary form by means of a Lagrangian parametrization for a suitably reduced canonical state. As a result, the corresponding Hamilton-Jacobi theory is established in manifestly covariant form. Physical implications of the theory are discussed. These include the investigation of the structural stability of the GR-Hamilton equations with respect to vacuum solutions of the Einstein equations, assuming that wave-like perturbations are governed by the canonical evolution equations.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2017

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    European Physical Journal C

  • ISSN

    1434-6044

  • e-ISSN

    1434-6052

  • Volume of the periodical

    77

  • Issue of the periodical within the volume

    5

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    16

  • Pages from-to

    '329-1'-'329-16'

  • UT code for WoS article

    000401899900001

  • EID of the result in the Scopus database

    2-s2.0-85019833905