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Influence of the cosmological constant on the motion of Magellanic Clouds in the gravitational field of Milky Way

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F11%3A%230003873" target="_blank" >RIV/47813059:19240/11:#0003873 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/1475-7516/2011/09/018" target="_blank" >http://dx.doi.org/10.1088/1475-7516/2011/09/018</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1475-7516/2011/09/018" target="_blank" >10.1088/1475-7516/2011/09/018</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Influence of the cosmological constant on the motion of Magellanic Clouds in the gravitational field of Milky Way

  • Original language description

    Using the pseudo-Newtonian (RN) potential reflecting properties of the Schwarzschild-de Sitter spacetime, we estimate the influence of the repulsive cosmological constant Lambda similar to 1.3 x 10(-56)cm(-2) implied by recent cosmological tests onto themotion of both Small and Large Magellanic Clouds (SMC and LMC) in the gravitational field of the Milky Way. Considering detailed modelling of the gravitational field of the Galaxy disc, bulge and cold dark matter halo, the trajectories of SMC and LMC constructed for the PN potential with the cosmological constant are confronted to those given for Lambda = 0. In the realistic model of the extended cold dark matter halo its edge and related total mass are taken at typical values reflecting recent diversity in the total Galaxy mass estimates. In all cases, strong influence of the cosmological constant, on 10% level or higher, has been found for motion of both SMC and LMC. Inside the halo, the Newtonian part of the PN potential is exact en

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BE - Theoretical physics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/LC06014" target="_blank" >LC06014: Center for Theoretical Astrophysics</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2011

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS

  • ISSN

    1475-7516

  • e-ISSN

  • Volume of the periodical

  • Issue of the periodical within the volume

    9

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    31

  • Pages from-to

    018

  • UT code for WoS article

  • EID of the result in the Scopus database