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Comparison of general relativistic and pseudo-newtonian description of magellanic-clouds motion in the 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%2F12%3A%230004519" target="_blank" >RIV/47813059:19240/12:#0004519 - isvavai.cz</a>

  • Result on the web

    <a href="http://www.worldscientific.com/doi/pdf/10.1142/S0218271812500319" target="_blank" >http://www.worldscientific.com/doi/pdf/10.1142/S0218271812500319</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1142/S0218271812500319" target="_blank" >10.1142/S0218271812500319</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Comparison of general relativistic and pseudo-newtonian description of magellanic-clouds motion in the field of milky way

  • Original language description

    We test precision of the Cosmological Paczynski-Wiita (CPW) potential eflecting properties of the Schwarzschild-de Sitter (SdS) spacetimes in modeling dynamical phenomena related to galaxy motion. We consider a simplified model of Magellanic Clouds moving in the field of Milky Way as test particles. Time evolution of their position along trajectories obtained in the CPW framework using the notion of Newtonian time is compared to the one obtained in the fully general relativistic (GR) approach when the time evolution is expressed in terms of time related to the location of Earth in the Galaxy field. The differences in the position-evolution of the Magellanic Clouds obtained in the CPW and GR approaches are given for appropriately chosen values of the Milky Way mass. It is shown that the integrated relativistic corrections represent ~10^-5 part of the Newtonian CPW predictions for the orbital characteristics of the motion and slightly grow with Galaxy mass growing, being at least by one

  • Czech name

  • Czech description

Classification

  • Type

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

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    International Journal of Modern Physics D

  • ISSN

    0218-2718

  • e-ISSN

  • Volume of the periodical

    21

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    SG - SINGAPORE

  • Number of pages

    32

  • Pages from-to

  • UT code for WoS article

    000303201900001

  • EID of the result in the Scopus database