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Influence of the cosmic repulsion on the MOND model of the Magellanic Cloud 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%2F13%3A%230004772" target="_blank" >RIV/47813059:19240/13:#0004772 - isvavai.cz</a>

  • Result on the web

    <a href="http://iopscience.iop.org/1475-7516/2013/12/026/" target="_blank" >http://iopscience.iop.org/1475-7516/2013/12/026/</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1475-7516/2013/12/026" target="_blank" >10.1088/1475-7516/2013/12/026</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Influence of the cosmic repulsion on the MOND model of the Magellanic Cloud motion in the field of Milky Way

  • Original language description

    It has been recently shown that the cosmic repulsion can have a highly significant influence on the motion of Magellanic Clouds (MC) in the gravitational field of Milky Way, treated in the framework of the Cold Dark Matter (CDM) halo model. However, there is an alternative to the CDM halo explanation of the rotation curves in the periphery of spiral galaxies, based on MOdified Newtonian Dynamics (MOND). Therefore, we study the role of the cosmic repulsion in the framework of the MOND theory applied to determine the MC motion. Our results demonstrate that in the MOND framework the influence of the cosmic repulsion on the motion of both Small and Large MC is also highly significant, but it is of a different character than in the framework of the CDM halomodel. Moreover, we demonstrate that the MC motion in the framework of the CDM halo and MOND models is subtantially different and can serve as a test of these fundamentally different approaches to the explanation of the phenomena related

  • 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

    S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2013

  • 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

    12

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    19

  • Pages from-to

  • UT code for WoS article

    000329609000025

  • EID of the result in the Scopus database