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
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Czech description
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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
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Result continuities
Project
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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
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Volume of the periodical
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Issue of the periodical within the volume
12
Country of publishing house
GB - UNITED KINGDOM
Number of pages
19
Pages from-to
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UT code for WoS article
000329609000025
EID of the result in the Scopus database
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