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
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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
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
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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
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UT code for WoS article
000303201900001
EID of the result in the Scopus database
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