J 2012

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

SCHEE, Jan and Zdeněk STUCHLÍK

Basic information

Original name

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

Authors

SCHEE, Jan and Zdeněk STUCHLÍK

Edition

International Journal of Modern Physics D, SG - Singapurská republika, 2012, 0218-2718

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

www

Organization unit

Faculty of Philosophy and Science in Opava

DOI

http://dx.doi.org/10.1142/S0218271812500319

UT WoS

000303201900001

Keywords in English

General relativity; Magellanic Clouds; Milky Way; Pseudo-Newtonian potential

Tags

UF

Tags

International impact, Reviewed

Links

MSM4781305903, plan (intention).
Změněno: 14/1/2021 14:24, Mgr. Pavlína Jalůvková

Abstract

V originále

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
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