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- W4220683024 abstract "Abstract By using geodesic equations to obtain a gravitational potential generated from an initially point-like source, we end up in the concept of a nearly Newtonian gravity to analyse effective potentials of quasi-circular orbits. By means of an approximate solution from an axially static and symmetric Weyl metric, we provide a numerical study on effective gravitational potential to investigate the character of motion in the meridional plane of an axially symmetric galaxy model obtaining periodic regular box orbits. Moreover, as a test for a toy model and using as initial condition a Plummer sphere, some initial prospects on star N-body simulation of cluster disruption were obtained for clusters with mass about $$3times 10^4;M_{odot }$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:mn>3</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mn>4</mml:mn> </mml:msup> <mml:mspace /> <mml:msub> <mml:mi>M</mml:mi> <mml:mo>⊙</mml:mo> </mml:msub> </mml:mrow> </mml:math> . In the studied cases, our results suggest that such disruptions are caused mostly by their gravitational processes than baryonic content in accordance with $$varLambda $$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mi>Λ</mml:mi> </mml:math> CDM bottom-up hierarchy." @default.
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- W4220683024 date "2022-03-01" @default.
- W4220683024 modified "2023-10-18" @default.
- W4220683024 title "Effective potentials and orbits in Weyl slender disk" @default.
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- W4220683024 doi "https://doi.org/10.1140/epjc/s10052-022-10175-6" @default.
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