Motion in a combined Newtonian gravitational field

We study a test particle moving under the influence of a system of two massive bodies in Newtonian gravity. Our main objective is to reveal and understand how the ratio of the masses of the two bodies, as well as the energy of the test particle, affects its nature of motion. For this purpose, we conduct a detailed and systematic survey by classifying the initial conditions of trajectories. In particular, we scan the phase space by considering two-dimensional (2D) maps on several types of planes. Then, we numerically integrate the starting conditions on these 2D maps and determine their final states. This procedure allows us to obtain a clear view of how the change in the masses and the energy influence the final states of the test particles. © 2023

Authors
Alrebdi H.I. , Alsaif N.A.M. , Steklain A.F. , Zotos E.E.
Publisher
Elsevier Ltd
Language
English
Status
Published
Number
113817
Volume
174
Year
2023
Organizations
  • 1 Department of Physics, College of Science, Princess Nourah bint Abdulrahman University, P.O. Box 84428, Riyadh, 11671, Saudi Arabia
  • 2 Department of Mathematics, Universidade Tecnológica Federal do Paraná, Curitiba, 80230901, Brazil
  • 3 Department of Physics, School of Science, Aristotle University of Thessaloniki, Thessaloniki, 541 24, Greece
  • 4 S.M. Nikolskii Mathematical Institute of the Peoples’ Friendship University of Russia (RUDN University), Moscow, 117198, Russian Federation
Keywords
Binary systems; Chaos indicators; Orbit taxonomy

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