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Modelling capabilities of Thermodynamic Gravity (TG) are compared to Dark Matter (DM) and Modified Newtonian Dynamics (MOND). The gravitational field equation of TG is solved using the mass distribution of the baryonic mass as the source of the gravitational field. In this paper, the numerical method is verified with the help of exact solutions. Th...
The long-term dynamical evolution is a crucial point in recent planetary research. Although the amount of observational data is continuously growing and the precision allows us to obtain accurate planetary orbits, the canonical stability analysis still requires N-body simulations and phase space trajectory investigations. We propose a method for st...
