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INVERSE N-BODY PROBLEM

31 March 2025, Version 1
This content is an early or alternative research output and has not been peer-reviewed by Cambridge University Press at the time of posting.

Abstract

The solution of the two-body gravitational problem led to the discovery of Newton's law of gravitation F = GMm/r^2. The solution of the inverse two-body problem (Bertrand problem) also leads to Newton's law of gravitation. However, the solution of the direct and inverse two-body problems does not provide a complete description of gravity. The law of gravitation for N bodies is missing. The fundamental law of gravitation for N bodies has not been discovered. The obstacle was the unsolved gravitational problem of N bodies. The inverse problem of N-bodies has not been studied in physics. Here we present a new method for finding the law of gravitational force for N bodies. The method is based on reducing the gravitational problem of N bodies to the two-body problem, where the central body is a system of N bodies. The problem of an N-body system is the inverse problem of the N-body problem. This is the problem of finding the law of gravitational force from the known integral characteristics of the N-body system. The solution of the inverse problem of N bodies gives a new law of gravitation F = (mc^2)√Ʌ. Instead of the gravitational constant G, the new law of gravity includes the cosmological constant Ʌ. The new law of gravity F = (mc^2)√Ʌ allows us to overcome the limitations inherent in Newton's law of gravity F = GMm/r^2 and leads to a new law of universal gravitation.

Keywords

Newton's law
N-body problem
law of universal gravitation
parameters of the observable universe
cosmological constant Ʌ.

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