Newtonian and relativistic theory of orbits and emission of gravitational waves
Mariafelicia De Laurentis

TL;DR
This review explores the classical and relativistic theories of orbital motion, including gravitational wave emission, focusing on the Newtonian framework, post-Newtonian corrections, and various orbit classifications.
Contribution
It provides a comprehensive comparison of Newtonian and relativistic orbital theories and calculates gravitational wave luminosity for different stellar encounters.
Findings
Derived gravitational wave luminosity for various orbit types
Analyzed relativistic corrections to orbital motion
Classified orbits based on motion conditions
Abstract
This review paper is devoted to the theory of orbits. We start with the discussion of the Newtonian problem of motion then we consider the relativistic problem of motion, in particular the PN approximation and the further gravitomagnetic corrections. Finally by a classification of orbits in accordance with the conditions of motion, we calculate the gravitational waves luminosity for different types of stellar encounters and orbits.
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