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An Introduction to Celestial Mechanics
2012This accessible text on classical celestial mechanics, the principles governing the motions of bodies in the Solar System, provides a clear and concise treatment of virtually all of the major features of solar system dynamics. Building on advanced topics in classical mechanics such as rigid body rotation, Langrangian mechanics and orbital perturbation ...
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Ambidextrous light transforms for celestial amplitudes
Journal of High Energy Physics, 2022Atul Sharma
exaly
1987
The equations of motion of central force motion of a point mass are given by (2.2.1) If the attracting force directed to the center satisfies Newton’s laws, we have (2.1.2) r and γ are the polar coordinates of motion, m and M are the masses of the two bodies, and γ and K are certain constants.
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The equations of motion of central force motion of a point mass are given by (2.2.1) If the attracting force directed to the center satisfies Newton’s laws, we have (2.1.2) r and γ are the polar coordinates of motion, m and M are the masses of the two bodies, and γ and K are certain constants.
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MHV graviton scattering amplitudes and current algebra on the celestial sphere
Journal of High Energy Physics, 2021Partha Paul
exaly