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Shows that exact solutions to the Kepler (two-body), the Euler (two-fixed center), and the Vinti (earth-satellite) problems can all be put in a form that admits the general representation of the orbits and follows a definite shared pattern
Includes a full analysis of the planar Euler problem via a clear generalization of the form of the solution in the Kepler case
Original insights that have hithertofore not appeared in book form
Direct involvement with the subject area of the present work dates from my years with NASA at its Electronics Research Center (ERC) in Cambridge, M- sachusetts, in the 1960s. However, my approach to the problems of mathem- ical physics had been shaped earlier in my time as a graduate student in the Mathematics Department at MIT. The passage of time tends merely to further enhance my appreciation of that graduate study program, where I had the b- e?t of the intensive courses from Norman Levinson, C.-C. Lin, Jurgen ? Moser, and Eric Reissner. In the case of Reissner, my years as research assistant were a formative apprenticeship one could say on the shop-?oor. The stimulus to organize my convictions in book form came from my friends at Birkh? auser Boston, and I wish to thank Ann Kostant for providing me with the opportunity and support in producing it; a special thanks goes to Edwin Beschler, formerly of Birkh? auser, for his consistent encouragement over the years. In the course of writing, I had the good-humored support and invaluable help from my one-time teacher and long-time friend, Vincent Hart. He read each chapter as it was written and his sharp eye picked up my many slips and errors. More signi?cantly, his persistent questioning on the original form of Chapter 3 forced me to address all parameter ranges and provide solution forms to cover all possibilities for the case of negative energy.General Introduction.- Lagrangian Mechanics.- The Kepler Problem.- The Euler Problem I lƒ!Copyright © 2018 - 2024 ShopSpell