The use of fictitious time in Lagrangian mechanics
DOI:
https://doi.org/10.31349/RevMexFisE.18.020201Keywords:
Lagrangian formulation, fictitious time, Kepler problem, Liouville systemsAbstract
We present some examples in the elementary Lagrangian formulation of classical mechanics where the introduction of a parameter in place of the time (sometimes called fictitious time or local time) decouples the equations of motion.References
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D.T. Greenwood, {it Classical Dynamics} (Prentice-Hall, Englewood Cliffs, New Jersey, 1977; reprinted by Dover, 1997), Sec. 2-3.
A.M. Perelomov, {it Integrable Systems of Classical Mechanics and Lie Algebras}, Vol. I (Birkh"auser, Basel, 1990), Sect. 2.3. doi.org/10.1007/978-3-0348-9257-5
D.C. Khandekar, S.V. Lawande, and K.V. Bhagwat, {it Path-Integral Methods and their Applications} (World Scientific, Singapore, 1993), Sec. 5.2. doi.org/10.1142/1332
G.F. Torres del Castillo, {it An Introduction to Hamiltonian Mechanics} (Springer, Cham, 2018). doi.org/10.1007/978-3-319-95225-3
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M.G. Calkin, {it Lagrangian and Hamiltonian Mechanics} (World Scientific, Singapore, 1996). doi.org/10.1142/3111
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Copyright (c) 2021 Gerardo Francisco Torres del Castillo
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