Abstract
In the previous chapter, we returned to the equation of the forced pendulum
assuming now that the forcing term e: R → R is a continuous T-periodic function, but not necessarily an odd function as it was in Chapter 5. It will be convenient to remember that \( a = \tfrac{g} {\ell } \) where g is the gravitational constant and l is the length of the pendulum, and therefore a > 0.
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© 2004 Springer Science+Business Media New York
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Brown, R.F. (2004). The Pendulum Swings Back. In: A Topological Introduction to Nonlinear Analysis. Birkhäuser, Boston, MA. https://doi.org/10.1007/978-0-8176-8124-1_13
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DOI: https://doi.org/10.1007/978-0-8176-8124-1_13
Publisher Name: Birkhäuser, Boston, MA
Print ISBN: 978-0-8176-3258-8
Online ISBN: 978-0-8176-8124-1
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