Abstract
The basics of dynamical systems are reviewed: phase plane analysis and bifurcation theory. The idea of a strange attractor for ordinary differential equations is introduced, the phenomenon of fluid turbulence is discussed and the subject of stochasticity in Hamiltonian systems, and particularly in celestial mechanics, is described. The chapter finishes with a discussion of the Lorenz equations, the derivation of the Lorenz map and a simple characterisation of chaos in one-dimensional maps.
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Notes
- 1.
A nonlinear oscillator is an equation of the form \(\ddot{x}+V'(x)=0\); the quantity V(x) is called the potential (energy) on account of its rôle in the energy-like conservation law \(E=\tfrac{1}{2}\dot{x}^2+V(x)\).
- 2.
We define \([x]_+=\max (x, 0)\).
- 3.
In a nutshell: if you know precisely the state of the universe at time \(t_{0}\), together with the deterministic laws governing it, then (if you’re God) you will know the state of the future. At an atomic level, this is countermanded by the uncertainty principle, and, at a practical macroscopic level, by the subject of this book.
- 4.
Now apparently eight since the relegation of Pluto.
- 5.
Currently thought to be about ten days.
- 6.
The Boussinesq approximation neglects density variations except in the buoyancy term. It is equivalent to the assumption that \(\alpha \Delta T \ll 1\), where \(\alpha \) is thermal expansion, and \(\Delta T\) the prescribed temperature drop.
- 7.
A set M is dense in X if X is the closure of M.
- 8.
We will have plenty of discussion of manifolds later, but essentially in \({\mathbf{R}}^n\) they are simply subspaces.
- 9.
Period-doubling is discussed in Chap. 2.
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Fowler, A., McGuinness, M. (2019). Introduction. In: Chaos. Springer, Cham. https://doi.org/10.1007/978-3-030-32538-1_1
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DOI: https://doi.org/10.1007/978-3-030-32538-1_1
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