Lagrange stability

Lagrange stability is a concept in the stability theory of dynamical systems, named after Joseph-Louis Lagrange.

For any point in the state space, x M {\displaystyle x\in M} in a real continuous dynamical system ( T , M , Φ ) {\displaystyle (T,M,\Phi )} , where T {\displaystyle T} is R {\displaystyle \mathbb {R} } , the motion Φ ( t , x ) {\displaystyle \Phi (t,x)} is said to be positively Lagrange stable if the positive semi-orbit γ x + {\displaystyle \gamma _{x}^{+}} is compact. If the negative semi-orbit γ x {\displaystyle \gamma _{x}^{-}} is compact, then the motion is said to be negatively Lagrange stable. The motion through x {\displaystyle x} is said to be Lagrange stable if it is both positively and negatively Lagrange stable. If the state space M {\displaystyle M} is the Euclidean space R n {\displaystyle \mathbb {R} ^{n}} , then the above definitions are equivalent to γ x + , γ x {\displaystyle \gamma _{x}^{+},\gamma _{x}^{-}} and γ x {\displaystyle \gamma _{x}} being bounded, respectively.

A dynamical system is said to be positively-/negatively-/Lagrange stable if for each x M {\displaystyle x\in M} , the motion Φ ( t , x ) {\displaystyle \Phi (t,x)} is positively-/negatively-/Lagrange stable, respectively.

References

  • Elias P. Gyftopoulos, Lagrange Stability and Liapunov's Direct Method. Proc. of Symposium on Reactor Kinetics and Control, 1963. (PDF)
  • Bhatia, Nam Parshad; Szegő, Giorgio P. (2002). Stability theory of dynamical systems. Springer. ISBN 978-3-540-42748-3.
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Joseph-Louis Lagrange


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