Orbital stability via the energy-momentum method: the case of higher   dimensional symmetry groups
  We consider the orbital stability of relative equilibria of Hamiltonian dynamical systems on Banach spaces, in the presence of a multi-dimensional invariance group for the dynamics. We prove a persistence result for such relative equilibria, present a generalization of the Vakhitov-Kolokolov slope condition to this higher dimensional setting, and show how it allows to prove the local coercivity of the Lyapunov function, which in turn implies orbital stability. The method is applied to study the orbital stability of relative equilibria of nonlinear Schr{\"o}dinger and Manakov equations. We provide a comparison of our approach to the one by Grillakis-Shatah-Strauss. 
Stephan De Bievre (LPP, MEPHYSTO), Simona Rota Nodari (IMB)
math.AP math.DS math.SG