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Non-linear r modes in neutron stars: a hydrodynamical limitation on r-mode amplitudes
Authors:Lap-Ming Lin  Wai-Mo Suen
Institution:Laboratoire de l'Univers et de ses Théories, Observatoire de Paris, F-92195 Meudon Cedex, France;McDonnell Centre for the Space Sciences, Department of Physics, Washington University, St Louis, MO 63130, USA;Department of Physics, The Chinese University of Hong Kong, Hong Kong, China
Abstract:
Keywords:gravitational waves  hydrodynamics  instabilities  stars: neutron  stars: rotation
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