The propagation of nonlinear dispersive gravity waves in an inviscid irrotational fluid can be described by a Hamiltonian system. The canonical equations contain a boundary integral which is computationally expensive. However, for fairly low and fairly long waves an approximation can be made that gi
β¦ LIBER β¦
A Hamiltonian approach to the strong gravity limit
β Scribed by J. N. Goldberg
- Publisher
- Springer US
- Year
- 1988
- Tongue
- English
- Weight
- 426 KB
- Volume
- 20
- Category
- Article
- ISSN
- 0001-7701
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We show that the finite difference BΓ€cklund formula for the SchrΓΆdinger Hamiltonians is a particular element of the transformation group on the set of Riccati equations considered by two of us in a previous paper. Then, we give a group theoretical explanation to the problem of Hamiltonians related b