![Geometric Aspects of the Einstein Equations and Integrable Systems [electronic resource] : Proceedings of the Sixth Scheveningen Conference, Scheveningen, The Netherlands, August 26–31, 1984 /](/search/themes/bootstrap3/images/libros.png)
Geometric Aspects of the Einstein Equations and Integrable Systems [electronic resource] : Proceedings of the Sixth Scheveningen Conference, Scheveningen, The Netherlands, August 26–31, 1984 /
Exact solutions in gauge theory, general relativity, and their supersymmetric extensions -- Symmetries and solutions of the einstein equations -- Superposition of solutions in general relativity -- Gauge fields, gravitation and Kaluza-Klein theory -- Gravitational shock waves -- Soliton surfaces and their applications (soliton geometry from spectral problems) -- Completely integrable systems of evolution equations on KAC moody lie algebras -- Integrable lattice systems in two and three dimensions -- Isovectors and prolongation structures by Vessiot's vector field formulation of partial differential equations -- Hamiltonian flow on an energy surface: 240 years after the euler-maupertuis principle.
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| Main Authors: | , |
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| Format: | Texto biblioteca |
| Language: | eng |
| Published: |
Berlin, Heidelberg : Springer Berlin Heidelberg,
1985
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| Subjects: | Physics., Theoretical, Mathematical and Computational Physics., |
| Online Access: | http://dx.doi.org/10.1007/3-540-16039-6 |
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| Summary: | Exact solutions in gauge theory, general relativity, and their supersymmetric extensions -- Symmetries and solutions of the einstein equations -- Superposition of solutions in general relativity -- Gauge fields, gravitation and Kaluza-Klein theory -- Gravitational shock waves -- Soliton surfaces and their applications (soliton geometry from spectral problems) -- Completely integrable systems of evolution equations on KAC moody lie algebras -- Integrable lattice systems in two and three dimensions -- Isovectors and prolongation structures by Vessiot's vector field formulation of partial differential equations -- Hamiltonian flow on an energy surface: 240 years after the euler-maupertuis principle. |
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