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Geometric Aspects of the Einstein Equations and Integrable Systems [electronic resource] : Proceedings of the Sixth Scheveningen Conference, Scheveningen, The Netherlands, August 26–31, 1984 / edited by R. Martini.

Contributor(s): Material type: TextTextSeries: Lecture Notes in Physics ; 239Publisher: Berlin, Heidelberg : Springer Berlin Heidelberg, 1985Description: V, 347 p. 10 illus. online resourceContent type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9783540397137
Subject(s): Additional physical formats: Printed edition:: No titleDDC classification:
  • 530.1 23
LOC classification:
  • QC19.2-20.85
Online resources:
Contents:
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.
In: Springer eBooks
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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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