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CR geometry and twisting type N vacuum solutions

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Please use this identifier to cite or link to this item: http://hdl.handle.net/1928/21097

CR geometry and twisting type N vacuum solutions

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dc.contributor.author Zhang, Xuefeng
dc.date.accessioned 2012-08-28T18:32:33Z
dc.date.available 2012-08-28T18:32:33Z
dc.date.issued 2012-08-28
dc.date.submitted July 2012
dc.identifier.uri http://hdl.handle.net/1928/21097
dc.description.abstract In the search for vacuum solutions, with or without the cosmological constant Λ, of the Einstein field equations for Petrov type N with twisting principal null directions, the CR structures, which describe the parameter space for the geodesic congruence tangent to such null vectors, provide a useful invariant approach. Work of Hill, Lewandowski and Nurowski has laid a solid foundation for this, reducing the field equations to a set of differential equations for two functions, one real, one complex, of three variables. Under the assumption of the existence of one special Killing vector, the infinite-dimensional classical symmetries of those equations are determined and group-invariant solutions are considered. This results in a single ODE of the third order which may easily be reduced to one of the second order. A one-parameter class of power series solutions, g(w), of this second-order equation is realized, holomorphic in a neighborhood of the origin and behaving asymptotically as a simple quadratic function plus lower-order terms for large values of w, which constitutes new solutions of the twisting type N problem. The solution found by Leroy, and also later by Nurowski, is shown to be a special case in this class. Cartan’s method for determining local equivalence of CR manifolds is used to show that this class is indeed much more general. Also for the general metrics determined by this second-order ODE, two Killing vectors, including the one already assumed, can be found, both of which are inherited from symmetries of the underlying CR structures. In addition, for a special choice of a parameter, this ODE may be integrated once, to provide a first-order Abel equation. It can also determine new solutions to the field equations although no general solution has yet been found for it. en_US
dc.language.iso en_US en_US
dc.subject Einstein field equations, exact solutions, classical symmetries, CR structure, Petrov type, Abel equations en_US
dc.subject.lcsh Gravitational waves--Mathematical models.
dc.subject.lcsh Einstein field equations--Numerical solutions.
dc.subject.lcsh CR submanifolds.
dc.subject.lcsh Abel integral equations.
dc.title CR geometry and twisting type N vacuum solutions en_US
dc.type Dissertation en_US
dc.description.degree Physics en_US
dc.description.level Doctoral en_US
dc.description.department University of New Mexico. Dept. of Physics & Astronomy en_US
dc.description.advisor Finley, Daniel
dc.description.committee-member Finley, Daniel
dc.description.committee-member Boyer, Charles
dc.description.committee-member Allahverdi, Rouzbeh
dc.description.committee-member Duan, Huaiyu


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