Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3255
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dc.contributor.authorVaradarajan, Madhavan-
dc.date.accessioned2007-07-16T09:46:22Z-
dc.date.available2007-07-16T09:46:22Z-
dc.date.issued2000-01-
dc.identifier.citationClassical and Quantum Gravity, 2000, Vol.17, p189-199en
dc.identifier.issn0264-9381-
dc.identifier.urihttp://hdl.handle.net/2289/3255-
dc.descriptionRestricted Access.en
dc.description.abstractEvery (one-polarization) cylindrical wave solution of vacuum general relativity is completely determined by a corresponding axisymmetric solution to the free scalar wave equation on an auxiliary (2 + 1)-dimensional flat spacetime. The physical metric at radius R is determined by the energy, gamma (R ), of the scalar field in a box (in the flat spacetime) of radius R . In a recent work, among other important results, Ashtekar and Pierri have introduced a strategy to study the quantum geometry in this system, through a regularized quantum counterpart of gamma (R ). We show that this regularized object is a densely defined symmetric operator, thereby correcting an error in their proof of this result. We argue that it admits a self-adjoint extension and show that the operator, unlike its classical counterpart, is not positive.en
dc.format.extent168028 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIOP Publishing Ltd.en
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/17/1/313en
dc.rights2000 IOP Publishing Ltd.en
dc.titleOn the metric operator for quantum cylindrical wavesen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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