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Observables in extended percolation models of causal set cosmology

dc.contributor.authorDowker, Fay
dc.contributor.authorSurya, Sumati
dc.date.accessioned2007-01-08T06:01:15Z
dc.date.available2007-01-08T06:01:15Z
dc.date.issued2006-02-07
dc.descriptionRestricted Access. An open access version is available at arXiv.org.en
dc.description.abstractClassical sequential growth models for causal sets provide an important step towards the formulation of a quantum causal set dynamics. The covariant observables in a class of these models known as generalized percolation have been completely characterized in terms of physically well-defined 'stem sets' and yield an insight into the nature of observables in quantum causal set cosmology. We discuss a recent extension of generalized percolation and show that the characterization of covariant observables in terms of stem sets is also complete in this extension.en
dc.format.extent127931 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationClassical and Quantum Gravity, 2006, Vol.23, p1381-1390en
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382 (Online)
dc.identifier.urihttp://hdl.handle.net/2289/1747
dc.language.isoenen
dc.publisherThe Institute of Physics Publishingen
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/23/4/018en
dc.relation.urihttp://arxiv.org/abs/gr-qc/0504069en
dc.rights(2006) by the Institute of Physicsen
dc.titleObservables in extended percolation models of causal set cosmologyen
dc.typeArticleen

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