Observables in extended percolation models of causal set cosmology

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1747

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DC Field	Value	Language
dc.contributor.author	Dowker, Fay	-
dc.contributor.author	Surya, Sumati	-
dc.date.accessioned	2007-01-08T06:01:15Z	-
dc.date.available	2007-01-08T06:01:15Z	-
dc.date.issued	2006-02-07	-
dc.identifier.citation	Classical and Quantum Gravity, 2006, Vol.23, p1381-1390	en
dc.identifier.issn	0264-9381	-
dc.identifier.issn	1361-6382 (Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/1747	-
dc.description	Restricted Access. An open access version is available at arXiv.org.	en
dc.description.abstract	Classical 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.extent	127931 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The Institute of Physics Publishing	en
dc.relation.uri	http://dx.doi.org/10.1088/0264-9381/23/4/018	en
dc.relation.uri	http://arxiv.org/abs/gr-qc/0504069	en
dc.rights	(2006) by the Institute of Physics	en
dc.title	Observables in extended percolation models of causal set cosmology	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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