Quantum gravity effects in the CGHS model of collapse to a black hole

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1306

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DC Field	Value	Language
dc.contributor.author	Varadarajan, Madhavan	-
dc.date.accessioned	2006-06-06T06:54:12Z	-
dc.date.available	2006-06-06T06:54:12Z	-
dc.date.issued	1998-03-15	-
dc.identifier.citation	Physical Review D, 1998, Vol.57, 3463-3473	en
dc.identifier.issn	ISSN 1550-2368 (online)	-
dc.identifier.issn	1550-7998	-
dc.identifier.uri	http://hdl.handle.net/2289/1306	-
dc.description.abstract	We show that only a sector of the classical solution space of the CGHS model describes the formation of black holes through the collapse of matter. This sector has either right or left moving matter. We describe the sector which has left moving matter in canonical language. In the nonperturbative quantum theory all operators are expressed in terms of the matter field operator which is represented on a Fock space. We discuss the existence of large quantum fluctuations of the metric operator when the matter field is approximately classical. We end with some comments which may pertain to Hawking radiation in the context of the model.	en
dc.format.extent	294767 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRD/v57/p3463	en
dc.rights	(1998) by the American Physical Society	en
dc.title	Quantum gravity effects in the CGHS model of collapse to a black hole	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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