THIRD QUANTIZATION IN BERGMANN-WAGONER THEORY

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Campo DC	Valor	Lengua/Idioma
dc.creator	SÁNCHEZ, RUBÉN	-
dc.creator	MORA, CÉSAR	-
dc.date	2012-03-28T19:35:03Z	-
dc.date	2012-03-28T19:35:03Z	-
dc.date	2008-04	-
dc.date.accessioned	2013-01-16T15:05:13Z	-
dc.date.available	2013-01-16T15:05:13Z	-
dc.date.issued	2013-01-16	-
dc.identifier	MEXICO, CITY	-
dc.identifier	1555-5534	-
dc.identifier	http://hdl.handle.net/123456789/901	-
dc.identifier.uri	http://www.repositoriodigital.ipn.mx/handle/123456789/11397	-
dc.description	The Wheeler-DeWitt (WDW) equation is a result of quantization of a geometry and matter ( SECOND QUANTIZATION OF GRAVITY), in this paper we consider the third quantization of a solvable inflationary universe model, i.e..by analogy with the quantum field theory, it can be done the second quantization of the universe wavefunction expanding it on the creation and annihilation operators (third quantization) [1].	-
dc.description	Centro de Investigación en Ciencia Aplicada y Tecnología Avanzada, Instituto Politécnico Nacional	-
dc.language	en	-
dc.publisher	PROGRESS IN PHYSICS	-
dc.relation	PROGRESS IN PHYSICS;Vol. 2 April 2008	-
dc.title	THIRD QUANTIZATION IN BERGMANN-WAGONER THEORY	-
dc.type	Article	-
Aparece en las colecciones:	Doctorado

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