Frontiers of Inflationary Cosmology

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3168

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DC Field	Value	Language
dc.creator	Brandenberger Robert H.	-
dc.date	2001	-
dc.date.accessioned	2013-05-30T00:46:11Z	-
dc.date.available	2013-05-30T00:46:11Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000200003	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=2&spage=131	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3168	-
dc.description	After a brief review the theory of cosmological perturbations, I highlight some recent progress in the area of reheating in inflationary cosmology, focusing in particular on parametric amplification of super-Hubble cosmological fluctuations, and on the role of noise in the resonance dynamics (yielding a new proof of Anderson localization). I then discuss several important conceptual problems for the current realizations of inflation based on fundamental scalar matter fields, and review some new approaches at solving these problems.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Frontiers of Inflationary Cosmology	-
Appears in Collections:	Physics and Astronomy

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