Cosmological Inflation and the delta N formalism

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dc.contributor.authorFransson, Emil
dc.contributor.departmentChalmers tekniska högskola / Institutionen för fundamental fysiksv
dc.contributor.departmentChalmers University of Technology / Department of Fundamental Physicsen
dc.date.accessioned2019-07-03T12:42:37Z
dc.date.available2019-07-03T12:42:37Z
dc.date.issued2011
dc.description.abstractIn this thesis we perform a study of cosmological inflation in the delta-N-formalism. Inflation is a period of time when the physical distances in the universe grew immensely. Most theories of inflation use one or more scalar fields to drive inflation. Through Fluctuations in these fields one can get theoretical predictions of the anisotropies in the Cosmic Microwave Background radiation by using the so called delta-N-formalism.
dc.identifier.urihttps://hdl.handle.net/20.500.12380/147805
dc.language.isoeng
dc.setspec.uppsokPhysicsChemistryMaths
dc.subjectGrundläggande vetenskaper
dc.subjectKosmologi
dc.subjectBasic Sciences
dc.subjectCosmology
dc.titleCosmological Inflation and the delta N formalism
dc.type.degreeExamensarbete för masterexamensv
dc.type.degreeMaster Thesisen
dc.type.uppsokH
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