Cosmological Inflation and the N-formalism

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dc.contributor.authorFransson, Emil L.A.
dc.contributor.departmentChalmers tekniska högskola / Institutionen för fundamental fysiksv
dc.contributor.departmentChalmers University of Technology / Department of Fundamental Physicsen
dc.date.accessioned2019-07-03T13:11:06Z
dc.date.available2019-07-03T13:11:06Z
dc.date.issued2011
dc.description.abstractIn this thesis we perform a study of cosmological inflation in the 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 N-formalism.
dc.identifier.urihttps://hdl.handle.net/20.500.12380/179098
dc.language.isoeng
dc.setspec.uppsokPhysicsChemistryMaths
dc.subjectFysik
dc.subjectPhysical Sciences
dc.titleCosmological Inflation and the N-formalism
dc.type.degreeExamensarbete för masterexamensv
dc.type.degreeMaster Thesisen
dc.type.uppsokH
local.programmeApplied physics (MPAPP), MSc
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