Cosmic microwave background anisotropies

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2691

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DC Field	Value	Language
dc.contributor.author	Subrahmanyan, Ravi	-
dc.date.accessioned	2007-06-11T09:06:26Z	-
dc.date.available	2007-06-11T09:06:26Z	-
dc.date.issued	1997	-
dc.identifier.citation	Proceedings of the symposium on the early universe, IIT, Madras, 1994, Hadronic Press, 1997, p1	en
dc.identifier.uri	http://hdl.handle.net/2289/2691	-
dc.description	Restricted Access.	en
dc.description.abstract	Anisotropies in the Cosmic Microwave Background are a probe of the spectrum of density perturbations in the early universe and of the astrophysical and dynamical evolution that caused the formation of galaxies and the present day observed structure in the universe. Theory of the coupling of the perturbations to the radiation predicts characteristic features in the spectrum of the anisotropies. Experiments measure the anisotropy power as viewed through spectral windows. We review the current status, of the predictions of the anisotropy power spectrum and the constraints on the spectrum from observations.	en
dc.format.extent	358726 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Hadronic Press	en
dc.rights	1997 Hadronic Press	en
dc.title	Cosmic microwave background anisotropies	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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