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A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background

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dc.contributor.author Netterfield, C. B. en_US
dc.contributor.author Ade, P. A. R. en_US
dc.contributor.author Bock, J. J. en_US
dc.contributor.author Bond, J. R. en_US
dc.contributor.author Borrill, J. en_US
dc.contributor.author Boscaleri, A. en_US
dc.contributor.author Coble, K. en_US
dc.contributor.author Contaldi, C. R. en_US
dc.contributor.author Crill, B. P. en_US
dc.contributor.author Bernardis, P. de en_US
dc.contributor.author Farese, P. en_US
dc.contributor.author Ganga, K. en_US
dc.contributor.author Giacometti, M. en_US
dc.contributor.author Hivon, E. en_US
dc.contributor.author Hristov, V. V. en_US
dc.contributor.author Iacoangeli, A. en_US
dc.contributor.author Jaffe, A. H. en_US
dc.contributor.author Jones, W. C. en_US
dc.contributor.author Lange, A. E. en_US
dc.contributor.author Martinis, L. en_US
dc.contributor.author Masi, S. en_US
dc.contributor.author Mason, P. en_US
dc.contributor.author Mauskopf, P. en_US
dc.contributor.author Melchiorri, A. en_US
dc.contributor.author Montroy, T. en_US
dc.contributor.author Pascale, E. en_US
dc.contributor.author Piacentini, F. en_US
dc.contributor.author Pogosyan, D. en_US
dc.contributor.author Pongetti, F. en_US
dc.contributor.author Prunet, S. en_US
dc.contributor.author Romeo, G. en_US
dc.contributor.author Ruhl, J. E. en_US
dc.contributor.author Scaramuzzi, F. en_US
dc.date.accessioned 2004-09-22T23:45:55Z
dc.date.available 2004-09-22T23:45:55Z
dc.date.issued 2001-07-12 en_US
dc.identifier.citation International Europhysics Conference on High Energy Physics en_US
dc.identifier.citation Budapest, Hungary en_US
dc.identifier.clearanceno 01-1282 en_US
dc.identifier.uri http://hdl.handle.net/2014/12912
dc.description.abstract This paper presents a measurement of the angular power spectrum of the Cosmic Microwave Background from l = 75 to l = 1025 (~10' to 5 degrees) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic-inflationary models in which the primordial plasma undergoes acoustic oscillations. en_US
dc.format.extent 19155380 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other BOOMERANG spectrum cosmos microwave en_US
dc.title A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background en_US


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