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A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave backgroundThis 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.
Document ID
Document Type
Conference Paper
External Source(s)
Netterfield, C. B.
Ade, P. A. R.
Bock, J. J.
Bond, J. R.
Borrill, J.
Boscaleri, A.
Coble, K.
Contaldi, C. R.
Crill, B. P.
Bernardis, P. de
Farese, P.
Ganga, K.
Giacometti, M.
Hivon, E.
Hristov, V. V.
Iacoangeli, A.
Jaffe, A. H.
Jones, W. C.
Lange, A. E.
Martinis, L.
Masi, S.
Mason, P.
Mauskopf, P.
Melchiorri, A.
Montroy, T.
Date Acquired
August 23, 2013
Publication Date
July 12, 2001
Distribution Limits
BOOMERANG spectrum cosmos microwave

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