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Cosmological Parameters from the 2003 Flight of BOOMERANG

MacTavish, C. J., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C. R., Brill, B. P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., de Troia, D, di Stefano, G., Hivon, E., Jaffe, A. H., Jones, W. C., Kisner, T. S., Lange, A. E., Lewis, A. M., Masi, S., Mauskopf, P. D., Melchiorri, A., Montroy, T. E., Natoli, P., Netterfield, C. B., Pascale, Enzo ORCID: https://orcid.org/0000-0002-3242-8154, Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S,, Ricciardi, S., Romeo, G., Ruhl, J. E., Santini, P., Tegmark, M., Veneziani, M. and Vittorio, N. 2006. Cosmological Parameters from the 2003 Flight of BOOMERANG. The Astrophysical Journal 647 (2) , pp. 799-812. 10.1086/505558

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Abstract

We present the cosmological parameters from the CMB intensity and polarization power spectra of the 2003 Antarctic flight of the BOOMERANG telescope. The BOOMERANG data alone constrain the parameters of the ?CDM model remarkably well and are consistent with constraints from a multiexperiment combined CMB data set. We add LSS data from the 2dF and SDSS redshift surveys to the combined CMB data set and test several extensions to the standard model including running of the spectral index, curvature, tensor modes, the effect of massive neutrinos, and an effective equation of state for dark energy. We also include an analysis of constraints to a model that allows a CDM isocurvature admixture

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QC Physics
Uncontrolled Keywords: Cosmic microwave background ; Cosmological parameters ; Polarization
ISSN: 0004-637X
Last Modified: 17 Oct 2022 08:57
URI: https://orca.cardiff.ac.uk/id/eprint/1599

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