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 ΛCDM 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.

Cosmological Parameters from the 2003 Flight of BOOMERANG

NATOLI, Paolo;
2006

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 ΛCDM 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.
2006
Mactavish, C. J.; Ade, P. A. R.; Bock, J. J.; Bond, J. R.; Borrill, J; Boscaleri, A; Cabella, P; Contaldi, C. R.; Crill, B. P.; DE BERNARDIS, P; DE GASPERIS, G; DE OLIVEIRA COSTA, A; DE TROIA, G; 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, Paolo; Netterfield, C. B.; Pascale, E; Piacentini, F; Pogosyan, D; Polenta, G; Prunet, S; Ricciardi, S; Romeo, G; Ruhl, J. E.; Santini, P; Tegmark, M; Veneziani, M; Vittorio, N.
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in SFERA sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/1560250
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 169
  • ???jsp.display-item.citation.isi??? 164
social impact