A measurement of $\Omega$ from the North American test flight of BOOMERANG

We use the angular power spectrum of the Cosmic Microwave Background, measured during the North American test flight of the BOOMERANG experiment, to constrain the geometry of the universe. Within the class of Cold Dark Matter models, we find that the overall fractional energy density of the universe...

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Detalles Bibliográficos
Autores principales: Melchiorri, A., Ade, P.A.R., de Bernardis, P., Bock, J.J., Borrill, J., Boscaleri, A., Crill, B.P., De Troia, G., Farese, P., Ferreira, P.G., Ganga, K., de Gasperis, G., Giacometti, M., Hristov, V.V., Jaffe, Andrew H., Lange, Andrew E., Masi, S., Mauskopf, P.D., Miglio, L., Netterfield, C.B., Pascale, E., Piacentini, F., Romeo, G., Ruhl, J.E., Vittorio, N.
Lenguaje:eng
Publicado: 1999
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1086/312744
http://cds.cern.ch/record/409319

Internet

https://dx.doi.org/10.1086/312744
http://cds.cern.ch/record/409319

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