To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.

Jaffe, A., Ade, P., Balbi, A., Bock, J., Bond, J., Borrill, J., et al. (2001). Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations. PHYSICAL REVIEW LETTERS, 86(16), 3475-3479 [10.1103/PhysRevLett.86.3475].

Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations

BALBI, AMEDEO;
2001-01-01

Abstract

To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.
2001
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Acoustic variables measurement; Anisotropy; Band structure; Calculations; Charged particles; Galaxies; Microwaves; Oscillations; Probability density function; Relativity; Signal to noise ratio; Acoustic oscillations; Baryon; Cosmic microwave background; Cosmology; Nonbaryonic dark matter; Astrophysics
Jaffe, A., Ade, P., Balbi, A., Bock, J., Bond, J., Borrill, J., et al. (2001). Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations. PHYSICAL REVIEW LETTERS, 86(16), 3475-3479 [10.1103/PhysRevLett.86.3475].
Jaffe, A; Ade, P; Balbi, A; Bock, J; Bond, J; Borrill, J; Boscaleri, A; Coble, K; Crill, B; de Bernardis, P; Farese, P; Ferreira, P; Ganga, K; Giacometti, M; Hanany, S; Hivon, E; Hristov, V; Iacoangeli, A; Lange, A; Lee, A; Martinis, L; Masi, S; Mauskopf, P; Melchiorri, A; Montroy, T; Netterfield, C; Oh, S; Pascale, E; Piacentini, F; Pogosyan, D; Prunet, S; Rabii, B; Rao, S; Richards, P; Romeo, G; Ruhl, J; Scaramuzzi, F; Sforna, D; Smoot, G; Stompor, R; Winant, C; Wu, J
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/53982
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