Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations

Recent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE-DMR, provide consistent and high signal-to-noise measurements of the CMB power spectrum at spherical harmonic multipole bands over $2<\ell\lta800$. Analysis of the combined data yields 68% (95%) confidence limits on the t...

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Main Authors: Jaffe, A, Ade, P, Balbi, A, Bock, J, Bond, JR, Borrill, J, Boscaleri, A, Coble, K, Crill, B, 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
Format: Journal article
Published: 2000
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author Jaffe, A
Ade, P
Balbi, A
Bock, J
Bond, JR
Borrill, J
Boscaleri, A
Coble, K
Crill, B
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
author_facet Jaffe, A
Ade, P
Balbi, A
Bock, J
Bond, JR
Borrill, J
Boscaleri, A
Coble, K
Crill, B
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
author_sort Jaffe, A
collection OXFORD
description Recent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE-DMR, provide consistent and high signal-to-noise measurements of the CMB power spectrum at spherical harmonic multipole bands over $2<\ell\lta800$. Analysis of the combined data yields 68% (95%) confidence limits on the total density, $\Omega_{\rm {tot}}\simeq 1.11 \pm 0.07 (^{+0.13}_{-0.12})$, the baryon density, $\Omega_b h^2\simeq 0.032^{+0.005}_{-0.004} (^{+0.009}_{-0.008})$, and the scalar spectral tilt, $n_s\simeq1.01^{+0.09}_{-0.07} (^{+0.17}_{-0.14})$. These data are consistent with inflationary initial conditions for structure formation. Taken together with other cosmological observations, they imply the existence of both non-baryonic dark matter and dark energy in the universe.
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spelling oxford-uuid:78aa7393-7678-4a44-a300-060f868450ea2022-03-26T20:32:16ZCosmology from Maxima-1, Boomerang and COBE/DMR CMB ObservationsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:78aa7393-7678-4a44-a300-060f868450eaSymplectic Elements at Oxford2000Jaffe, AAde, PBalbi, ABock, JBond, JRBorrill, JBoscaleri, ACoble, KCrill, BBernardis, PFarese, PFerreira, PGanga, KGiacometti, MHanany, SHivon, EHristov, VIacoangeli, ALange, ALee, AMartinis, LMasi, SMauskopf, PMelchiorri, AMontroy, TRecent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE-DMR, provide consistent and high signal-to-noise measurements of the CMB power spectrum at spherical harmonic multipole bands over $2<\ell\lta800$. Analysis of the combined data yields 68% (95%) confidence limits on the total density, $\Omega_{\rm {tot}}\simeq 1.11 \pm 0.07 (^{+0.13}_{-0.12})$, the baryon density, $\Omega_b h^2\simeq 0.032^{+0.005}_{-0.004} (^{+0.009}_{-0.008})$, and the scalar spectral tilt, $n_s\simeq1.01^{+0.09}_{-0.07} (^{+0.17}_{-0.14})$. These data are consistent with inflationary initial conditions for structure formation. Taken together with other cosmological observations, they imply the existence of both non-baryonic dark matter and dark energy in the universe.
spellingShingle Jaffe, A
Ade, P
Balbi, A
Bock, J
Bond, JR
Borrill, J
Boscaleri, A
Coble, K
Crill, B
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
Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title_full Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title_fullStr Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title_full_unstemmed Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title_short Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
title_sort cosmology from maxima 1 boomerang and cobe dmr cmb observations
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