Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data
We use combinations of ten small-scale cosmic microwave background anisotropy data sets from the UCSB South Pole 1994, ARGO, MAX 4 and 5, White Dish and SuZIE experiments to constrain cosmogonies. We consider open and spatially-flat-Lambda cold dark matter cosmogonies. Marginalizing over all paramet...
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ftcern:oai:cds.cern.ch:375612 2023-05-15T18:22:00+02:00 Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data Ratra, B Stompor, R Ganga, K Rocha, G Sugiyama, N Górski, K M 1999 http://cds.cern.ch/record/375612 eng eng http://cds.cern.ch/record/375612 astro-ph/9901014 KSU-PT-98-4 KUNS-1532 oai:cds.cern.ch:375612 Astrophysics and Astronomy 1999 ftcern 2018-07-28T03:53:13Z We use combinations of ten small-scale cosmic microwave background anisotropy data sets from the UCSB South Pole 1994, ARGO, MAX 4 and 5, White Dish and SuZIE experiments to constrain cosmogonies. We consider open and spatially-flat-Lambda cold dark matter cosmogonies. Marginalizing over all parameters but $\Omega_0$, the combined data favors an Omega_0 simeq 1 for both open and flat-Lambda models. Excluding the smallest angular scale SuZIE data, an Omega_0 simeq 0.3 (1.0) open (flat-Lambda) model is favored. Considering only multi-frequency data with error bars consistent with sample variance and noise considerations, an Omega_0 simeq 0.1 (1) open (flat-Lambda) model is favored. For both open and flat-$\Lambda$ models, after marginalizing over all the other parameters, a lower Omega_B h^2 (sim 0.005) or younger (t_0 sim 10 Gyr) universe is favored. However, the data do not rule out other values of Omega_0 in the flat-Lambda model and other values of Omega_B h^2 in both models. (abriged) Other/Unknown Material South pole CERN Document Server (CDS) Lambda ENVELOPE(-62.983,-62.983,-64.300,-64.300) South Pole |
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CERN Document Server (CDS) |
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Astrophysics and Astronomy |
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Astrophysics and Astronomy Ratra, B Stompor, R Ganga, K Rocha, G Sugiyama, N Górski, K M Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
topic_facet |
Astrophysics and Astronomy |
description |
We use combinations of ten small-scale cosmic microwave background anisotropy data sets from the UCSB South Pole 1994, ARGO, MAX 4 and 5, White Dish and SuZIE experiments to constrain cosmogonies. We consider open and spatially-flat-Lambda cold dark matter cosmogonies. Marginalizing over all parameters but $\Omega_0$, the combined data favors an Omega_0 simeq 1 for both open and flat-Lambda models. Excluding the smallest angular scale SuZIE data, an Omega_0 simeq 0.3 (1.0) open (flat-Lambda) model is favored. Considering only multi-frequency data with error bars consistent with sample variance and noise considerations, an Omega_0 simeq 0.1 (1) open (flat-Lambda) model is favored. For both open and flat-$\Lambda$ models, after marginalizing over all the other parameters, a lower Omega_B h^2 (sim 0.005) or younger (t_0 sim 10 Gyr) universe is favored. However, the data do not rule out other values of Omega_0 in the flat-Lambda model and other values of Omega_B h^2 in both models. (abriged) |
author |
Ratra, B Stompor, R Ganga, K Rocha, G Sugiyama, N Górski, K M |
author_facet |
Ratra, B Stompor, R Ganga, K Rocha, G Sugiyama, N Górski, K M |
author_sort |
Ratra, B |
title |
Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
title_short |
Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
title_full |
Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
title_fullStr |
Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
title_full_unstemmed |
Cosmic Microwave Background Anisotropy Constraints on Open and Flat-Lambda Cold Dark Matter Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data |
title_sort |
cosmic microwave background anisotropy constraints on open and flat-lambda cold dark matter cosmogonies from ucsb south pole, argo, max, white dish, and suzie data |
publishDate |
1999 |
url |
http://cds.cern.ch/record/375612 |
long_lat |
ENVELOPE(-62.983,-62.983,-64.300,-64.300) |
geographic |
Lambda South Pole |
geographic_facet |
Lambda South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://cds.cern.ch/record/375612 astro-ph/9901014 KSU-PT-98-4 KUNS-1532 oai:cds.cern.ch:375612 |
_version_ |
1766201357445890048 |