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• W1780340181 abstract "A peak has been unambiguously detected in the cosmic microwave background angular spectrum. Here we characterize its properties with fits to phenomenological models. We find that the TOCO and BOOM/NA data determine the peak location to be in the range 175-243 and 151-259, respectively (at 95% confidence) and determine the peak amplitude to be between approximately 70 and 90 &mgr;K. The peak shape is consistent with inflation-inspired flat, cold dark matter plus cosmological constant models of structure formation with adiabatic, nearly scale invariant initial conditions. It is inconsistent with open models and presents a great challenge to defect models." @default.
• W1780340181 created "2016-06-24" @default.
• W1780340181 creator A5042907865 @default.
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• W1780340181 date "2000-08-14" @default.
• W1780340181 modified "2023-09-27" @default.
• W1780340181 title "Characterizing the Peak in the Cosmic Microwave Background Angular Power Spectrum" @default.
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• W1780340181 doi "https://doi.org/10.1103/physrevlett.85.1366" @default.
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