Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
Open Access
- 10 January 2002
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 564 (2), 559-566
- https://doi.org/10.1086/324298
Abstract
Three peaks and two dips have been detected in the power spectrum of the cosmic microwave background by the BOOMERANG experiment, at l = (213), (541), (845) and l = (416), (750), respectively. Using model-independent analyses, we find that all five features are statistically significant, and we measure their location and amplitude. These are consistent with the adiabatic inflationary model. We also calculate the mean and variance of the peak and dip locations and amplitudes in a large seven-dimensional parameter space of such models, which gives good agreement with the model-independent estimates. We forecast where the next few peaks and dips should be found if the basic paradigm is correct. We test the robustness of our results by comparing Bayesian marginalization techniques on this space with likelihood maximization techniques applied to a second seven-dimensional cosmological parameter space, using an independent computational pipeline, and find excellent agreement: Ωtot = 1.02 versus 1.04 ± 0.05, Ωbh2 = 0.022 versus 0.019, and ns = 0.96 versus 0.90 ± 0.08. The determination of the best fit by the maximization procedure effectively ignores nonzero optical depth of reionization τC > 0, and the difference in primordial spectral index ns between the two methods is thus a consequence of the strong correlation of ns with the τC.This publication has 37 references indexed in Scilit:
- Cosmic Microwave Background Observables and Their Cosmological ImplicationsThe Astrophysical Journal, 2001
- Cosmological parameters from the first results of BoomerangPhysical Review D, 2001
- New constraints on inflation from the cosmic microwave backgroundPhysical Review D, 2000
- Constraints on Cosmological Parameters from MAXIMA-1The Astrophysical Journal, 2000
- MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10[arcmin]–5°The Astrophysical Journal, 2000
- General primordial cosmic perturbationPhysical Review D, 2000
- Characterizing the Peak in the Cosmic Microwave Background Angular Power SpectrumPhysical Review Letters, 2000
- A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background from [CLC][ITAL]l[/ITAL][/CLC] = 100 to 400The Astrophysical Journal, 1999
- Constraints on Cosmological Models from [ITAL]Hubble Space Telescope[/ITAL] Observations of High-[CLC][ITAL]z[/ITAL][/CLC] SupernovaeThe Astrophysical Journal, 1998
- Residual Fluctuations in the Matter and Radiation Distribution After the Decoupling EpochPhysica Scripta, 1980