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Dark energy and cosmic microwave background bispectrum | | Licia Verde
; David N. Spergel
; | | Date: |
10 Aug 2001 | | Journal: | Phys.Rev. D65 (2002) 043007 | | Subject: | astro-ph | | Affiliation: | Princeton & Rutgers), David N. Spergel (Princeton & IAS | | Abstract: | We compute the cosmic microwave background bispectrum arising from the cross-correlation of primordial, lensing and Rees-Sciama signals. The amplitude of the bispectrum signal is sensitive to the matter density parameter, Omega_0, and the equation of state of the dark energy, which we parameterize by w_Q. We conclude that the dataset of the Atacama Cosmology Telescope, combined with MAP 2-year data or the Planck data set alone will allow us to break the degeneracy between Omega_0 and w_Q that arises from the analysis of CMB power spectrum. In particular a joint measurement of Omega_0 and w_Q with 10% and 30% error on the two parameters respectively, at the 90% confidence level can realistically be achieved. | | Source: | arXiv, astro-ph/0108179 | | Services: | Forum | Review | PDF | Favorites | |
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