Hints of Isocurvature Perturbations in the Cosmic Microwave Background
Nov, 2006
4 pages
Published in:
- JCAP 09 (2007) 008
e-Print:
- astro-ph/0611917 [astro-ph]
Report number:
- HIP-2006-52-TH,
- ICG-06-43
View in:
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Abstract: (arXiv)
The improved data on the cosmic microwave background (CMB) anisotropy allow a better determination of the adiabaticity of the primordial perturbation. Interestingly, we find that recent CMB data seem to favor a contribution of a primordial isocurvature mode where the entropy perturbation is positively correlated with the primordial curvature perturbation and has a large spectral index (niso ~ 3). With 4 additional parameters we obtain a better fit to the CMB data by Delta chi^2 = 9.7 compared to an adiabatic model. For this best-fit model the nonadiabatic contribution to the CMB temperature variance is 4%. According to a Markov Chain Monte Carlo analysis the nonadiabatic contribution is positive at more than 95% C.L. The exact C.L. depends somewhat on the choice of priors, and we discuss the effect of different priors as well as additional cosmological data.References(35)
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