Astrophysics
[Submitted on 1 Jun 2007 (v1), last revised 3 Jul 2008 (this version, v3)]
Title:Matching WMAP 3-yrs results with the Cosmological Slingshot Primordial Spectrum
View PDFAbstract: We consider a recently proposed scenario for the generation of primordial cosmological perturbations, the so called Cosmological Slingshot scenario. We firstly obtain a general expression for the Slingshot primordial power spectrum which extends previous results by including a blue pre-bounce residual contribution at large scales. Starting from this expression we numerically compute the CMB temperature and polarization power spectra arising from the Slingshot scenario and show that they excellently match the standard WMAP 3-years best-fit results. In particular, if the residual blue spectrum is far above the largest WMAP observed scale, the Slingshot primordial spectrum fits the data well by only fixing its amplitude and spectral index at the pivot scale k_p=10^{-3}h x Mpc^{-1}. We finally show that all possible distinctive Slingshot signatures in the CMB power spectra are confined to very low multipoles and thus very hard to detect due to large cosmic variance dominated error bars at these scales.
Submission history
From: Cristiano Germani [view email][v1] Fri, 1 Jun 2007 15:45:26 UTC (32 KB)
[v2] Mon, 1 Oct 2007 17:12:36 UTC (39 KB)
[v3] Thu, 3 Jul 2008 19:36:27 UTC (40 KB)
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