Punctuated inflation and the low CMB multipoles

Details Punctuated inflation and the low CMB multipoles Punctuated inflation and the low CMB multipoles

2008-09-23

arxiv.org/abs/0809.3915v2

JCAP0901:009,2009

Astronomy and Astrophysics

Astrophysics

v1: 19 pages, 8 figures; v2: 20 pages, 8 figures, title changed, discussion and figures improved, references added, to appear

Scientific paper

10.1088/1475-7516/2009/01/009

We investigate inflationary scenarios driven by a class of potentials which are similar in form to those that arise in certain minimal supersymmetric extensions of the standard model. We find that these potentials allow a brief period of departure from inflation sandwiched between two stages of slow roll inflation. We show that such a background behavior leads to a step like feature in the scalar power spectrum. We set the scales such that the drop in the power spectrum occurs at a length scale that corresponds to the Hubble radius today--a feature that seems necessary to explain the lower power observed in the quadrupole moment of the Cosmic Microwave Background (CMB) anisotropies. We perform a Markov Chain Monte Carlo analysis to determine the values of the model parameters that provide the best fit to the recent WMAP 5-year data for the CMB angular power spectrum. We find that an inflationary spectrum with a suppression of power at large scales that we obtain leads to a much better fit (with just one extra parameter, $\chi_{\rm eff}^{2}$ improves by 6.62) of the observed data when compared to the best fit reference $\Lambda$CDM model with a featureless, power law, primordial spectrum.

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