Ruling out the power-law form of the scalar primordial spectrum

被引：30

作者：

Hazra, Dhiraj Kumar ^{[1
]}

Shafieloo, Arman ^{[1
,2
]}

Smoot, George F. ^{[3
,4
,5
]}

Starobinsky, Alexei A. ^{[6
]}

机构：

[1] Asia Pacific Ctr Theoret Phys, Pohang 790784, Gyeongbuk, South Korea

[2] POSTECH, Dept Phys, Pohang 790784, Gyeongbuk, South Korea

[3] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[4] Ewha Womans Univ, Inst Early Universe, Seoul 120750, South Korea

[5] Univ Paris Diderot, APC, Paris Ctr Cosmol Phys, Paris, France

[6] RAS, LD Landau Theoret Phys Inst, Moscow 119334, Russia

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 06期

基金：

新加坡国家研究基金会;

关键词：

inflation; physics of the early universe; gravitaional waves and CMBR polarization; cosmological perturbation theory; PROBE WMAP OBSERVATIONS; OPEN INFLATION; PLANCK; RADIATION; UNIVERSE; MODEL; CMB;

D O I：

10.1088/1475-7516/2014/06/061

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Combining Planck CMB temperature 111 and BICEP2 B-mode polarization data [2, 3] we show qualitatively that, assuming inflationary consistency relation, the power-law form of the scalar primordial spectrum is ruled out at more than :3 sigma CL. This is an important finding, since the power-law form of the scalar primordial spectrum is one of the main assumptions of concordance model of cosmology and also a direct prediction of many inflationary scenarios. We show that a break or step in the form of the primordial scalar perturbation spectrum, similar to what we studied recently analyzing Planck data [4], can address both Planck and BICEP2 results simultaneously. Our findings also indicate that the data may require more flexibilities than what running of scalar spectral index can provide. Finally we show that an inflaton potential, originally appeared in [5], can generate both the step and the break model of scalar primordial spectrum in two different limits. The discussed potential is found to be favored by Planck data but marginally disfavored by BICEP2 results as it produces slightly lower amplitude of tensor primordial spectrum. Hence, if the tensor-to-scalar ratio (r) quoted by BICEP2 persists, it is of importance that we generate inflationary models with large r and at the same time provide suppression in scalar primordial spectrum at large scales.

引用

页数：19

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