The TT, TB, EB and BB correlations in anisotropic inflation

被引:45
作者
Chen, Xingang [1 ]
Emami, Razieh [2 ]
Firouzjahi, Hassan [3 ]
Wang, Yi [4 ]
机构
[1] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA
[2] Inst Res Fundamental Sci IPM, Sch Phys, Tehran, Iran
[3] Inst Res Fundamental Sci IPM, Sch Astron, Tehran, Iran
[4] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Cambridge CB3 0WA, England
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 08期
基金
欧洲研究理事会;
关键词
inflation; gravitational waves and CMBR polarization; cosmological perturbation theory;
D O I
10.1088/1475-7516/2014/08/027
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ongoing and future experiments will measure the B-mode from different sky coverage and frequency bands, with the potential to reveal non-trivial features in polarization map. In this work we study the TT, TB, EB and BB correlations associated with the B-mode polarization of CMB map in models of charged anisotropic inflation. The model contains a chaotic-type large field complex inflaton which is charged under the U(1) gauge field. We calculate the statistical anisotropies generated in the power spectra of the curvature perturbation, the tensor perturbation and their cross-correlation. It is shown that the asymmetry in tensor power spectrum is a very sensitive probe of the gauge coupling. While the level of statistical anisotropy in temperature power spectrum can be small and satisfy the observational bounds, the interactions from the gauge coupling can induce large directional dependence in tensor modes. This will leave interesting anisotropic fingerprints in various correlations involving the B-mode polarization such as the TB cross-correlation which may be detected in upcoming Planck polarization data. In addition, the TT correlation receives an anisotropic contribution from the tensor sector which naturally decays after l greater than or similar to 100. We expect that the mechanism of using tensor sector to induce asymmetry at low l to be generic which can also be applied to address other low l CMB anomalies.
引用
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页数:36
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