CMB probes on the correlated axion isocurvature perturbation

CMB probes on the correlated axion isocurvature perturbation
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DOI:
10.1088/1475-7516/2015/03/026
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发表时间:
2014-11
影响因子:
6.4
通讯作者:
K. Kadota;Jinn-Ouk Gong;K. Ichiki;T. Matsubara
K. Kadota;Jinn-Ouk Gong;K. Ichiki;T. Matsubara
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
K. Kadota;Jinn-Ouk Gong;K. Ichiki;T. Matsubara

文献摘要

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我们探讨了暴胀子和类轴子场之间引力耦合的可能宇宙学后果。鉴于即将到来的宇宙微波背景(CMB)的偏振和透镜数据,我们研究的曲率和轴子等曲率扰动之间的互相关的CMB数据的敏感性。通过一个具体的例子,说明了尺度相关功率谱对轴子参数的明显依赖性。
We explore the possible cosmological consequence of the gravitational coupling between the inflaton and axion-like fields. In view of the forthcoming cosmic microwave background (CMB) polarization and lensing data, we study the sensitivity of the CMB data on the cross-correlation between the curvature and axion isocurvature perturbations. Through a concrete example, we illustrate the explicit dependence of the scale dependent cross-correlation power spectrum on the axion parameters.