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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1007.5148 (astro-ph)
[Submitted on 29 Jul 2010 (v1) , last revised 11 Jan 2011 (this version, v3)]

Title: Scale-dependence of Non-Gaussianity in the Curvaton Model

Title: 曲率子模型中非高斯性的尺度依赖性

Authors:Christian T. Byrnes, Kari Enqvist, Tomo Takahashi
Abstract: We investigate the scale-dependence of f_NL in the self-interacting curvaton model. We show that the scale-dependence, encoded in the spectral index n_{f_NL}, can be observable by future cosmic microwave background observations, such as CMBpol, in a significant part of the parameter space of the model. We point out that together with information about the trispectrum g_NL, the self-interacting curvaton model parameters could be completely fixed by observations. We also discuss the scale-dependence of g_NL and its implications for the curvaton model, arguing that it could provide a complementary probe in cases where the theoretical value of n_{f_NL} is below observational sensitivity.
Abstract: 我们研究了自相互作用波动子模型中f_NL的尺度依赖性。 我们表明,尺度依赖性以谱指数n_{非线性函数}的形式编码,可以通过未来的宇宙微波背景观测(如CMBpol)在模型参数空间的很大一部分中被观测到。 我们指出,结合关于四点函数g_NL的信息,自相互作用波动子模型的参数可以通过观测完全确定。 我们还讨论了g_NL的尺度依赖性及其对波动子模型的影响,并认为在理论上的n_{非线性函数}值低于观测灵敏度的情况下,它可能提供一个互补的探测手段。
Comments: 14 pages, 5 figures, Eq.(10) corrected
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO) ; High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
Cite as: arXiv:1007.5148 [astro-ph.CO]
  (or arXiv:1007.5148v3 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1007.5148
arXiv-issued DOI via DataCite
Journal reference: JCAP 1009:026,2010
Related DOI: https://doi.org/10.1088/1475-7516/2010/09/026
DOI(s) linking to related resources

Submission history

From: Tomo Takahashi [view email]
[v1] Thu, 29 Jul 2010 08:42:56 UTC (352 KB)
[v2] Mon, 27 Sep 2010 13:07:17 UTC (358 KB)
[v3] Tue, 11 Jan 2011 00:48:12 UTC (358 KB)
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