Multi-field inflation with random potentials: field dimension, feature scale and non-Gaussianity
Multi-field inflation with random potentials: field dimension, feature scale and non-Gaussianity
复制标题
具有随机势的多场膨胀:场维数、特征尺度和非高斯性
DOI:
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发表时间:
2011
期刊:
影响因子:
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通讯作者:
A. Liddle
中科院分区:
文献类型:
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作者:
J. Frazer;A. Liddle
We explore the super-horizon evolution of the two-point and three-point correlation functions of the primordial density perturbation in randomly-generated multi-field potentials. We use the Transport method to evolve perturbations and give full evolutionary histories for observables. Identifying the separate universe assumption as being analogous to a geometrical description of light rays, we give an expression for the width of the bundle, thereby allowing us to monitor evolution towards the adiabatic limit, as well as providing a useful means of understanding the behaviour in fNL. Finally, viewing our random potential as a toy model of inflation in the string landscape, we build distributions for observables by evolving trajectories for a large number of realisations of the potential and comment on the prospects for testing such models. We find the distributions for observables to be insensitive to the number of fields over the range 2 to 6, but that these distributions are highly sensitive to the scale of features in the potential. Most sensitive to the scale of features is the spectral index, with more than an order of magnitude increase in the dispersion of predictions over the range of feature scales investigated. Least sensitive was the non-Gaussianity parameter fNL, which was consistently small; we found no examples of realisations whose non-Gaussianity is capable of being observed by any planned experiment.
影响因子:
8.7
作者:
Komatsu, E.;Smith, K. M.;Wright, E. L.
通讯作者:
Wright, E. L.