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Multi-stream inflation
DOI:10.1088/1475-7516/2009/07/033.png)
Abstract
En 中文
We propose a multi-stream inflation model, which is a double field model with spontaneous breaking and restoration of an approximate symmetry. We calculate the density perturbation and non-Gaussianity in this model. We find that this model can have large, scale dependent, and probably oscillating non-Gaussianity. We also note that our model can produce features in the CMB power spectrum hemispherical power asymmetry.
Keywords:
inflation
cosmological perturbaiton theory
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