Thermal fluctuations in viscous cosmology
arXiv:1001.5152 · doi:10.1016/j.physletb.2010.03.009
Abstract
In this paper we investigate the power spectrum of thermal fluctuations in very early stage of viscous cosmology. When the state parameter as well as the viscous coefficient of a barotropic fluid is properly chosen, a scale invariant spectrum with large non-Gaussianity can be obtained. In contrast to the results previously obtained in string gas cosmology and holographic cosmology, we find the non-Gaussianity in this context can be k-independent such that it is not suppressed at large scale, which is expected to be testified in future observation.
13 pages, no figure, typos corrected, references added
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- Crossing the phantom divide with dissipative normal matter in the Israel-Stewart-Hiscock formalism
- Remarks on cosmological bulk viscosity in different epochs
- Cosmology with viscous generalized Chaplygin gas in gravity
- Quadra-Spectrum and Quint-Spectrum from Inflation and Curvaton Models
- Energy stored on a cosmological horizon and its thermodynamic fluctuations in holographic equipartition law
- Testing a dissipative kinetic k-essence model