Cosmological perturbations from statistical thermal fluctuations
arXiv:1302.6463 · doi:10.1103/PhysRevD.88.023517
Abstract
Cosmological perturbations due to statistical thermal fluctuations in a single fluid characterized by an arbitrary equation of state are computed. Formulas to predict the scalar and tensor perturbation spectra and nongaussianity parameters at a given temperature are derived. These results are relevant to any cosmological scenario where cosmic structures may have been seeded thermally instead of originating purely from quantum vacuum fluctuations.
13 pages, no figures. v2: references added
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- Inflation and Alternatives with Blue Tensor Spectra
- Pre-inflationary primordial perturbations
- Note on the thermodynamics and the speed of sound of a scalar field
- String-Inspired Infinite-Derivative Theories of Gravity: A Brief Overview
- Gravitational-wave background in bouncing models from semi-classical, quantum and string gravity
- Energy stored on a cosmological horizon and its thermodynamic fluctuations in holographic equipartition law
- Phase transitions during Cyclic-Inflation and Non-gaussianity
- Self-gravitating -media
- Thermal Fluctuations of Dark Matter in Bouncing Cosmology
- Perturbations in Bouncing and Cyclic Models, a General Study
- Primordial perturbations in a rainbow universe with running Newton constant
- Has inflation really solved the problems of flatness and absence of relics?
- Non-Gaussian Signatures of a Thermal Big Bang