Cosmological perturbations: Vorticity, isocurvature and magnetic fields
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Publication:2940688
DOI10.1142/S0218271814300249zbMath1303.83043arXiv1409.4721MaRDI QIDQ2940688
Publication date: 20 January 2015
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1409.4721
Relativistic cosmology (83F05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Classical and relativistic thermodynamics (80A10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (2)
Perturbations of a class of locally rotationally symmetric cosmologies with applications to dissipative fluids ⋮ Intrinsic entropy perturbations from the dark sector
Cites Work
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- Cosmological Inflation and Large-Scale Structure
- Evolution of second-order cosmological perturbations
- Vorticity production through rotation, shear, and baroclinicity
- Cosmological Constraints on Isocurvature and Tensor Perturbations
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- A general proof of the conservation of the curvature perturbation
- Generating the curvature perturbation without an inflaton
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