Long wavelength limit of evolution of cosmological perturbations in the universe where scalar fields and fluids coexist
Author:
Publisher
Elsevier BV
Subject
Nuclear and High Energy Physics
Reference33 articles.
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1. Construction and applications of the manifestly gauge invariant expressions of the solutions of the cosmological perturbation theory;Annals of Physics;2018-07
2. Constraints on neutrino density and velocity isocurvature modes from WMAP-9 data;Physical Review D;2013-09-27
3. CONSTRAINTS ON SCALAR AND TENSOR PERTURBATIONS IN PHENOMENOLOGICAL AND TWO-FIELD INFLATION MODELS: BAYESIAN EVIDENCES FOR PRIMORDIAL ISOCURVATURE AND TENSOR MODES;The Astrophysical Journal;2012-06-25
4. Manifestly gauge invariant theory of the nonlinear cosmological perturbations in the leading order of the gradient expansion;Physical Review D;2011-07-05
5. Long wavelength limit of evolution of nonlinear cosmological perturbations;Physical Review D;2008-11-14
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