Cosmological status of Lagrangian theory of density perturbations
arXiv:astro-ph/0612397 · doi:10.1134/S1063772907060017
Abstract
We show that hydrodynamical and field approaches in theory of cosmological scalar perturbations are equivalent for a single medium. We also give relations between notations introduced by V. Lukash, J. Bardeen, J. Bardeen et al. and G. Chibisov and V. Mukhanov.
8 pages, no figures, submitted to Astronomy Reports
Cited by in corpus (6)
- Hanbury Brown-Twiss interferometry and second-order correlations of inflaton quanta
- The scalar modes of the relic gravitons
- Glauber theory and the quantum coherence of curvature inhomogeneities
- Violation of consistency relations and the protoinflationary transition
- Magnetization of fluid phonons and large-scale curvature perturbations
- Squeezed relic photons beyond the horizon