Derives perturbation equations for Bianchi spacetimes in Newtonian gauge and computes density contrasts for EdS and Bianchi I models.
Mukhanov,Physical Foundations of Cosmology(Cambridge University Press, 2005)
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
A vacuum-decay model generates primordial curvature perturbations from spatially correlated stochastic noise rather than inflaton fluctuations, solving horizon and flatness problems with zero tensor-to-scalar ratio.
citing papers explorer
-
Fundamental Cosmic Anisotropy and its Ramifications II: Perturbations in Bianchi spacetimes, and fixed in the Newtonian gauge
Derives perturbation equations for Bianchi spacetimes in Newtonian gauge and computes density contrasts for EdS and Bianchi I models.
-
The Noise of Vacuum
A vacuum-decay model generates primordial curvature perturbations from spatially correlated stochastic noise rather than inflaton fluctuations, solving horizon and flatness problems with zero tensor-to-scalar ratio.