A comprehensive Mukhanov chart PDF will also extend into the radiation and matter-dominated eras. After inflation ends, the Hubble radius grows. At a much later time, the perturbation's wavelength re-enters the horizon, shown on the chart as a second crossing point, leading to gravitational collapse.
Mukhanov chart PDF, Mukhanov-Sasaki variable, primordial density perturbations, inflationary cosmology, comoving curvature perturbation, physical foundations of cosmology, quantum fluctuations in curved spacetime. mukhanov chart pdf
(radiation/matter domination):
Md=α⋅w⋅d12cap M sub d equals alpha center dot w center dot d sub 1 squared : The coefficient from Mukhanov’s chart. : The local pressure at the base plate. : The length of the free edge or the panel dimension. A comprehensive Mukhanov chart PDF will also extend
The typically visualizes the evolution of these perturbations across cosmic time, specifically plotting the comoving curvature perturbation (often denoted as ( \mathcalR )) or the Mukhanov variable ( v ) against time or scale factor. : The length of the free edge or the panel dimension