The Origin of Time Asymmetry
S.W. Hawking, R. Laflamme, G.W. Lyons

TL;DR
This paper investigates the origin of the Thermodynamic Arrow of Time within the no boundary proposal, showing that density perturbations grow and create a consistent arrow throughout the universe's expansion and contraction, without reversing at maximum expansion.
Contribution
It demonstrates that density perturbations, unlike gravitational waves, lead to a persistent Thermodynamic Arrow of Time in a universe with no boundary conditions, challenging previous claims.
Findings
Density perturbations grow and become non-linear as the universe expands.
Gravitational wave perturbations remain linear and symmetric over time.
The Thermodynamic Arrow of Time does not reverse at maximum expansion.
Abstract
It is argued that the observed Thermodynamic Arrow of Time must arise from the boundary conditions of the universe. We analyse the consequences of the no boundary proposal, the only reasonably complete set of boundary conditions that has been put forward. We study perturbations of a Friedmann model containing a massive scalar field but our results should be independent of the details of the matter content. We find that gravitational wave perturbations have an amplitude that remains in the linear regime at all times and is roughly time symmetric about the time of maximum expansion. Thus gravitational wave perturbations do not give rise to an Arrow of Time. However density perturbations behave very differently. They are small at one end of the universe's history, but grow larger and become non linear as the universe gets larger. Contrary to an earlier claim, the density perturbations do…
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