Arrow of time in dissipationless cosmology
Varun Sahni, Yuri Shtanov, Aleksey Toporensky

TL;DR
This paper shows that a cosmological arrow of time can emerge in dissipationless systems through attractors and hysteresis effects, challenging the idea that entropy production is necessary for time asymmetry.
Contribution
It introduces a mechanism for the arrow of time in cyclic cosmology without entropy production, based on attractors and hysteresis in scalar-field driven models.
Findings
Dissipationless systems can exhibit a preferred time direction via attractors.
Hysteresis in cyclic cosmology causes an arrow of time without entropy increase.
A cyclic universe can evolve from a single past to two futures with opposite arrows of time.
Abstract
It is generally believed that a cosmological arrow of time must be associated with entropy production. Indeed, in his seminal work on cyclic cosmology, Tolman introduced a viscous fluid in order to make successive expansion/contraction cycles larger than previous ones, thereby generating an arrow of time. However, as we demonstrate in this letter, the production of entropy is not the only means by which a cosmological arrow of time may emerge. Remarkably, systems which are dissipationless may nevertheless demonstrate a preferred direction of time provided they possess attractors. An example of a system with well defined attractors is scalar-field driven cosmology. In this case, for a wide class of potentials (especially those responsible for inflation), the attractor equation of state during expansion can have the form , and during contraction . If the…
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