The microcanonical thermodynamics of finite systems: The microscopic origin of condensation and phase separations; and the conditions for heat flow from lower to higher temperatures
D.H.E.Gross, J.F.Kenney

TL;DR
This paper explores how microcanonical thermodynamics applies to finite and self-gravitating systems, revealing that entropy convexity and heat flow directions can differ from classical expectations, especially during phase separation.
Contribution
It demonstrates the microscopic origin of entropy convexity during phase separation and challenges traditional views on heat flow and temperature in small systems.
Findings
Entropy becomes convex at phase separation.
Heat can flow from colder to hotter regions in certain conditions.
Standard thermodynamic assumptions may not hold for finite systems.
Abstract
Microcanonical thermodynamics allows the application of statistical mechanics both to finite and even small systems and also to the largest, self-gravitating ones. However, one must reconsider the fundamental principles of statistical mechanics especially its key quantity, entropy. Whereas in conventional thermostatistics, the homogeneity and extensivity of the system and the concavity of its entropy are central conditions, these fail for the systems considered here. For example, at phase separation, the entropy, S(E), is necessarily convex to make exp[S(E)-E/T] bimodal in E. Particularly, as inhomogeneities and surface effects cannot be scaled away, one must be careful with the standard arguments of splitting a system into two subsystems, or bringing two systems into thermal contact with energy or particle exchange. Not only the volume part of the entropy must be considered. As will be…
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