# Flux and storage of energy in non-equilibrium, stationary states

**Authors:** Robert Ho{\l}yst, Anna Macio{\l}ek, Yirui Zhang, Marek Litniewski,, Piotr Knycha{\l}a, Maciej Kasprzak, Michal Banaszak

arXiv: 1902.10013 · 2019-04-24

## TL;DR

This paper investigates the energy storage and transfer in non-equilibrium stationary states of ideal gas and Lennard-Jones fluids, revealing that the characteristic energy outflow time is minimized in stable states like Rayleigh-Benard convection.

## Contribution

It introduces a method to determine energy storage in non-equilibrium states and shows the minimization of energy outflow time in stable configurations across different energy transfer modes.

## Key findings

- Energy storage depends on energy flux and transfer mode.
- The ratio of stored energy to flux is minimized in stable states.
- The characteristic energy outflow time is minimized in Rayleigh-Benard stable states.

## Abstract

Systems kept out of equilibrium in stationary states by an external source of energy store an energy $\Delta U=U-U_0$. $U_0$ is the internal energy at equilibrium state, obtained after the shutdown of energy input. We determine $\Delta U$ for two model systems: ideal gas and Lennard-Jones fluid. $\Delta U$ depends not only on the total energy flux, $J_U$, but also on the mode of energy transfer into the system. We use three different modes of energy transfer where: the energy flux per unit volume is (i) constant; (ii) proportional to the local temperature (iii) proportional to the local density. We show that $\Delta U /J_U=\tau$ is minimized in the stationary states formed in these systems, irrespective of the mode of energy transfer. $\tau$ is the characteristic time scale of energy outflow from the system immediately after the shutdown of energy flux. We prove that $\tau$ is minimized in stable states of the Rayleigh-Benard cell.

## Full text

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## Figures

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## References

27 references — full list in the complete paper: https://tomesphere.com/paper/1902.10013/full.md

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Source: https://tomesphere.com/paper/1902.10013