# Fluctuating, Lorentz-force-like coupling of Langevin equations and heat   flux rectification

**Authors:** Benedikt Sabass

arXiv: 1706.08367 · 2017-08-09

## TL;DR

This paper explores how fluctuating antisymmetric couplings, similar to Lorentz forces, affect Langevin systems, leading to heat flux control and rectification without causing instabilities.

## Contribution

It introduces a novel analysis of antisymmetric, fluctuating couplings in Langevin equations, revealing their role in heat flux rectification and non-equilibrium dynamics.

## Key findings

- Fluctuating antisymmetric couplings do not induce instabilities.
- Such couplings renormalize effective non-equilibrium friction.
- They enable control and rectification of heat transfer.

## Abstract

In a description of physical systems with Langevin equations, interacting degrees of freedom are usually coupled through symmetric parameter matrices. This coupling symmetry is a consequence of time-reversal symmetry of the involved conservative forces. If coupling parameters fluctuate randomly, the resulting noise is called multiplicative. For example, mechanical oscillators can be coupled through a fluctuating, symmetric matrix of spring "constants". Such systems exhibit well-studied instabilities. In this note, we study the complementary case of antisymmetric, time-reversal symmetry breaking coupling that can be realized with Lorentz forces or various gyrators. We consider the case that these antisymmetric couplings fluctuate. This type of multiplicative noise does not lead to instabilities in the stationary state but renormalizes the effective non-equilibrium friction. Fluctuating Lorentz-force-like couplings also allow to control and rectify heat transfer. A noteworthy property of this mechanism of producing asymmetric heat flux is that the controlling couplings do not exchange energy with the system..

## Full text

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## Figures

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## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1706.08367/full.md

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Source: https://tomesphere.com/paper/1706.08367