The role of thermal fluctuations in the motion of a free body
Pep Espa\~nol, Mark Thachuk, J.A. de la Torre

TL;DR
This paper extends classical Euler's equations to include thermal fluctuations and internal dissipation, providing a thermodynamically consistent model for the stochastic motion and orientation of deformable bodies influenced by thermal effects.
Contribution
It introduces a generalized, stochastic version of Euler's equations that accounts for internal thermal fluctuations and dissipation mechanisms in free bodies.
Findings
Thermal fluctuations cause deformable bodies to explore all orientations.
Spinning bodies tend to align their principal axis with angular momentum.
The theory predicts equilibrium shapes of spinning bodies.
Abstract
The motion of a rigid body is described in Classical Mechanics with the venerable Euler's equations which are based on the assumption that the relative distances among the constituent particles are fixed in time. Real bodies, however, cannot satisfy this property, as a consequence of thermal fluctuations. We generalize Euler's equations for a free body in order to describe dissipative and thermal fluctuation effects in a thermodynamically consistent way. The origin of these effects is internal, i.e. not due to an external thermal bath. The stochastic differential equations governing the orientation and central moments of the body are derived from first principles through the theory of coarse-graining. Within this theory, Euler's equations emerge as the reversible part of the dynamics. For the irreversible part, we identify two distinct dissipative mechanisms; one associated with…
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Taxonomy
TopicsAdvanced Thermodynamics and Statistical Mechanics · Micro and Nano Robotics · Material Dynamics and Properties
