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Heat equation and Brownian motion of an overdamped rotating sphere
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abstract
The governing equations of Brownian rigid bodies that both translate and rotate are of interest in fields such as self-assembly of proteins, anisotropic colloids, dielectric theory, and liquid crystals. In this paper, the partial differential equation that describes the evolution of concentration is derived from the stochastic differential equation of a sphere experiencing Brownian motion in a viscous medium where a potential field may be present. The potential field may be either interactions between particles or applied externally. The derivation is performed once for particles whose orientation can be specified by a vector ($S^2$), and again for particles which require a rotation matrix ($SO(3)$). The derivation shows the important difference between probability density and concentration, the Ito and Stratonovich calculus, and a Piola-type identity is obtained to complete the derivation.
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Cited by 1 Pith paper
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New Agegraphic Dark Energy Driven Reconstruction of \boldmath{$f(Q)$} Gravity and its Cosmological Implications
An f(Q) gravity function is derived by forcing its dark energy density to match New Agegraphic Dark Energy, and this NADE-equal-f(Q) model fits BAO data only marginally better than the standard model.
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