Rayleigh dissipation function

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In physics, the Rayleigh dissipation function, named after Lord Rayleigh, is a function used to handle the effects of velocity-proportional frictional forces in Lagrangian mechanics. It was first introduced by him in 1873.[1] If the frictional force on a particle with velocity v can be written as Ff=kv, the Rayleigh dissipation function can be defined for a system of N particles as

R(v)=12i=1N(kxvi,x2+kyvi,y2+kzvi,z2).

This function represents half of the rate of energy dissipation of the system through friction. The force of friction is negative the velocity gradient of the dissipation function, Ff=vR(v), analogous to a force being equal to the negative position gradient of a potential. This relationship is represented in terms of the set of generalized coordinates qi={q1,q2,qn} as

Ff=Rq˙i.

As friction is not conservative, it is included in the Qi term of Lagrange's equations,

ddtLqi˙Lqi=Qi.

Applying of the value of the frictional force described by generalized coordinates into the Euler-Lagrange equations gives (see [2])

ddt(Lqi˙)Lqi=Rq˙i.

Rayleigh writes the Lagrangian L as kinetic energy T minus potential energy V, which yields Rayleigh's Eqn. (26) from 1873.

ddt(Tqi˙)Tqi+Rq˙i+Vqi=0.

Since the 1970s the name Rayleigh dissipation potential for R is more common. Moreover, the original theory is generalized from quadratic functions qR(q˙)=12q˙𝕍q˙ to dissipation potentials that are depending on q (then called state dependence) and are non-quadratic, which leads to nonlinear friction laws like in Coulomb friction or in plasticity. The main assumption is then, that the mapping q˙R(q,q˙) is convex and satisfies 0=R(q,0)R(q,q˙), see e.g. [3] [4] [5]


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