Appell's equation of motion
In classical mechanics, Appell's equation of motion is an alternative general formulation of classical mechanics described by Paul Émile Appell in 1900
Here, is an arbitrary generalized acceleration, the second time derivative of the generalized coordinates qr and Qr is its corresponding generalized force; that is, the work done is given by
where the index r runs over the D generalized coordinates qr, which usually correspond to the degrees of freedom of the system. The function S is defined as the mass-weighted sum of the particle accelerations squared,
where the index k runs over the N particles, and
is the acceleration of the kth particle, the second time derivative of its position vector rk. Each rk is expressed in terms of generalized coordinates, and ak is expressed in terms of the generalized accelerations.
Appells formulation does not introduce any new physics to classical mechanics. It is fully equivalent to the other formulations of classical mechanics such as Newton's second law, Lagrangian mechanics, Hamiltonian mechanics, and the principle of least action. Appell's equation of motion may be more convenient in some cases, particularly when nonholonomic constraints are involved. Appell’s formulation is an application of Gauss' principle of least constraint.
The change in the particle positions rk for an infinitesimal change in the D generalized coordinates is
Taking two derivatives with respect to time yields an equivalent equation for the accelerations
The work done by an infinitesimal change dqr in the generalized coordinates is
where Newton's second law for the kth particle
has been used. Substituting the formula for drk and swapping the order of the two summations yields the formulae
Therefore, the generalized forces are
This equals the derivative of S with respect to the generalized accelerations
yielding Appell’s equation of motion
Euler's equations provide an excellent illustration of Appell's formulation.
Consider a rigid body of N particles joined by rigid rods. The rotation of the body may be described by an angular velocity vector , and the corresponding angular acceleration vector
The generalized force for a rotation is the torque N, since the work done for an infinitesimal rotation is . The velocity of the kth particle is given by
where rk is the particle's position in Cartesian coordinates; its corresponding acceleration is
Therefore, the function S may be written as
Setting the derivative of S with respect to equal to the torque yields Euler's equations
- ↑ Appell, P (1900). "Sur une forme générale des équations de la dynamique.". Journal für die reine und angewandte Mathematik. 121: 310–?.
- Whittaker, ET (1937). A Treatise on the Analytical Dynamics of Particles and Rigid Bodies, with an Introduction to the Problem of Three Bodies (4th ed.). New York: Dover Publications. ISBN.
- Seeger (1930). "Unknown title". Journal of the Washington Academy of Science. 20: 481–?.
- Brell, H (1913). "Unknown title". Wien. Sitz. 122: 933–?. Connection of Appell's formulation with the principle of least action.
- PDF copy of Appell's article at Goettingen University
- PDF copy of a second article on Appell's equations and Gauss's principle