Loading [MathJax]/jax/output/HTML-CSS/jax.js
Skip to main content
Library homepage
 

Text Color

Text Size

 

Margin Size

 

Font Type

Enable Dyslexic Font
Physics LibreTexts

2.4: Other Conservation Laws

( \newcommand{\kernel}{\mathrm{null}\,}\)

Looking at the Lagrange equation (19), we immediately see that if LTU is independent of some generalized coordinate qj,L/qj=0,15 then the corresponding generalized momentum is an integral of motion: 16 pjL˙qj= const.  For example, for a 1D particle with the Lagrangian (21), the momentum px is conserved if the potential energy is constant (and hence the x-component of force is zero) - of course. As a less obvious example, let us consider a 2D motion of a particle in the field of central forces. If we use polar coordinates r and φ in the role of generalized coordinates, the Lagrangian function, 17 LTU=m2(˙r2+r2˙φ2)U(r), is independent of φ and hence the corresponding generalized momentum, pφL˙φ=mr2˙φ, is conserved. This is just a particular (2D) case of the angular momentum conservation - see Eq. (1.24). Indeed, for the 2 D motion within the [x,y] plane, the angular momentum vector, Lr×p=|nxnynzxyzm˙xm˙ym˙z|, has only one component different from zero, namely the component normal to the motion plane: Lz=x(m˙y)y(m˙x) Differentiating the well-known relations between the polar and Cartesian coordinates, x=rcosφ,y=rsinφ, over time, and plugging the result into Eq. (52), we see that Lz=mr2˙φpφ. Thus the Lagrangian formalism provides a powerful way of searching for non-evident integrals of motion. On the other hand, if such a conserved quantity is evident or known a priori, it is helpful for the selection of the most appropriate generalized coordinates, giving the simplest Lagrange equations. For example, in the last problem, if we knew in advance that pφ had to be conserved, this could provide a motivation for using the angle φ as one of generalized coordinates.


16 This fact may be considered a particular case of a more general mathematical statement called the Noether theorem - named after its author, Emmy Nöther, sometimes called the "greatest woman mathematician ever lived". Unfortunately, because of time/space restrictions, for its discussion I have to refer the interested reader elsewhere - for example to Sec. 13.7 in H. Goldstein et al., Classical Mechanics, 3rd  ed. Addison Wesley, 2002

17 Note that here ˙r2 is the square of the scalar derivative ˙r, rather than the square of the vector ˙r=v.


This page titled 2.4: Other Conservation Laws is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by Konstantin K. Likharev via source content that was edited to the style and standards of the LibreTexts platform.

Support Center

How can we help?