Rotation and Translation coordinates

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Discussion Overview

The discussion revolves around the interpretation of generalized coordinates in the context of kinetic energy for a holonomic system, particularly focusing on the distinction between translation and rotation coordinates in spherical coordinates. Participants explore the implications of these definitions on the dependence of kinetic energy on various coordinates.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions how the kinetic energy T can depend on the polar angle θ, which is associated with rotation, while the radial coordinate r, associated with translation, also influences T.
  • Another participant asserts that T depends on the rates of change of the coordinates (i.e., ##\dot{\theta}## and ##\dot{r}##) rather than the coordinates themselves.
  • A definition is provided stating that a system admits translation along a generalized coordinate ##q^j## if the partial derivative of T with respect to ##q^j## is zero, indicating invariance under translation.
  • Further clarification is given that the transformation of θ does not correspond to a rotation about a fixed axis, which affects how points in space behave under this transformation.
  • A detailed explanation is presented regarding the conditions under which coordinates are classified as translation or rotation coordinates, emphasizing the role of time dependence in the unit vectors associated with these coordinates.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between kinetic energy and the generalized coordinates, particularly regarding the roles of θ and r. There is no consensus on the implications of these relationships, and the discussion remains unresolved.

Contextual Notes

Participants highlight the time dependence of unit vectors in spherical coordinates, which complicates the classification of coordinates as translation or rotation. The discussion does not resolve the implications of these dependencies on the kinetic energy formulation.

FrederikPhysics
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I am currently reading Goldstein's Classical mechanics and come on to this problem. Let q1,q2,...,qn be generalized coordinates of a holonomic system and T its kinetic energy. qk correspondes to a translation of the entire system and qj a rotation of the entire system around some axis, then ∂qjT=∂qkT=0 since velocities are not affected by a translation of the origin or a rotation of the coordinate axes.
Now take as an example the kinetic energy of a single particle in spherical coordiantes, here the polar angle θ correspondes to a rotation of the system, but T is dependent on θ. r correspondes to a translation of the particle and therefore the system but T depends on r. How should I undersand this?
Mvh. Frederik
 
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T does not depend on ##\theta## but on ##\dot\theta## which is a different generalized coordinate...
idem ##r## and ##\dot r##
 
Actually it is a definition:
"the system admits translation along the generalized coordinate ##q^j##"##\Longleftrightarrow## ##"\frac{\partial T}{\partial q^j}=0"##. Or equivalently iff ##T## is invariant under the group ##q^j\mapsto q^j+s,\quad s\in \mathbb{R}##
It doesn't matter what is ## q^j##. If ##q^j## is an angle then we say that the system admits a rotation.
 
BvU said:
T does not depend on ##\theta## but on ##\dot\theta## which is a different generalized coordinate...
idem ##r## and ##\dot r##

For a system consisting of one particle with mass m one writes T=½m(dr/dt2+r2 dθ/dt2+r2sin2θ dφ/dt2) in spherical coordinates, θ being the polar angle and φ the azimutal angle, that makes T=T(r, θ, dr/dt, dθ/dt, dφ/dt).
 
O now I see what you want. This is a good question indeed. It is because ##\theta\mapsto \theta+s## is not a rotation of the space about a fixed axis. Look how all the points of the space conduct under this transformation
 
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Okay, so one might say:
Let ##T=\frac{1}{2}m\dot{\textbf{r}}\cdot\dot{\textbf{r}}## be the kinetic energy of a one particle system, ##\textbf{r}## the position vector in some frame and q a set of generalized coordinates. ##q_{k}## is called a translation coordinate when there exists a vector ##\textbf{n}## such that ##\frac{\partial \textbf{r}}{\partial q_{k}}=\textbf{n}## fulfilling ##\dot{\textbf{n}}=\textbf{0}##. Then ##\frac{\partial T}{\partial q_{k}}=m\dot{\textbf{r}}\cdot\frac{d}{dt}\frac{\partial\textbf{r}}{\partial q_{k}}=0##.
When this is true ##q_{k}##is said to translate the system in the direction of ##\textbf{n}##.

##q_{j}## is called a rotation coordinate when there exists a vector ##\textbf{n}## such that ##\frac{\partial \textbf{r}}{\partial q_{j}}=\textbf{n}\times\textbf{r}## fulfilling ##\dot{\textbf{n}}=\textbf{0}##. Then ##\frac{\partial T}{\partial q_{j}}=m\dot{\textbf{r}}\cdot\frac{d}{dt}\frac{\partial\textbf{r}}{\partial q_{j}}=0##.
When this is true ##q_{k}## is said to rotate the system around the direction of ##\textbf{n}##.
The generalazation to more particles follows naturally.

Within this definition the coordinates r and ##\theta## of the spherical coordinate system, in general neither translates nor rotates the system since the r unitvector, ##\hat{\textbf{r}}##, depends on time and the rotation axis of ##\theta##, nθ, depends on time. The coordinate φ is a rotation coordinate since its rotation axis nφ correspondes to the fixed polar axis.
 

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