D Alembert's Principle: Dependence of kinetic energy on generalized coordinates.

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SUMMARY

The discussion centers on D'Alembert's Principle and the dependence of kinetic energy on generalized coordinates, specifically contrasting Cartesian and polar coordinates. In Cartesian coordinates, the partial derivative of kinetic energy (T) with respect to the generalized coordinate (qj) is zero, while in polar coordinates, it is not, particularly due to the presence of angular velocity. The kinetic energy in polar coordinates is expressed as T = (1/2)m˙r² + (1/2)mr²˙θ², where the term ∂T/∂r = mr˙θ² is non-zero, highlighting the role of curvature in coordinate systems.

PREREQUISITES
  • Understanding of classical mechanics principles, particularly kinetic energy.
  • Familiarity with generalized coordinates and their application in physics.
  • Knowledge of differential geometry concepts related to curvature.
  • Basic understanding of polar coordinates and their mathematical representation.
NEXT STEPS
  • Study the derivation of kinetic energy in various coordinate systems, focusing on polar coordinates.
  • Explore the implications of D'Alembert's Principle in classical mechanics.
  • Learn about the relationship between generalized coordinates and independent variables in mechanics.
  • Investigate the role of curvature in differential geometry and its impact on physical systems.
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This discussion is beneficial for physics students, educators in classical mechanics, and researchers interested in the mathematical foundations of motion and energy in different coordinate systems.

puneeth9b
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Hey!
I was reading Goldestein's book on classical mechanics and I came across this (Page 20 3rd Edition):

"Note that in a system of Cartesian coordinates the partial derivative of T with
respect to qj vanishes. Thus, speaking in the language of differential geometry,
this term arises from the curvature of the coordinates qj. In polar coordinates,
e.g., it is in the partial derivative of T with respect to an angle coordinate that the
centripetal acceleration teml appears."

Here T=Kinetic energy of the system
qj= the jth generalized coordinate.

I don't exactly understand how this works.
1.Why isn't it (dT/dq) zero in polar coordinates if it is zero in cartesian coordinates?
2.What if velocity was a function of coordinates? dT/dq can't possibly be zero even in cartesian coordinates then right?

I might have missed some assumption that makes everything clear, so all those of you who've read the book, please help!
 
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I have the exact same question, no luck yet...
 
I'm not sure why you'd expect ##\partial T/\partial q_i## to be zero in polar coordinates. The kinetic energy in polar coordinates is given by
$$T=\frac{1}{2}m\dot{r}^2+ \frac{1}{2}mr^2\dot{\theta}^2.$$ Clearly, ##\partial T/\partial r = mr\dot{\theta}^2## is not zero in general. Goldstein should have said it was the partial derivative with respect to the radial coordinate that gives rise to the centripetal acceleration term.

Regarding your second question, remember that the coordinates ##q_i## and velocities ##\dot{q_i}## are considered independent variables.
 
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