Simple application of euler-lagrange equation

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Discussion Overview

The discussion revolves around the application of the Euler-Lagrange equation to a particle constrained to move along a parabolic path in a uniform gravitational field. Participants explore the implications of the Lagrangian formulation and the nature of forces acting on the particle.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant presents the Lagrangian for a particle in a gravitational field constrained to a parabolic path and expresses confusion over obtaining a velocity-dependent force.
  • Another participant questions why a velocity-dependent force would be unreasonable, suggesting that the constraint introduces such dependencies.
  • A third participant notes that energy conservation can be applied since the Lagrangian does not explicitly depend on time.
  • A later reply acknowledges the derivation of a force equation that includes both gravitational and velocity-dependent terms, indicating a shift in understanding regarding the nature of forces in constrained motion.
  • Further discussion emphasizes that even in the absence of gravity, the particle would still experience acceleration due to the curvature of the path.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the nature of the forces involved, but there is a general agreement on the validity of the velocity-dependent force in the context of the problem. The discussion reflects a process of clarification rather than resolution.

Contextual Notes

Participants acknowledge that constraints introduce complexities in the dynamics of the system, and there is an implicit recognition of the need to consider both gravitational effects and the geometry of motion.

Who May Find This Useful

This discussion may be useful for students and practitioners interested in classical mechanics, particularly those exploring Lagrangian dynamics and constrained motion in gravitational fields.

snoopies622
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Suppose I have a particle of mass m in a uniform, downward gravitational field g, constrained to move on a frictionless parabola

[tex] y = x^2[/tex]

I get

[tex] <br /> L = KE - PE = \frac {1}{2} m (\dot x^2 + \dot y^2) - mgy = \frac {1}{2}m \dot x^2 (1+4x^2) - mgx^2<br /> [/tex]

[tex] \frac {\partial L}{\partial x} = (\frac {1}{2}m \dot x^2)(8x) - 2mgx[/tex]

[tex] <br /> \frac {\partial L}{\partial \dot x} = (m \dot x)(1+4x^2)<br /> [/tex]

From here, no matter how I go about differentiating, I get a velocity-dependent force ( [itex]m \ddot x[/itex] ), which does not seem reasonable to me.

Where exactly is my error?
 
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I don't see any error so far. Why shouldn't the force be velocity dependent? You have a constraint here, and the centripetal part of the constraining forces is velocity dependent. Just write down the Euler-Lagrange equation.
 
PS: Of course, you can use energy conservation here, since the Lagrangian is not explicitly dependent on time, i.e.,

[tex]H=\dot{x} \frac{\partial L}{\partial \dot{x}}-L=E=\text{const}.[/tex]
 
hmmm...thinking...
 
Ok, I get

[tex] <br /> m \ddot x = \frac {-2mg}{1+4x^2} - \frac {4 x \dot x ^2 m}{1+4x^2}<br /> [/tex]

I was expecting only the first term, which is the one caused by the gravitational field, but yes, what you say makes sense to me. Thank you.

(Constraints are new to me.)
 
Last edited:
Yes, it makes even more sense to me now. For - if there were no gravitational field, the particle would move along the parabola at a constant speed, and [itex]\ddot x[/itex] would still be non-zero, since the path is curved.

Thanks again.
 

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