Lagrange - Mass under potential in spherical

In summary, the conversation discusses a particle moving in a force field with a potential in spherical coordinates and identifies the two constants of motion of the system, including the energy function or Hamiltonian.
  • #1
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Homework Statement



A particle of mass [itex]m[/itex] moves in a force field whose potential in spherical coordinates is,

[tex]U = \frac{-K \cos \theta}{r^3}[/tex]

where [itex]K[/itex] is constant.

Identify the two constants of motion of the system.

The Attempt at a Solution



[tex]L = T - V = \frac{1}{2} m (\dot{r}^2 + r^2 \dot{\theta}^2 + r^2 \sin^2 \theta ~\dot{\phi}^2) + \frac{K \cos \theta}{r^3}[/tex]

I don't see how there are two constants of motion if the Lagrangian is missing only [itex]\phi[/itex], i.e.,

[tex]\frac{ \partial L}{\partial \phi} = 0 \Rightarrow \frac{\partial L}{\partial \dot{\phi}} = constant[/tex]
 
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  • #2
I'm not 100% sure that this is what the questioner has in mind, but I can think of one quantity that is always a constant of motion whenever the Lagrangian has no explicit time dependence...:wink:
 
  • #3
Energy function/Hamiltonian?

[tex]\frac{\partial L}{\partial t} = 0 = - \frac{dH}{dt}[/tex]

So H = constant.
 
  • #4
Yup.:smile:
 

FAQ: Lagrange - Mass under potential in spherical

What is the concept of Lagrange - Mass under potential in spherical?

The concept of Lagrange - Mass under potential in spherical refers to the mathematical framework used to describe the motion of a small mass under the influence of a central force in a spherical coordinate system. It is derived from the Lagrangian mechanics, which is a mathematical formalism for studying the dynamics of a system.

How does Lagrange - Mass under potential in spherical differ from other Lagrangian mechanics concepts?

Lagrange - Mass under potential in spherical differs from other Lagrangian mechanics concepts as it takes into account the spherical coordinate system, which is particularly useful for studying systems with a central force, such as celestial objects orbiting around a central star.

What are the key equations used in Lagrange - Mass under potential in spherical?

The key equations used in Lagrange - Mass under potential in spherical include the Lagrangian function, the Euler-Lagrange equations, and the Hamiltonian function. These equations are used to describe the motion of a small mass under the influence of a central force in a spherical coordinate system.

What are some real-world applications of Lagrange - Mass under potential in spherical?

Lagrange - Mass under potential in spherical has various real-world applications, including the study of celestial mechanics, such as the motion of planets around the sun, the motion of satellites around the Earth, and the motion of stars in a galaxy. It is also used in the study of fluid dynamics and in the design of control systems for spacecraft and satellites.

What are some limitations of Lagrange - Mass under potential in spherical?

One limitation of Lagrange - Mass under potential in spherical is that it assumes a point mass, which may not accurately represent the actual mass distribution of an object. It also does not take into account the effects of relativity, which becomes important for high-speed objects. Additionally, it may be challenging to solve the equations for complex systems with multiple bodies and forces.

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