- #1
Brian-san
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Homework Statement
Consider a 3D space measured with spherical coordinates (r, θ,Φ). A particle moves under the influence of the potential
[tex]V(\vec{r})=\frac{1}{2}k(\vec{r}\cdot\vec{r}), k>0[/tex]
(a) Find the generalized momenta pr, pθ, pΦ.
(b) What is the Lagrangian in these coordinates?
(c) Find the Lagrangian equations of motion.
(d) Find the Hamiltonian in these coordinates.
(e) Find the Hamiltonian equations of motion.
(f) What are the conserved quantities?
(g) Are the solutions the ones you expected from elementary methods?
The attempt at a solution
*I used the prime (') notation to represent time derivatives (d/dt)
Lagrangian: L=0.5m(r'²+r²θ'²+r²sin²(θ)Φ'²)-0.5kr²
Generalized Momenta:
pr=dL/dr'=mr'
pθ=dL/dθ'=mr²θ'
pΦ=dL/dΦ'=mr²sin²(θ)Φ'
Lagrangian Equations of Motion:
mr''=mr(θ'²+sin²(θ)Φ'²)-kr
(mr²θ')'=0.5mr²sin(2θ)Φ'²
mr²sin²θΦ'=l (constant)
Hamiltonian: H=(1/2m)(pr²+pθ²/r²+pΦ²/r²sin²(θ))+0.5kr²
Hamiltonian Equations of Motion:
p'r=-dH/dr=(-1/2mr3)(pθ²+pΦ²/sin²(θ))-kr
p'θ=-dH/dθ=(-1/2mr²)(pΦ²cos(θ)/sin3(θ))
p'Φ=-dH/dΦ=0
r'=pr/m
θ'=pθ/mr²
Φ'=pΦ/mr²sin²(θ)=l/mr²sin²(θ)
Conserved Quantities: Total Energy (E), Momentum in Φ (l)
Does all of this look right? As for the final part, I'm not exactly sure what the result would be from elementary methods. I've gotten so used to the advanced/abstract stuff.
Consider a 3D space measured with spherical coordinates (r, θ,Φ). A particle moves under the influence of the potential
[tex]V(\vec{r})=\frac{1}{2}k(\vec{r}\cdot\vec{r}), k>0[/tex]
(a) Find the generalized momenta pr, pθ, pΦ.
(b) What is the Lagrangian in these coordinates?
(c) Find the Lagrangian equations of motion.
(d) Find the Hamiltonian in these coordinates.
(e) Find the Hamiltonian equations of motion.
(f) What are the conserved quantities?
(g) Are the solutions the ones you expected from elementary methods?
The attempt at a solution
*I used the prime (') notation to represent time derivatives (d/dt)
Lagrangian: L=0.5m(r'²+r²θ'²+r²sin²(θ)Φ'²)-0.5kr²
Generalized Momenta:
pr=dL/dr'=mr'
pθ=dL/dθ'=mr²θ'
pΦ=dL/dΦ'=mr²sin²(θ)Φ'
Lagrangian Equations of Motion:
mr''=mr(θ'²+sin²(θ)Φ'²)-kr
(mr²θ')'=0.5mr²sin(2θ)Φ'²
mr²sin²θΦ'=l (constant)
Hamiltonian: H=(1/2m)(pr²+pθ²/r²+pΦ²/r²sin²(θ))+0.5kr²
Hamiltonian Equations of Motion:
p'r=-dH/dr=(-1/2mr3)(pθ²+pΦ²/sin²(θ))-kr
p'θ=-dH/dθ=(-1/2mr²)(pΦ²cos(θ)/sin3(θ))
p'Φ=-dH/dΦ=0
r'=pr/m
θ'=pθ/mr²
Φ'=pΦ/mr²sin²(θ)=l/mr²sin²(θ)
Conserved Quantities: Total Energy (E), Momentum in Φ (l)
Does all of this look right? As for the final part, I'm not exactly sure what the result would be from elementary methods. I've gotten so used to the advanced/abstract stuff.