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Damian Owls (talk | contribs) →An example: a particle confined to a sphere: added the derivations of the secondary constraints |
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From this consistency condition, we immediately get the [[First class constraints#Constrained Hamiltonian dynamics from a Lagrangian gauge theory|secondary constraint]]
<math>\begin{align}
By the same reasoning, this constraint should be added into the Hamiltonian with an undetermined (not necessarily constant) coefficient {{mvar|u}}<sub>2</sub>. At this point, the Hamiltonian is▼
0&=\{H,p_\lambda\}_\text{PB}\\
&=\sum_{i}\frac{\partial H}{\partial q_i}\frac{\partial p_\lambda}{\partial p_i}-\frac{\partial H}{\partial p_i}\frac{\partial p_\lambda}{\partial q_i}\\
&=\frac{\partial H}{\partial \lambda}\\
&=\frac{1}{2}(r^2-R^2)\\
&\Downarrow\\
0&=r^2-R^2
\end{align}</math>
▲
:<math>
H = \frac{p^2}{2m} + mgz - \frac{\lambda}{2}(r^2-R^2) + u_1 p_\lambda + u_2 (r^2-R^2) ~.
</math>
<math>\vec{p}\cdot\vec{r}=0</math>,▼
<math>\begin{align}
0&=\{H,r^2-R^2\}_{PB}\\
&=\{H,x^2\}_{PB}+\{H,y^2\}_{PB}+\{H,z^2\}_{PB}\\
&=\frac{\partial H}{\partial p_x}2x+\frac{\partial H}{\partial p_y}2y+\frac{\partial H}{\partial p_z}2z\\
&=\frac{2}{m}(p_xx+p_yy+p_zz)\\
&\Downarrow\\
\end{align}</math>
Again, one should add this constraint into the Hamiltonian, since, on-shell, no one can tell the difference. Therefore, so far, the Hamiltonian looks like
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where {{mvar|u}}<sub>1</sub>, {{mvar|u}}<sub>2</sub>, and {{mvar|u}}<sub>3</sub> are still completely undetermined.
Note that, frequently, all constraints that are found from consistency conditions are referred to as
We keep turning the crank, demanding this new constraint have vanishing [[Poisson bracket]]
:<math>
0=\{\vec{p}\cdot\vec{r},\, H\}_{PB} = \frac{p^2}{m} - mgz+ \lambda r^2 -2 u_2 r^2
</math>
We might despair and think that there is no end to this, but because one of the new Lagrange multipliers has shown up, this is not a new constraint, but a condition that fixes the Lagrange multiplier:
:<math>
u_2 = \frac{\lambda}{2} + \frac{1}{r^2}\left(\frac{p^2}{2m}-\frac{1}{2}mgz \right).
</math>
Plugging this into our Hamiltonian gives us (after a little algebra)
<math>
H = \frac{p^2}{2m}(2-\frac{R^2}{r^2}) + \frac{1}{2}mgz(1+\frac{R^2}{r^2})+u_1p_\lambda+u_3\vec p \cdot\vec r
</math>
Now that there are new terms in the Hamiltonian, one should go back and check the consistency conditions for the primary and secondary constraints. The secondary constraint's consistency condition gives
:<math>
\frac{2}{m}\vec{r}\cdot\vec{p} + 2 u_3 r^2 = 0.
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