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Definition/Summary
Hamilton's equations of motion is a very general equation of a system evolving deterministically in phase space.
Equations
[tex]\left( {\begin{array}{*{20}{c}}
{\dot q}\\
{\dot p}
\end{array}} \right) = \left( {\begin{array}{*{20}{c}}
0&1\\
{ - 1}&0
\end{array}} \right)\left( {\begin{array}{*{20}{c}}
{\partial H/\partial q}\\
{\partial H/\partial p}
\end{array}} \right)[/tex]
Extended explanation
A common misconception is that Hamilton's equations is only applicable in classical mechanics (celestial mechanics and elastic mechanics). Although this may have once been true, it has found applications everywhere in physics. It applies in almost every conservative system in classical (deterministic) physics. The meat of Hamilton's equations is given by the function H (the 'Hamiltonian'). This is a real function given by position variables and momenta variables with continuous second partial derivatives.
In Newtonian gravity, the Hamiltonian may be given as
[tex]H = \frac{{{p^2}}}{{2}} - \phi [/tex]
Here, phi is the gravitational potential. Mass is taken to be unity.
In classical electrodynamics, the Hamiltonian may be given as
[tex]H = \frac{1}{2}{\left( {{\bf{p}} - e{\bf{A}}} \right)^2} + e\phi [/tex]
Here, e is electric charge, phi is now the electric potential, and A is the magnetic vector potential. Mass is again taken to be unity.
In general relativity, the expression of the Hamiltonian function gets far more complicated.
* This entry is from our old Library feature. If you know who wrote it, please let us know so we can attribute a writer. Thanks!
Hamilton's equations of motion is a very general equation of a system evolving deterministically in phase space.
Equations
[tex]\left( {\begin{array}{*{20}{c}}
{\dot q}\\
{\dot p}
\end{array}} \right) = \left( {\begin{array}{*{20}{c}}
0&1\\
{ - 1}&0
\end{array}} \right)\left( {\begin{array}{*{20}{c}}
{\partial H/\partial q}\\
{\partial H/\partial p}
\end{array}} \right)[/tex]
Extended explanation
A common misconception is that Hamilton's equations is only applicable in classical mechanics (celestial mechanics and elastic mechanics). Although this may have once been true, it has found applications everywhere in physics. It applies in almost every conservative system in classical (deterministic) physics. The meat of Hamilton's equations is given by the function H (the 'Hamiltonian'). This is a real function given by position variables and momenta variables with continuous second partial derivatives.
In Newtonian gravity, the Hamiltonian may be given as
[tex]H = \frac{{{p^2}}}{{2}} - \phi [/tex]
Here, phi is the gravitational potential. Mass is taken to be unity.
In classical electrodynamics, the Hamiltonian may be given as
[tex]H = \frac{1}{2}{\left( {{\bf{p}} - e{\bf{A}}} \right)^2} + e\phi [/tex]
Here, e is electric charge, phi is now the electric potential, and A is the magnetic vector potential. Mass is again taken to be unity.
In general relativity, the expression of the Hamiltonian function gets far more complicated.
* This entry is from our old Library feature. If you know who wrote it, please let us know so we can attribute a writer. Thanks!