Klein-Gordon equation: Difference between revisions

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<math>E^2=\bold p^2c^2+m^2c^4</math>
<math>E^2=\bold p^2c^2+m^2c^4</math>


Substituting <math>E \rightarrow i\hbar \frac{\partial}{\partial t}</math> and <math>\bold p \rightarrow -i\hbar \nabla</math>, we get Klein-Gordon as follows:
Substituting <math>E \rightarrow i\hbar \frac{\partial}{\partial t}</math> and <math>\bold p \rightarrow -i\hbar \nabla</math>, we get Klein-Gordon equation for free particles as follows:


<math>-\hbar^2 \frac{\partial ^2\phi(\bold r, t)}{\partial t^2}=(-\hbar^2c^2\nabla^2+m^2c^4)\phi(\bold r, t)\qquad \qquad \qquad \qquad \qquad (9.2)</math>  
<math>-\hbar^2 \frac{\partial ^2\psi(\bold r, t)}{\partial t^2}=(-\hbar^2c^2\nabla^2+m^2c^4)\psi(\bold r, t)\qquad \qquad \qquad \qquad \qquad (9.2)</math>  


Klein-Gordon can also be written as the following:
Klein-Gordon can also be written as the following:


<math>(\square-K^2)\phi(\bold r, t)=0\qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad (9.3)</math>
<math>(\square-K^2)\psi(\bold r, t)=0\qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad(9.3)</math>


where <math>\square=\nabla^2-\frac{1}{c^2}\frac{\partial^2}{\partial t^2}</math>  is d'Alembert operator and <math>K=\frac{mc}{\hbar}</math>.
where <math>\square=\nabla^2-\frac{1}{c^2}\frac{\partial^2}{\partial t^2}</math>  is d'Alembert operator and <math>K=\frac{mc}{\hbar}</math>.


Equation (9.3) looks like a classical wave equation with an extra term <math>K^2</math>.
Equation (9.3) looks like a classical wave equation with an extra term <math>K^2</math>.
For a charged particle couple with electromagnetic field, Klein-Gordon equation is as follows:
<math>[i\hbar \frac {\partial}{\partial t}-e\phi(\bold r, t)]^2\psi(\bold r, t)=([-i\hbar\nabla-\frac{e}{c}\bold A(\bold r, t)]^2c^2+m^2c^4)\psi(\bold r, t)</math>
Klein-Gordon is second order in time. Therefore, to see how the states of a system evolve in time we need to know both <math>\psi(\bold r, t)</math> and  <math>\frac{\partial\psi(\bold r, t)}{\partial t}</math> at a certain time. While in nonrelativistic quantum mechanics, we only need <math>\psi(\bold r, t)</math>
Also because the Klein-Gordon equation is second order in time, it has the solutions <math>\psi(\bold r, t)=e^{i(\bold p \bold r - Et)/\hbar}</math> with either sign of energy <math>E=\pm c\sqrt{\bold p^2+m^2c^2}</math>.  The negative energy solution of Klein-Gordon equation has a strange property that the energy decreases as the magnitude of the momentum increases. We will see that the negative energy solutions of Klein-Gordon equation describe antiparticles, while the positive energy solutions describe particles.


==Continuity equation==
==Continuity equation==


==Nonrelativistic limit==
==Nonrelativistic limit==

Revision as of 01:23, 15 April 2009

How to construct

Starting from the relativistic connection between energy and momentum:

Substituting and , we get Klein-Gordon equation for free particles as follows:

Klein-Gordon can also be written as the following:

where is d'Alembert operator and .

Equation (9.3) looks like a classical wave equation with an extra term .

For a charged particle couple with electromagnetic field, Klein-Gordon equation is as follows:

Klein-Gordon is second order in time. Therefore, to see how the states of a system evolve in time we need to know both and at a certain time. While in nonrelativistic quantum mechanics, we only need

Also because the Klein-Gordon equation is second order in time, it has the solutions with either sign of energy . The negative energy solution of Klein-Gordon equation has a strange property that the energy decreases as the magnitude of the momentum increases. We will see that the negative energy solutions of Klein-Gordon equation describe antiparticles, while the positive energy solutions describe particles.

Continuity equation

Nonrelativistic limit