Klein Gordon equation, probability density

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SUMMARY

The discussion focuses on the application of the Klein-Gordon Equation to demonstrate the conservation of probability density, specifically showing that \(\partial_{\mu}j^{\mu} = 0\). The Klein-Gordon Equation is defined as \(\left(\frac{\partial^{2}}{\partial t^{2}} - \nabla^{2} + m^{2}\right) \phi = 0\). The current density \(j^{\mu}\) is expressed as \(j^{\mu} = \frac{i}{2m} \left[\phi^{*}(\partial^{\mu} \phi) - (\partial^{\mu} \phi^{*}) \phi\right]\). The solution involves expanding \(j^{\mu}\) and applying the product rule to compute \(\partial_{\mu}j^{\mu}\), utilizing the Klein-Gordon equation to simplify terms and achieve the desired result.

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  • Understanding of the Klein-Gordon Equation and its implications in quantum field theory.
  • Familiarity with the concept of probability density in quantum mechanics.
  • Knowledge of partial differential equations and their applications in physics.
  • Proficiency in using mathematical notation and manipulation of complex functions.
NEXT STEPS
  • Study the derivation of the Klein-Gordon Equation in detail.
  • Learn about the implications of conservation laws in quantum field theory.
  • Explore the product rule in the context of vector calculus and its applications.
  • Investigate the role of mass terms in field equations and their physical significance.
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This discussion is beneficial for theoretical physicists, graduate students in quantum mechanics, and anyone studying quantum field theory, particularly those interested in the mathematical foundations of particle physics.

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[SOLVED] Klein Gordon equation, probability density

Homework Statement



Use the Klein-Gordon Equation to show that

\partial_{\mu}j^{\mu} = 0

Homework Equations



KG:

\left(\frac{\partial^{2}}{\partial t^{2}} - \nabla^{2} + m^{2}\right) \phi = (\partial_{\mu}\partial^{\mu} + m^{2}) \phi = 0

j:

j^{\mu} = \frac{i}{2m} \left[\phi^{*}(\partial^{\mu} \phi) - (\partial^{\mu} \phi^{*}) \phi]\right

The Attempt at a Solution



OK, so I've expanded j out, taking the differentials and have the following for my components:

time component:

\frac{i}{2m} \left[\phi^{*} \frac{\partial^{2} \phi}{\partial t^{2}} - \phi \frac{\partial^{2} \phi^{*}}{\partial t^{2}}\right]

space components:

\frac{i}{2m} \left[- \phi^{*} \frac{\partial^{2} \phi}{\partial r^{2}} + \phi \frac{\partial^{2} \phi^{*}}{\partial r^{2}}\right]

(where I've used r = (x,y,z) )

Putting them in this form:

\frac{i \phi^{*}}{2m} \left[\frac{\partial^{2} \phi}{\partial t^{2}} - \frac{\partial^{2} \phi}{\partial r^{2}}\right] - \frac{i \phi}{2m} \left[\frac{\partial^{2} \phi^{*}}{\partial t^{2}} - \frac{\partial^{2} \phi^{*}}{\partial r^{2}}\right]

Which looks slightly more like the KG equation. However, my trouble is with the mass terms, I have no (mass)² terms to complete the KG equation and hence show the desired expression is zero. Can anyone see what I'm missing here?
 
Physics news on Phys.org
Don't expand out components, just compute \partial_{\mu}j^{\mu} expanding the partial using the product rule. You can reduce parts using the Klein-Gordon equation and then they and the other parts will cancel.
 

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