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Klein–Gordon Equation

This is a compact lookup card. The mass-shell derivation, two-data Cauchy problem, conserved-current calculation, and one-particle interpretation boundary are owned by the Klein–Gordon Equation page.

With metric signature η=diag⁡(1,−1,−1,−1)\eta=\operatorname{diag}(1,-1,-1,-1) and

□=1c2∂2∂t2−∇2,\Box = \frac{1}{c^2} \frac{\partial^2}{\partial t^2} - \nabla^2,

the free Klein–Gordon equation is

(□+m2c2ℏ2)ϕ=0.\left( \Box+\frac{m^2c^2}{\hbar^2} \right)\phi=0.

Equivalently,

(1c2∂2∂t2−∇2+m2c2ℏ2)ϕ=0.\left( \frac{1}{c^2} \frac{\partial^2}{\partial t^2} - \nabla^2 + \frac{m^2c^2}{\hbar^2} \right)\phi=0.

For a plane wave

ϕ∝exp⁡[−iEtℏ+ip⋅xℏ],\phi \propto \exp \left[ -\frac{iEt}{\hbar} + \frac{i\mathbf p\cdot\mathbf x}{\hbar} \right],

the equation gives the relativistic dispersion relation

E2=p2c2+m2c4.E^2 = \mathbf p^2c^2+m^2c^4.
  • The field or wavefunction is scalar under Lorentz transformations.
  • The metric signature and definition of □\Box are fixed.
  • The displayed equation is free; external electromagnetic coupling requires a covariant-derivative prescription.
  • A one-particle probability interpretation is not the same as the nonrelativistic Schrödinger interpretation.

The Klein–Gordon equation is the natural second-order relativistic equation associated with E2=p2c2+m2c4E^2=\mathbf p^2c^2+m^2c^4. As a fixed-particle wave equation it has interpretive limitations, including negative-frequency solutions and a conserved current whose time component is not positive definite for arbitrary solutions. In modern use, it is cleanest as the field equation for a scalar field or as a controlled relativistic-wave-equation bridge.

  • Mixing metric signatures without changing the sign of □\Box or the mass term.
  • Treating every solution as a nonrelativistic probability amplitude with density ∣ϕ∣2\lvert\phi\rvert^2.
  • Forgetting that both positive- and negative-frequency branches appear.
  • Calling the equation “spinless Schrödinger theory” without the relativistic interpretation caveats.

Insert a plane wave into the free equation and recover the dispersion relation.

Solution

For the plane wave, ∂t2ϕ=−E2ϕ/ℏ2\partial_t^2\phi=-E^2\phi/\hbar^2 and ∇2ϕ=−p2ϕ/ℏ2\nabla^2\phi=-\mathbf p^2\phi/\hbar^2. Therefore

(−E2ℏ2c2+p2ℏ2+m2c2ℏ2)ϕ=0.\left( -\frac{E^2}{\hbar^2c^2} + \frac{\mathbf p^2}{\hbar^2} + \frac{m^2c^2}{\hbar^2} \right)\phi=0.

Multiplying by ℏ2c2\hbar^2c^2 gives −E2+p2c2+m2c4=0-E^2+\mathbf p^2c^2+m^2c^4=0, or E2=p2c2+m2c4E^2=\mathbf p^2c^2+m^2c^4.

  • O. Klein, “Quantentheorie und fünfdimensionale Relativitätstheorie”, Zeitschrift für Physik 37, 895-906, 1926.
  • W. Gordon, “Der Comptoneffekt nach der Schrödingerschen Theorie”, Zeitschrift für Physik 40, 117-133, 1926.
  • J. J. Sakurai, Advanced Quantum Mechanics, Addison-Wesley, 1967.
  • S. Weinberg, The Quantum Theory of Fields, Volume I, Cambridge University Press, 1995.