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Proca Equation


The Proca equation is a linear partial differential equation for a massive four-vector field A^nu. In flat spacetime, with units chosen so that c=h=1 and metric signature (+,-,-,-), it is

 partial_muF^(munu)+m^2A^nu=J^nu,
(1)

where F^(munu)=partial^muA^nu-partial^nuA^mu, m>0 is the mass parameter, and J^nu is a source (Gondran 2009, Schambach and Sanders 2018).

Applying partial_nu to both sides gives

 m^2partial_nuA^nu=partial_nuJ^nu.
(2)

If the source is conserved, so that partial_nuJ^nu=0, the field also satisfies partial_nuA^nu=0. Substitution into the defining equation yields

 partial_mupartial^muA^nu+m^2A^nu=J^nu.
(3)

Thus each component satisfies an inhomogeneous Klein-Gordon equation. Setting m=0 in the defining equation gives the source form of Maxwell's equations, but the divergence condition above follows only for m>0 (Schambach and Sanders 2018).


See also

Klein-Gordon Equation, Maxwell's Equations

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References

Gondran, M. "Proca Equations Derived from First Principles." Amer. J. Phys. 77, 925-926, 2009. https://doi.org/10.1119/1.3137042.Schambach, M. and Sanders, K. "The Proca Field in Curved Spacetimes and Its Zero Mass Limit." Rep. Math. Phys. 82, 203-239, 2018. https://doi.org/10.1016/S0034-4877(18)30086-7.

Cite this as:

Weisstein, Eric W. "Proca Equation." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/ProcaEquation.html

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