In physics, specifically field theory and particle physics, the Proca action describes a massive spin-1 field of mass m in Minkowski spacetime. The corresponding equation is a relativistic wave equation called the Proca equation. The Proca action and equation are named after Romanian physicist Alexandru Proca.
The Proca equation is involved in the Standard Model and describes there the three massive vector bosons, i.e. the Z and W bosons.
This article uses the (+−−−) metric signature and tensor index notation in the language of 4-vectors.
The field involved is a complex 4-potential , where is a kind of generalized electric potential and is a generalized magnetic potential. The field transforms like a complex four-vector.
The Lagrangian density is given by:
where is the speed of light in vacuum, is the reduced Planck constant, and is the 4-gradient.
The Euler–Lagrange equation of motion for this case, also called the Proca equation, is:
which is equivalent to the conjunction of
with (in the massive case)
which may be called a generalized Lorenz gauge condition. For non-zero sources, with all fundamental constants included, the field equation is:
When , the source free equations reduce to Maxwell's equations without charge or current, and the above reduces to Maxwell's charge equation. This Proca field equation is closely related to the Klein–Gordon equation, because it is second order in space and time.
In the vector calculus notation, the source free equations are:
and is the D'Alembert operator.
The Proca action is the gauge-fixed version of the Stueckelberg action via the Higgs mechanism. Quantizing the Proca action requires the use of second class constraints.
If , they are not invariant under the gauge transformations of electromagnetism
where is an arbitrary function.
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In differential geometry, the four-gradient (or 4-gradient) is the four-vector analogue of the gradient from vector calculus. In special relativity and in quantum mechanics, the four-gradient is used to define the properties and relations between the various physical four-vectors and tensors. This article uses the (+ − − −) metric signature. SR and GR are abbreviations for special relativity and general relativity respectively. indicates the speed of light in vacuum. is the flat spacetime metric of SR.
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Covers the study of a vibrating string, wave equations, sinusoidal waves, and eigenvalue problems.
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We prove that the critical Maxwell-Klein-Gordon equation on R4+1 is globally well-posed for smooth initial data which are small in the energy norm. This reduces the problem of global regularity for large, smooth initial data to precluding concentration of ...