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.[1] 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.
B\mu=\left(
\phi | |
c |
,A\right)
\phi
A
B\mu
The Lagrangian density is given by:[2]
| ||||
\mu |
*-\partial | |
B | |
\nu |
*)(\partial | |
B | |
\mu |
\muB\nu-\partial\nu
| ||||
B |
* | |
B | |
\nu |
B\nu.
where
c
\hbar
\partial\mu
The Euler–Lagrange equation of motion for this case, also called the Proca equation, is:
\mu | |
\partial | |
\mu(\partial |
B\nu-\partial\nu
| ||||
B |
\right)2B\nu=0
which is equivalent to the conjunction of[3]
\left[\partial\mu\partial\mu+\left(
mc | |
\hbar |
\right)2\right]B\nu=0
with (in the massive case)
\partial\muB\mu=0
which may be called a generalized Lorenz gauge condition. For non-zero sources, with all fundamental constants included, the field equation is:
c{{\mu}0
When
m=0
In the vector calculus notation, the source free equations are:
\Box\phi-
\partial | \left( | |
\partialt |
1 | |
c2 |
\partial\phi | |
\partialt |
+\nabla ⋅ A\right)=-\left(
mc | |
\hbar |
\right)2\phi
\BoxA+\nabla\left(
1 | |
c2 |
\partial\phi | |
\partialt |
+\nabla ⋅ A\right)=-\left(
mc | |
\hbar |
\right)2A
and
\Box
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
m ≠ 0
B\mu → B\mu-\partial\muf
where
f