I don't understand where a_{\mu} \rightarrow \Lambda_{\mu}{}^{\nu} a_{\nu} + \partial_{\mu}\Omega comes from.
If I assume \acute{a}_{\mu} is a regauged (dual) 4-vector, \acute{a}=a + d\Omega,
the Lorentz transformation, or any linear transform for that matter, acts on the entire tensor, \acute{a}_{\mu}\rightarrow \Lambda_{\mu}\\ ^\nu [a_{\nu} + (\partial_{\nu}\Omega)]
Gauge transformation tells you that the difference between two potentials is a 4-vector:
a_{(2)}^{\mu} - a_{(1)}^{\mu} = \partial^{\mu} \omega
Thus, under Lorentz transformation, (a_{(2)} - a_{(1)}) transforms like a 4-vector
\left( a_{(2)}^{\mu} - a_{(1)}^{\mu} \right)^{'} = \Lambda^{\mu}{}_{\nu} \left( a_{(2)}^{\nu} - a_{(1)}^{\nu}\right)
Clearly, this is satisfied by
a_{(1,2)}^{\mu^{'}} = \Lambda^{\mu}{}_{\nu} a_{(1,2)}^{\nu} + \partial^{\mu}\Omega
i.e., Lorentz transformation is always associated a gauge transformation so that the same choice of gauge is available for all Lorentz observers. Indeed the above transformation law guarantees that our gauge-invariant theory is Lorentz invariant as well.
You can now see exactly what is involved for a particular choice of gauge. In the Lorentz gauge, for example, we require \partial . a to be relativistic invariant
\partial^{'} . \ a^{'} = \partial \ . \ a
even though a is not a 4-vector. From the above transformation law, you see that this is possible only if
\partial^{2}\Omega = 0
which is the familiar equation for \Omega in the Lorentz gauge.
The inhomogeneous transformation law
a \rightarrow \Lambda a + \partial \Omega
results from the fact that the gauge potential is a connection 1-form on principal bundle \left(R^{4} \times U(1)\right).
Connections 1-forms have the following properties:
1) they transform inhomogeneously under coordinate transformations.
2) if \Gamma is an arbitrary connection, and T is a tensor field, then (T + \Gamma ) is another connection. Conversely, if \Gamma_{1} and \Gamma_{2} are connections, then \Gamma_{2} - \Gamma_{1} is a tensor field.
3) they enable us to define a covariant derivatives D = \partial + \Gamma, and a curvature 2-form (= field tensor):
R^{(.)}{}_{(.) \mu \nu} = D_{\mu} \Gamma^{(.)}{}_{\nu (.)} - D_{\nu} \Gamma^{(.)}{}_{\mu (.)}
You can now see that (not just the gauge potential a_{\mu}) the gravitatinal potential \Gamma^{\lambda}{}_{\mu \nu} ( Reimannian connection) also satisfies the above three conditions.
If I have asked you (and the other participants in this thread) to prove that \Gamma^{\lambda}{}_{\mu \nu} is a (1,2)-type world tensor, would not you (and the others) have laughed at me and said: "but \Gamma is not a tensor!"
regards
sam