vanhees71 said:
I'm not so sure about what you wrote about the transformation properties of the em. current.
Why is that? I started with the transformation law of a covariant vector field with respect to the
group of general coordinate transformations. That is
[tex]
\bar{J}^{\mu}( \bar{x}) = \frac{\partial \bar{x}^{\mu}}{\partial x^{\nu}} \ J^{\nu}(x). \ \ (1)[/tex]
For general
infinitesimal coordinates transformation,
[tex]\bar{x}^{\mu} = x^{\mu} + \delta x^{\mu},[/tex]
I wrote eq(1) as
[tex]
\bar{J}^{\mu}( x + \delta x ) = J^{\nu}(x) \frac{\partial}{\partial x^{\nu}}\left( x^{\mu} + \delta x^{\mu}\right). \ \ (2)[/tex]
Since,
[tex]
\frac{\partial \bar{x}^{\mu}}{\partial x^{\nu}} = \frac{\partial}{\partial x^{\nu}}\left( x^{\mu} + \delta x^{\mu}\right) = \delta^{\mu}_{\nu} + \partial_{\nu}\left( \delta x^{\mu}\right),[/tex]
I can rewrite eq(2) as
[tex]
\bar{J}^{\mu}(x + \delta x ) = J^{\mu}(x) + J^{\nu}(x) \partial_{\nu}\left( \delta x^{\mu}\right). [/tex]
Since, [itex]\partial_{\nu}J^{\nu} = 0[/itex], I can write the above equation in the form,
[tex]
\bar{J}^{\mu}(x + \delta x ) = J^{\mu}(x) + \partial_{\nu}\left( \delta x^{\mu}J^{\nu}(x) \right). \ \ (3)[/tex]
Expanding the LEFT HAND SIDE of eq(3), to first order in [itex]\delta x[/itex], leads to
[tex]
\bar{J}^{\mu}( x + \delta x ) \approx \bar{J}^{\mu}(x) + \delta x^{\rho}\partial_{\rho}\bar{J}^{\mu}(x). \ \ (4)[/tex]
Now, I claim that,
[tex]\delta x^{\rho}\partial_{\rho}\bar{J}^{\mu}(x) \approx \delta x^{\rho} \partial_{\rho}J^{\mu}(x). \ \ (5)[/tex]
Why? Well, the calculus of infinitesimals tells you so. If the two functions, [itex]\bar{J}(x)[/itex] and [itex]J(x)[/itex], differ by an infinitesimal [itex]\omega[/itex], i.e., if
[tex]\bar{J}(x) \approx J(x) + \mathcal{O}(\omega ),[/tex]
then,
[tex]\omega \ \bar{J}(x) \approx \omega \ J(x) + \mathcal{O}( \omega^{2}).[/tex]
Thus, to first order in [itex]\omega[/itex], we write
[tex]\omega \ \bar{J}(x) \approx \omega \ J(x),[/tex]
which proves the claim in eq(5). The same is true for [itex]J(\bar{x})[/itex] and [itex]J(x)[/itex], i.e. we can, to the first order, write
[tex]\omega \ J(\bar{x}) \approx \omega \ J(x). \ \ \ (R)[/tex]
Ok, now putting eq(4) and eq(5) into eq(3) leads to
[tex]
\bar{J}^{\mu}(x) - J^{\mu}(x) = \partial_{\nu}\left( \delta x^{\mu}J^{\nu}(x) \right) - \delta x^{\rho}\partial_{\rho}J^{\mu}(x). \ \ (6)[/tex]
To specialized eq(6) to infinitesimal Lorentz transformation,
[tex]\delta x^{\mu} = \omega^{\mu}{}_{\nu}x^{\nu},[/tex]
I use the fact (which follows from [itex]\omega_{\mu\nu}= -\omega_{\nu\mu}[/itex]) that
[tex]\partial_{\nu}\left( \delta x^{\nu}\right) = 0. \ \ (7)[/tex]
Using eq(7) in eq(6), we arrive at the infinitesimal LORENTZ transformation of the CONSERVED vector current
[tex]
\delta J^{\mu}(x) = \partial_{\nu}\left( \delta x^{\mu}J^{\nu}(x) - \delta x^{\nu}J^{\mu}(x) \right). \ \ (8)[/tex]
It's a four-vector field. So its transformation property is
$$\bar{J}^{\mu}(\bar{x})={\Lambda^{\mu}}_{\nu} J^{\nu}(x),$$
where
This Lorentz transformation follows from the general case of eq(1), when you specify
[tex]\frac{\partial \bar{x}^{\mu}}{\partial x^{\nu}} = \Lambda^{\mu}{}_{\nu}.[/tex]
$$\bar{x}=\Lambda x$$
and [itex]\Lambda[/itex] is the Lorentz-transformation matrix.
which means that YOU can write
[tex]\Lambda = \frac{\partial \bar{x}}{\partial x}.[/tex]
For an infinitesimal Lorentz transformation you have
[tex]{\Lambda^{\mu}}_{\nu} =\delta_{\nu}^{\mu}+{\delta \omega^{\mu}}_{\nu}[/tex] with [itex]\delta \omega_{\mu \nu}=g_{\mu \rho} {\delta \omega^{\rho}}_{\nu}[/itex] antisymmetric.
YOU can write this as,
[tex]\frac{\partial \bar{x}^{\mu}}{\partial x^{\nu}} = \frac{\partial x^{\mu}}{\partial x^{\nu}} + \omega^{\mu}{}_{\nu},[/tex]
or,
[tex]
\omega^{\mu}{}_{\nu} = \frac{\partial}{\partial x^{\nu}}\left( \bar{x}^{\mu} - x^{\mu}\right) = \frac{\partial}{\partial x^{\nu}}\left( \omega^{\mu}{}_{\rho}x^{\rho}\right).[/tex]
So, YOU can write YOUR infinitesimal Lorentz transformation in the form
[tex]\bar{x}^{\mu} = x^{\mu} + \delta x^{\mu},[/tex]
with
[tex]\delta x^{\mu} = \omega^{\mu}{}_{\nu}x^{\nu},[/tex]
so that YOUR Lorentz condition, [itex]\omega_{\mu\nu}= - \omega_{\nu\mu}[/itex], become equivalent to
[tex]\partial_{\mu}\left( \delta x^{\mu}\right) = 0.[/tex]
This gives
$$\bar{J}^{\mu}(\bar{x})=J^{\mu}(x)+{\delta \omega^{\mu}}_{\nu} J^{\nu}(x) = J^{\mu}(x')-{\delta \omega^{\rho}}_{\sigma} \bar{x}^{\sigma} \bar{\partial}_{\rho} J^{\mu}(\bar{x})+{\delta \omega^{\mu}}_{\nu} J^{\nu}(x).$$
This equation is correct but UGLY. This is why it doesn’t look like eq(8). OK, let us turn it into something BEAUTIFUL. First instead of YOUR [itex]\delta \omega[/itex], I will use [itex]\omega[/itex]; it is the infinitesimal parameter, so there is no need to stick [itex]\delta[/itex] in front of it.
As explained above, we write
[tex]
\omega^{\mu}{}_{\nu} = \bar{\partial}_{\nu}\left( \omega^{\mu}{}_{\rho}\bar{x}^{\rho}\right) = \bar{\partial}_{\nu}\left( \delta \bar{x}^{\mu}\right),[/tex]
and eq(R) (remember the infinitesimal stuff),
[tex]\omega^{\mu}{}_{\nu} \ J^{\nu}(x) \approx \omega^{\mu}{}_{\nu} \ J^{\nu}(\bar{x}).[/tex]
This transforms YOUR equation into
[tex]
\bar{J}^{\mu}(\bar{x}) – J^{\mu}(\bar{x}) = - \delta \bar{x}^{\nu}\bar{\partial}_{\nu}J^{\mu}(\bar{x}) + J^{\nu}(\bar{x}) \bar{\partial}_{\nu}\left( \delta \bar{x}^{\mu}\right). \ \ \ (Y)[/tex]
Next, we use current conservation,
[tex]\bar{\partial}_{\nu}J^{\nu}(\bar{x}) = 0,[/tex]
and the Lorentz condition
[tex]\bar{\partial}_{\nu} \left( \delta \bar{x}^{\nu}\right) = 0.[/tex]
With these, eq(Y) becomes
[tex]
\delta J^{\mu}(\bar{x}) = \bar{\partial}_{\nu}\left( \delta \bar{x}^{\mu}J^{\nu}(\bar{x}) - \delta \bar{x}^{\nu}J^{\mu}(\bar{x}) \right).[/tex]
Isn’t this eq(8)?
The current-conservation law (continuity equation), [itex]\partial_{\mu} J^{\mu}=0[/itex], ensures that the total charge
$$Q=\int_{\mathbb{R}^3} \mathrm{d}^3 \vec{x} J^0(x)$$
is a scalar (i.e., Lorentz invariant) quantity.
Well Sir, the whole thread was about proving that very statement.
Regards
Sam