petergreat said:
It relies on coupling between Einstein tensor and EM stress-energy tensor, which has NO experimental support whatsoever.
Why do you say that? I'm not an expert on experimental tests of GR, but it seems to me that there is quite a bit of experimental evidence on this.
Of course there are classic tests like the deflection of light by the sun and the Pound-Rebka experiment, both of which showed that light interacts gravitationally pretty much as predicted by standard GR.
As an example of an alternative rule for coupling, I could imagine [itex]G_{ab}=c_1T_{ab}+c_2g_{ab}T^c_c[/itex] for the Einstein field equations, but then the equivalence principle would be violated by the second term, which vanishes for EM waves. The equivalence principle has a lot of support from extremely precise experiments.
In general, I think it's quite difficult to come up with alternative forms of the Einstein field equations that are consistent with observational support for mass-energy conservation, momentum conservation, and the equivalence principle.
The early universe was radiation-dominated, so cosmological observations that probe that era should be very direct tests of whether light produces gravitational fields in the way described by GR. Don't modern high-precision CMB measurements probe this in some detail?
Do you know of any currently viable alternative theory of gravity (tensor-scalar theories, etc.) that disagrees with GR on this issue?
Of course extrapolating all the way to the intense fields of a highly charged black hole is a very big extrapolation. Clearly astrophysical black holes with these properties don't exist naturally. Even if the human race avoids extinction for another thousand years, I would be surprised if the Reissner–Nordström metric is ever tested directly against experiment. Maybe if large extra dimensions exist, in which case you might be able to make microscopic black holes in particle accelerators.