gptejms said:
Your question 'suggests' to me that with our present capabilities,we can't produce such high intensity electromagnetic fields---enough to cause any significant spacetime curvature.Can you give an order of magnitude calculation to give us an idea?An experiment to test the idea could look like this---if light bends in region of such a high intensity electromag. field(perhaps we could concentrate on just the magnetic field and try producing extraordinarily strong magnets)then we would know that the curvature has been produced.But I am sure there must be better ways around.
Let's think about this from the PoV of what the most intense EM fields and greatest spacetime curvature is, in the present universe, and later we'll examine whether any of these are amenable to tests - even in principle - of well-formed hypotheses. OK?
First, the most intense magnetic fields, in the present universe, are likely to be http://solomon.as.utexas.edu/~duncan/magnetar.html , whose fields are likely to be as many OOM stronger than the strongest we can generate here on Earth is greater than the Earth's own field.
Next, the most energetic gammas may well have a comparable 'curvature effect' to objects whose gravity we can measure. For example, we have
'seen' TeV gammas from the Crab pulsar (or nebula), and expect that GRBs emit PeV or higher gammas (such energetic gammas probably cannot propogate clear across the universe, but as we've 'seen' a couple of nearby AGN in TeV, perhaps a nearby GRB might be 'visible' in PeV gammas). Homework question: if a TeV gamma were converted (magically) into a lump of baryons (yes, it would be magic!), what would the mass of that lump be?
Next (2), it may be that a 'long duration' GRB results in the formation of black hole whose mass is several times that of the Sun. If the progenator star had a magnetic field, it may be that, in the last few microseconds before the BH formed, that field reached an intensity which makes a magnetar's field look like a fridge magnet. Too, the spacetime curvature would be far more extreme than that around the Sun (which has provided the most sensitive tests of some aspects of GR to date).
Finally, as the two neutron stars in a binary merge/collide (they lose energy as gravitational waves; without some external event, a collision is certain), many kinds of extreme environments will likely be created.
Closer to home, you might like to read the reports of the
Fundamental Physics Working Group (it's in the middle of the page), from the recent ESA Cosmic Visions workshop. Do you feel that any of the proposed (local) experiments would test a hypothesis related to spacetime curvature resulting from EM?