Chronos you might find the following of interest, especially the part about GR.
u = energy density
S= energy flux
I’d be glad to post the complete section but I don’t think I’m suppose to do that.
Chronos you might find the following of interest, especially the part about GR.
u = energy density
S= energy flux
I’d be glad to post the complete section but I don’t think I’m suppose to do that.
Sure, all electrical problems can be done using field theory. However electricity becomes useful when charges are moving and by far the vast majority of charges are in conductors and all of the charges that go to our devices are in some sort of conductor. Circuit theory was developed precisely because of this fact and we use circuit theory in ordinary electrical work maybe 100 times as often as field theory so why not think in terms of it? To use field theory seems to me sorta like finding the area of a triangle each time by integrating.
Both methods are models. One of them is useful day in and day out. The other is vital when it is needed but most applications don’t need it.
It is true that we’ve never observed a Riser-Nordstrom black hole, which would be the real test case for this, and given how weak gravity is, we probably haven’t ever measured the gravitational effect of electromagnetic fields at all. Offhand, I’d say the best bet would be the radio lobes of active galactic nuclei (which can contain millions of solar masses in magnetic field energy), but we’d need to know a lot more about dark matter before we could get any meaningful data out of them.
On the other hand, it is in principle to perform such an experiment, and u = 1/2(E[sup]2[/sup]+B[sup]2[/sup]) is consistent with the theory (I’m not certain this is true of all of the other hypothetical formulae for u mentioned in your quote). Incidentally, what’s the source of that quote? I don’t recall seeing it in Griffiths or Jackson, the two most likely suspects.
The same as above “The Feynman Lectures” II, 27-6.
BTW what’s the big deal about determining the radial distance when applying Coulomb’s law to a Reissner-Nordstrom Black Hole?
I’m not aware there is any big deal about it. Could you care to elaborate?
(aside: I had a hunch I was misspelling Reissner)
From sci.physics.research.
Radial distance when dealing with any black hole isn’t exactly corn flakes, but from the tone of the above post I took it that there was something especially odd about it when dealing with a RN BH.