kev said:
I am talking more about the intrinsic physical frequency or energy of the photon. I agree that observers at different heights would measure different frequencies and that is the conventional view but I am looking deeper than that, as I always like to get a feel for what is really physically happening by deduction and logic.
But you are just arbitrarily choosing one observer as your reference observer and then transforming other observations to the local frame of the reference observer. You're entitled to do this, but I'm entitled to choose another observer as my reference and come to a different conclusion.
If you're looking for some frame-invariant notion of frequency, the only answer is zero, which doesn't help much. (Zero because it's proportional to energy; the "rest energy" of a photon is proportional to its "rest mass" which is zero. Or just let v \rightarrow c in the Doppler shift formula.)
kev said:
Potential energy in the gravitational context is a Newtonian concept. In GR, the concept of a rising photon giving up its energy to be stored as potential energy in a classical gravitational field is very questionable. See this discussion by Baez:
http://math.ucr.edu/home/baez/physics/Relativity/GR/energy_gr.html
In general, energy is a problem in GR. I'm no expert in this, but I understand that in some specific circumstances it is nevertheless possible to come up with a sensible definition of energy that is conserved. The link that you provided includes these words:
"In certain special cases, energy conservation works out with fewer caveats. The two main examples are static spacetimes and asymptotically flat spacetimes."
"The Schwarzschild metric is both static and asymptotically flat, and energy conservation holds without major pitfalls."
I haven't just made up potential energy in GR. In Schwarzschild coordinates it is, for a hovering object,
\frac{mc^2}{\sqrt{1 - 2GM/rc^2}}
See Woodhouse, N M J (2007),
General Relativity, Springer, London, ISBN 978-1-84628-486-1, pp. 100-101.
kev said:
Here is something else to consider. I shine a household torch at a black hole for a few seconds. The photons from the torch are blue shifted as they fall towards the black hole and the frequency of the photons goes to infinity as they approach the event horizon of the black hole. Have really added infinite energy to the black hole by shining a torch at it for a few seconds?
No, because,
in the frame of a distant hovering observer the photons would also lose an infinite amount of potential energy as they fell (taking an infinite time to do so). (Other frames would disagree, as energy is a frame-dependent concept.)