Photon wavelength shift from gravitational lensing?

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Discussion Overview

The discussion centers on whether a photon traveling through a vacuum loses energy due to gravitational interactions with massive bodies, particularly in the context of gravitational lensing. Participants explore the implications of energy conservation, potential shifts in photon wavelength, and the effects of gravitational fields over vast distances.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants question if a photon loses energy while interacting with gravity, suggesting that gravitational lensing may affect its wavelength.
  • Others argue that the energy of the photon remains the same before and after gravitational lensing, particularly in cases of small deflections.
  • A participant introduces the idea of extreme scenarios, such as close approaches to black holes, where the interaction might differ and could involve a "slingshot effect."
  • One participant speculates about the cumulative effects of gravitational fields over long distances, questioning if photons could experience a gradual energy loss through multiple lensing events.
  • Another participant asserts that the average photon experiences balanced gravitational forces over time, leading to negligible overall effects on its observed frequency.
  • A later reply mentions the Integrated Sachs-Wolfe Effect, suggesting that photons lose energy when traversing gravitational potential wells due to cosmic expansion, which could be relevant to the cosmic microwave background.

Areas of Agreement / Disagreement

Participants express differing views on whether photons experience energy shifts due to gravitational lensing. While some maintain that energy is conserved, others propose that there could be effects under specific conditions. The discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Participants note that observational errors may mask any potential energy shifts, and there is uncertainty regarding the calculations of such effects over extensive distances and varying gravitational fields.

toliynyk
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The basic question is: will a photon traveling through a vacuum lose some of its energy due to interactions with gravity from a massive body?
Gravitational lensing implies that the photon will change its initial direction but is its energy conserved (i.e. differences in blueshift/redshift before and after the point of closest approach to the gravitational origin)? Classical theory implies that both objects contribute to the gravitational interaction and since the photon is assumed to be massless, then the delta in kinetic energy should come from its wavelength... any suggestions?
 
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The energy of the photon will be the same before and after the interaction. That is true, at least, for the kind of gravitational lensing that we observe, where the deflection is extremely small.

If you imagine an extreme situation in which the photon has a very close approach to a black hole and consequently undergoes a large deflection, then the statement needs to be qualified: in the rest frame of the black hole. In a rest frame in which the black hole is moving, the photon (or any other projectile) will experience a "slingshot effect" similar to the one that has been used to add speed to a planetary spacecraft as it undergoes a close approach to Jupiter.
 
Bill_K said:
The energy of the photon will be the same before and after the interaction. That is true, at least, for the kind of gravitational lensing that we observe, where the deflection is extremely small.

So what I understand is that if there hypotheticaly IS some sort of energy shift going on, it lies well within the current observational error? If so, can't this effect stack up in, say, x->infinity lensing events? i.e. a photon slowly snaking through billions of light years of variable gravitatioanl fields... even if the effect is miniscule it'll to get "tired". I know I would :)
Which leads to an other question - has anyone done the calculations on the probability and posible magnitude of such an event? I keep getting the standard redshift equation when I try to calculate this so I'm rather confused...
 
I would say that the average photon experiences equal amounts of gravitational pull in all directions over a long period of time, probably having little overall effect on it's observed frequency once it reaches us.
 
toliynyk said:
So what I understand is that if there hypotheticaly IS some sort of energy shift going on

There is not. The photon enters the gravity well and gains an energy E1. It then leaves the gravity well and loses an energy E2. E1 = E2.
 
On a very large scale there is something called the Integrated Sachs-Wolfe Effect. When passing through a gravitational potential well a photon will lose part of its energy, because the expansion of the universe causes the well to be shallower on the way out than it was on the way in. This effect can be seen in the small variations from uniformity of the cosmic microwave background.
 

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