Shift in wavelength of photons from the Sun using energy argument

Click For Summary

Discussion Overview

The discussion revolves around the change in wavelength of photons emitted from the Sun as they travel to Earth, specifically examining the gravitational potential energy (GPE) of the photon and its relationship to energy conservation and wavelength change. The conversation touches on theoretical aspects and the implications of gravitational effects on light, with references to both classical mechanics and General Relativity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant outlines a method for calculating the change in wavelength of a photon based on its GPE, leading to an approximate expression for change in GPE.
  • Another participant asserts that energy conservation dictates that as the photon gains GPE, it must lose energy, resulting in an increase in wavelength.
  • A later reply questions the rigor of the argument, suggesting that a more thorough approach would involve General Relativity.
  • One participant references the Pound-Rebka experiment as an example of measuring wavelength changes due to gravitational effects, indicating interest in experimental validation.

Areas of Agreement / Disagreement

Participants generally agree on the conservation of energy principle as it applies to the photon’s GPE and wavelength change. However, there is disagreement regarding the rigor of the initial argument, with some advocating for a more formal treatment using General Relativity.

Contextual Notes

The discussion highlights the reliance on assumptions regarding the effective GPE of photons and the simplifications made in the calculations. There is also an acknowledgment of the limitations of classical mechanics in fully addressing the phenomenon.

etotheipi
I came across a question recently which involved calculating the change in wavelength of a photon between being emitted from the surface of the sun and arriving at the Earth.

The method that was implied involved calculating the GPE's of the photon (assuming the photon to have a mass h/[c lambda]) at the start and end points in order to calculate the overall decrease in its GPE, with Mph, Me and Ms being the photon, Earth and Sun masses respectively and rs, re and rse being the Sun's radius, Earth's radius and Earth-Sun distance respectively. This turns out to be: $$\Delta U = GM_{ph}[-\frac{M_{e}}{r_{e}}-\frac{M_{s}}{r_{se}}+\frac{M_{s}}{r_{s}}+\frac{M_{e}}{r_{se}}]$$ Since the term Ms/Rs is substantially larger than the others, we omit all of the other terms and find the following approximate expression for change in GPE: $$\Delta U = GM_{ph}\frac{M_{s}}{r_{s}}$$The last step is to equate this change in GPE to the change in energy of the photon from which we can approximate the change in wavelength of that photon:$$\Delta E_{ph} \approx hc \frac{\Delta \lambda}{\lambda^{2}} = \frac{GM_{s}}{r_{s}}\frac{h}{\lambda c}$$ This yields the result $$\frac{\Delta \lambda}{\lambda} = 2.1\cdot10^{-6}$$Whilst I can understand the mathematical steps, I have trouble understanding the intuition for this last part. Why can we equate the increase in the photon's GPE to the decrease in the energy associated with its wavelength? Thanks a bunch.
 
Science news on Phys.org
Energy is conserved. So if the photon gains GPE as it climbs out of the sun's gravitational well, it must lose energy from somewhere. Since the photon's energy is hc/λ, and h and c are constants, λ must increase.
 
  • Like
Likes   Reactions: etotheipi
phyzguy said:
Energy is conserved. So if the photon gains GPE as it climbs out of the sun's gravitational well, it must lose energy from somewhere. Since the photon's energy is hc/λ, and h and c are constants, λ must increase.

Thanks for the really quick reply! That makes sense. I was also wondering how rigorous is this argument considering that the photon only really has an effective GPE?
 
I think what you have outlined is a heuristic argument which is not completely rigorous. To do it properly, you need to use General Relativity. This Wikipedia article has a description of how you do that, as well as experimental tests. I find the Pound-Rebka experiment really fascinating. They were able to measure the increase in wavelength of light propagating from the basement of their lab up to the roof, as it climbed out of the Earth's gravitational field.
 
  • Like
Likes   Reactions: etotheipi

Similar threads

Replies
3
Views
2K
  • · Replies 0 ·
Replies
0
Views
2K
Replies
15
Views
3K
  • · Replies 2 ·
Replies
2
Views
6K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
Replies
1
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 27 ·
Replies
27
Views
3K