Does Light Lose Energy and Change Frequency Due to Gravitational Waves?

In summary, the conversation discusses the potential loss of energy for light due to gravitational waves and the redshifting of light from distant galaxies. There is also a mention of the expected production of high frequency gravitational waves from thermal motion of matter, but no evidence of contribution from radiation (photons). This raises questions about the applicability of treating photons as point particles in quantum electrodynamics.
  • #1
rahuljayanthb
13
0
hi,
since light is energy moving through the fabric of space time at velocity c , it should lose energy due to gravitational waves. doesn't this mean that the light from a distant galaxy would keep decreasing in frequency? further more this would imply that light that was originally emitted as blue light would be observed by the observer as (say) red assuming the observer and galaxy are at relative rest.
 
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  • #2
rahuljayanthb said:
since light is energy moving through the fabric of space time at velocity c , it should lose energy due to gravitational waves.
Gravitational radiation is quadrupole. An object moving at constant speed does not emit gravitational waves.
 
  • #3
Light does get redshifted due to the expansion of the universe, however.
 
  • #4
While the OP's premise of straight line photon propagation giving gravitational wave emission is not per se correct, there is something else here that surely needs a good answer. The expected production of HFGW's (high frequency gravitational waves) owing to thermal motion of matter within say the sun, white dwarf stars, neutron stars etc has been calculated e.g. http://arxiv.org/abs/0708.3343.
Cannot find a single reference to any contribution from radiation (photons). Which seems strange because in large hot stars for instance pressure from thermal radiation dominates. A simple appeal to relativistic beaming would, by analogy with Bremsstrahlung radiation http://en.wikipedia.org/wiki/Bremsstrahlung , suggest an infinitely large contribution to HFGW's from photon emission/absorption/scattering events within stellar cores. This doesn't happen. So does this have something to say about the applicability of treating photons as point particles that propagate through space at c? One school of thought in QED views them as such.
 
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FAQ: Does Light Lose Energy and Change Frequency Due to Gravitational Waves?

1. What is energy degradation of light?

The energy degradation of light refers to the loss of energy that occurs when light travels through a medium or interacts with matter. This can be caused by absorption, scattering, or reflection.

2. How does energy degradation of light impact the environment?

The energy degradation of light can have both positive and negative impacts on the environment. On one hand, it is essential for photosynthesis and plays a crucial role in the Earth's climate. On the other hand, excessive energy degradation due to human activities, such as light pollution, can disrupt ecosystems and harm wildlife.

3. What factors affect the rate of energy degradation of light?

The rate of energy degradation of light can be influenced by several factors, including the type of medium the light is passing through, the distance the light travels, the wavelength of the light, and the angle at which the light is hitting the surface.

4. Can energy degradation of light be prevented or reduced?

While energy degradation of light is a natural phenomenon, it can be reduced through various methods such as using energy-efficient light sources, directing light only where it is needed, and minimizing light pollution. It is also important to consider the environmental impacts when designing and using lighting systems.

5. How is energy degradation of light relevant in other scientific fields?

The concept of energy degradation of light is relevant in various scientific fields, such as optics, atmospheric science, and astronomy. Understanding how light interacts with matter and how its energy is degraded is crucial for developing new technologies, studying the Earth's climate, and exploring the universe.

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