Why does the expanding universe redshift light?

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SUMMARY

The discussion centers on the phenomenon of redshift in the context of an expanding universe, emphasizing that light emitted from distant cosmological points experiences energy loss as it travels, resulting in redshift. Participants clarify that energy is not an inherent property of light but is relative to the observer's frame of reference. The conversation distinguishes between inflation and expansion, noting that inflation does not affect the Cosmic Microwave Background (CMB) wavelength, which is instead influenced by the universe's expansion. The discussion highlights the importance of understanding redshift through the lens of comoving observers and the Robertson-Walker metric.

PREREQUISITES
  • Understanding of cosmological redshift and its implications
  • Familiarity with the concept of comoving observers in cosmology
  • Knowledge of the Robertson-Walker metric in General Relativity
  • Basic principles of wave frequency and Doppler effect
NEXT STEPS
  • Study the principles of cosmological redshift in detail
  • Learn about the Robertson-Walker metric and its applications in cosmology
  • Explore the differences between inflation and expansion in the universe
  • Investigate the role of comoving observers in the context of General Relativity
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Astronomers, physicists, and students of cosmology seeking to deepen their understanding of redshift, the expansion of the universe, and the implications of General Relativity on light propagation.

tovisonnenberg
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How does the expansion of space cause light to lose energy?
 
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Wikipedia has a good article on redshift. Could you narrow the question down so that someone can recognize which part is confusing?

You can look at waves in a puddle, pond, or a large bucket. The frequency of the waves is the number of times per second that the wave peaks reach a point. Suppose your "point" is moving, maybe like a fly above a pond. When the fly flies toward the location where a pebble created the waves it will pass more peaks per second. If the fly is flying away from the splash it will pass fewer peaks per second. The frequency measured from the fly's perspective changes when the relative velocity of the source changes.

The light has not really changed energy. If someone throws a baseball from the back of moving pickup truck it will not be going very fast when you catch it. It would hit your glove hard if they threw it forwards and you caught it. The pitcher throws the ball with the same energy/momentum each time. It is only the measurement from your perspective that changes with each pitch.
 
stefan r said:
The light has not really changed energy.
That is not correct. In an expanding universe light emitted from a cosmologically remote point DOES lose energy as it travels and is red-shifted more and more, and loses energy more and more, as the point of reception is farther and farther away. There is no conservation of energy on cosmological scales.
 
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First of all, you should be aware of the fact that energy is not something inherent of the light itself. It only has an energy relative to some chosen frame of reference. Redshift is the shift in the observed frequency relative to that frequency that would be observed by the emitter. That being said, one usually looks at comoving observers in cosmology and there are several different, equivalent, interpretations of cosmological redshift. They may sound different, but it is all a question of what coordinates you use to describe things. To just name a couple:
  • You can see nearby comoving observers as moving relative to each other locally on scales so small that everything looks like Minkowski space. In that sense, the cosmological redshift is an accumulation of Doppler shifts as the light passes from one comoving observer to the next.
  • You can look at the scale factor ##a(t)## in the Robertson-Walker metric, which describes the overall scale of the homogenous and isotropic spatial slices of the universe. In this description, as ##a(t)## grows, the wavelength of the light relative to the comoving observers grows and therefore the frequency that they would observe would be decreasing.

phinds said:
That is not correct. In an expanding universe light emitted from a cosmologically remote point DOES lose energy as it travels and is red-shifted more and more, and loses energy more and more, as the point of reception is farther and farther away. There is no conservation of energy on cosmological scales.
Just to be clear, this refers specifically to the energy relative to comoving observers, an assumption that is not always stated explicitly. Energy is not an inherent property of a light signal by itself (the stress-energy tensor is). In that sense, the light has not changed energy, because energy is not a property inherently associated to it.

stefan r said:
If someone throws a baseball from the back of moving pickup truck it will not be going very fast when you catch it. It would hit your glove hard if they threw it forwards and you caught it. The pitcher throws the ball with the same energy/momentum each time. It is only the measurement from your perspective that changes with each pitch.
This is missing a qualifying statement. The baseball does not have an inherent energy and momentum either - it only has a particular energy and momentum given some fixed frame. As we all know, energy and momentum are not Galilei invariant. They will take different values in different inertial frames and no frame can be said to be preferred over another.
 
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Orodruin said:
Just to be clear, this refers specifically to the energy relative to comoving observers, an assumption that is not always stated explicitly. Energy is not an inherent property of a light signal by itself (the stress-energy tensor is). In that sense, the light has not changed energy, because energy is not a property inherently associated to it.
Good point. Thank you for that clarification.
 
So, inflation itself has zero effect on (for example) CMB wavelength and it's shift to microwave can be explained only by evaluating frames of reference?
 
Ilythiiri said:
So, inflation itself has zero effect on (for example) CMB wavelength
Inflation has no effect on CMB wavelength because it happened before the CMB was released. Do not confuse inflation with expansion. Expansion is the scale of the universe increasing with time, inflation is a hypothetical period of rapid expansion in the very beginning of the universe, before CMB, before nucleosynthesis, intended to explain (among other things) why the universe is so homogeneous.

Also, do not misjudge the effect of expansion on the CMB redshift. What you have to realize is that in GR the "cause" of some effect may be described differently in different coordinates (this is true in SR too). I am not sure what you mean by "evaluating frames of reference". That is not something that one does. What I said was that you can split the redshift into several small step where every step can be described as a Doppler shift between comoving observers. What defines comoving observers is still something that depends on the overall geometry of the spacetime, which is preferentially given in Robertson-Walker coordinates and the coordinate independent statement is that a light signal from one comoving observer to the another will be redshifted if the scale factor at the receiving event is larger (and vice versa). The coordinate-independent maths behind it can be boiled down to comparing the emitter 4-velocity with the 4-frequency of the light to the receiver 4-velocity with the 4-frequency of the light under the knowledge that the 4-frequency is parallel transported along the light world-line. I described this in a technical PF Insight (at A-level) some time ago.
 

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