Doppler Shift and Light Quanta: Questions on the Nature of Light and Observation

In summary, the conversation discusses the concept of Doppler Shift and the implications of quantum physics on the behavior of light. It is concluded that the state of the light and the measuring device are both necessary to determine its measured frequency. It is also noted that there may be a theoretical limit on the number of people who can visually observe a burst of light due to a finite number of photons emitted, and that a faraway observer may potentially see an event that a nearer observer cannot due to the probabilistic nature of light's path. Overall, it is stated that while everyday light can be treated classically, quantum aspects of light require more precise experiments to fully understand.
  • #1
Andy_K
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Dear All,

I have a couple of (noob) questions regarding Doppler Shift and light from a quantum physics perspective:

a) Since different observers will see the light at different frequencies depending on their reference frame / velocity thus resulting in Doppler Shift, does that mean that any light emitted exists in an infinite variation / probability of frequencies, and only the "observed" / measured frequencies will materialize?

b) If there are an infinite / very large number of observers, would the emitted light (say a very brief burst) run out of observable light? Because if a single photon is emitted, then even if there are 2 detectors, only one will fire. Likewise, if an emitted light burst contains only say 1 million photons, does that mean the 1,000,001th observer (or detector) will not see anything?

Thank you for "shedding light on the matter". :)
 
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  • #2
Andy_K said:
does that mean that any light emitted exists in an infinite variation / probability of frequencies, and only the "observed" / measured frequencies will materialize?

No, it means that the state of the light alone is not enough to determine what its measured frequency will be; you also need to know the state of the measuring device (or at least enough of it to determine the Doppler shift). This is not an issue specific to QM.

Andy_K said:
If there are an infinite / very large number of observers, would the emitted light (say a very brief burst) run out of observable light?

It depends on what measurement you make and how the observers get the results. Yes, if you make a measurement that counts photons, you will only count a finite number and then there will be no more. But there is no reason why any given observer can only know the result of his own counter. And you can also make other measurements that don't count photons (they measure other observables).
 
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  • #3
Thank you for your clarifications. Let's say if we are solely looking at "visual" measurements, i.e. with humans seeing the light, where the underlying process is similar to counting photons.

Does that mean there is a theoretical limit as to how many people can visually observe a burst of light, due to a finite number of photons / energy emitted?

Consequently, does that mean that a faraway observer could potentially visually observe an event that a nearer observer may not see, since the light can take on any path (though with differing probabilities)?
PeterDonis said:
It depends on what measurement you make and how the observers get the results. Yes, if you make a measurement that counts photons, you will only count a finite number and then there will be no more. But there is no reason why any given observer can only know the result of his own counter. And you can also make other measurements that don't count photons (they measure other observables).
 
  • #4
Andy_K said:
Let's say if we are solely looking at "visual" measurements, i.e. with humans seeing the light, where the underlying process is similar to counting photons.

Sort of.

Andy_K said:
Does that mean there is a theoretical limit as to how many people can visually observe a burst of light, due to a finite number of photons / energy emitted?

In principle there could be, yes. But you might want to try estimating how likely it would be for such a limit to be reached in practice.

Andy_K said:
does that mean that a faraway observer could potentially visually observe an event that a nearer observer may not see, since the light can take on any path (though with differing probabilities)?

Again, in principle this could happen (with sufficiently faint light emitted from the event), but you might want to try estimating how likely it would be in practice for a typical amount of light emitted from a typical event.

The short answer is that the everyday light we see can be treated classically; the quantum aspects of light take much more precise experiments to probe.
 
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FAQ: Doppler Shift and Light Quanta: Questions on the Nature of Light and Observation

1. What is Doppler Shift?

Doppler Shift is the change in frequency or wavelength of a wave in relation to an observer who is moving relative to the wave source.

2. How does Doppler Shift affect light?

Doppler Shift can cause a change in the frequency and wavelength of light waves, resulting in a shift in the color of the light. This is known as the Doppler Effect.

3. What is the difference between redshift and blueshift?

Redshift and blueshift are both examples of the Doppler Effect. Redshift occurs when an object is moving away from an observer, causing the light waves to stretch and decrease in frequency, resulting in a shift towards the red end of the spectrum. Blueshift occurs when an object is moving towards an observer, causing the light waves to compress and increase in frequency, resulting in a shift towards the blue end of the spectrum.

4. How is Doppler Shift used in astronomy?

Doppler Shift is used in astronomy to determine the speed and direction of objects in space. By measuring the amount of redshift or blueshift in the light emitted from an object, scientists can calculate its velocity and determine if it is moving away or towards us.

5. What are light quanta?

Light quanta, also known as photons, are the smallest units of light energy. They are particles that make up electromagnetic radiation, including visible light. They have both wave-like and particle-like properties and are responsible for the transmission of light energy.

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