Can Spacetime Perturbance Reveal Paths in the Double Slit Experiment?

In summary, if you could use the spacetime perturbance caused by the energy-momentum of a photon (or any other particle) to figure out which way it took in a double slit experiment, then you wouldn't need interference any more.
  • #1
greypilgrim
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Hi.

Would it be possible (at least in principle) to use the spacetime perturbance caused by the energy-momentum of a photon (or any other particle) to figure out which way it took in a double slit experiment? Can this question even be answered in today's attempts at quantum gravity?
 
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  • #2
greypilgrim said:
Would it be possible (at least in principle) to use the spacetime perturbance caused by the energy-momentum of a photon (or any other particle) to figure out which way it took in a double slit experiment?
If you can figure out which way it took you don't get interference any more.
It doesn't matter how exactly you can figure it out. You don't need anything exotic, a simple polarizer does the job. This is an experiment you can do in a classroom.
 
  • #3
Orthogonally polarized beams of light don't create an interference pattern because you can figure out in principle which way a photon took, even if the measurement is not performed. Since we see interference in normal experiments, it shouldn't even be possible in principle to use spacetime perturbance to figure out which way, no matter how good our future measurement devices will be. Why not? As far as I know, GR doesn't allow superpositions of spacetime perturbances that collapse into one when interacting with the measurement device.
 
  • #4
greypilgrim said:
Orthogonally polarized beams of light don't create an interference pattern because you can figure out in principle which way a photon took, even if the measurement is not performed. Since we see interference in normal experiments, it shouldn't even be possible in principle to use spacetime perturbance to figure out which way, no matter how good our future measurement devices will be. Why not? As far as I know, GR doesn't allow superpositions of spacetime perturbances that collapse into one when interacting with the measurement device.

There would need to be a quantum interaction to obtain the which way information. That is not present in GR, but would be in a quantum theory of gravity. The fact that quantum interference is observed in the standard version of the experiment might rule out some candidate quantum gravity theories.

There have been attempts to research this area. Here are a couple that might be up your alley, from some top teams:

https://arxiv.org/abs/1206.0965
Quantum mechanics and general relativity have been extensively and independently confirmed in many experiments. However, the interplay of the two theories has never been tested: all experiments that measured the influence of gravity on quantum systems are consistent with non-relativistic, Newtonian gravity. On the other hand, all tests of general relativity can be described within the framework of classical physics. Here we discuss a quantum interference experiment with single photons that can probe quantum mechanics in curved space-time. We consider a single photon traveling in superposition along two paths in an interferometer, with each arm experiencing a different gravitational time dilation. If the difference in the time dilations is comparable with the photon's coherence time, the visibility of the quantum interference is predicted to drop, while for shorter time dilations the effect of gravity will result only in a relative phase shift between the two arms. We discuss what aspects of the interplay between quantum mechanics and general relativity are probed in such experiments and analyze the experimental feasibility.

https://arxiv.org/abs/1304.7912
In the last years quantum correlations received large attention as key ingredient in advanced quantum metrology protocols, in this letter we show that they provide even larger advantages when considering multiple-interferometer setups. In particular we demonstrate that the use of quantum correlated light beams in coupled interferometers leads to substantial advantages with respect to classical light, up to a noise-free scenario for the ideal lossless case. On the one hand, our results prompt the possibility of testing quantum gravity in experimental configurations affordable in current quantum optics laboratories and strongly improve the precision in "larger size experiments" such as the Fermilab holometer; on the other hand, they pave the way for future applications to high precision measurements and quantum metrology.
 
  • #5
The energy is way too low to lead to a detectable signature via gravity. Send Planck energy photons and the result will be different.
 
  • #6
mfb said:
The energy is way too low to lead to a detectable signature via gravity.
In practice or fundamentally? If the latter, why would there be a fundamental limit?
 
  • #7
Fundamentally.
Gravity is simply way too weak. Tens of orders of magnitude too weak.

If it would be strong enough the double slit experiment wouldn't work.
 
  • #8
Why overcomplicate things? "spacetime perturbance" isn't a thing, but it sounds like you are thinking about general relativity, which is completely unnecessary and just makes things more complicated. Clasical gravity is just fine.

So, how would you go about measuring the gravitational force ("spacetime perturbance") from your beam? (Which can be atoms or molecuules instead of light, if you want to make it easier) Hang a weight and see how far it moves when the beam passes it.

Problem is, just as the beam exerts a force on the weight, the weight exerts a force on the beam. If there is enough force to determine which slit the beam passed through, there is enough force to drive it towards only one of the slits - you will get the same pattern as if it were single slit. If there's not enough force to drive the beam to only one slit there is not enough to determine which slit it went through.

In short, this is a very difficult way to effectively cover one slit.
 
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1. What is spacetime perturbance?

Spacetime perturbance refers to small changes or disturbances in the fabric of space and time caused by the presence of massive objects. These changes can affect the motion of other objects or particles in the vicinity.

2. How can spacetime perturbance be used to determine direction?

By analyzing the magnitude and direction of spacetime perturbances, scientists can infer the presence and location of massive objects that are causing the disturbances. This information can then be used to determine the direction of these objects.

3. What tools or technologies are used to measure spacetime perturbance?

Scientists use advanced instruments such as gravitational wave detectors, telescopes, and satellites to measure spacetime perturbances. They also use mathematical models and simulations to analyze the data and make predictions about the direction and location of massive objects.

4. Can spacetime perturbance be used to study objects beyond our solar system?

Yes, spacetime perturbances can be observed and studied on a variety of scales, from objects within our own solar system to distant galaxies. By measuring these disturbances, scientists can gain insights into the nature of these objects and their interactions with other objects in the universe.

5. What are the potential applications of using spacetime perturbance to determine direction?

Studying spacetime perturbances and using them to determine direction can have many practical applications, such as improving navigation systems for spacecraft or satellites, predicting the motion of comets and asteroids, and understanding the behavior of celestial bodies in the universe.

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