Detecting Gravitons: Challenging the Foundations of General Relativity

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Discussion Overview

The discussion revolves around the theoretical implications of detecting gravitons and how this relates to the foundations of general relativity. Participants explore the challenges of graviton detection, the assumptions behind proposed detection methods, and the broader context of quantum gravity theories.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • Some participants suggest that detecting gravitons could challenge the assumptions underlying general relativity.
  • Others argue that general relativity does not incorporate gravitons and is viewed as an approximation of a more comprehensive theory of quantum gravity.
  • It is noted that while gravitational waves have been detected, gravitons remain undetected, and the feasibility of building a sensitive detector for individual gravitons is questioned.
  • Concerns are raised about the assumptions in a referenced paper regarding the size and placement of detectors, particularly the claim that a Jupiter-sized detector cannot be placed closer than 100,000 light years to a black hole.
  • Some participants propose alternative configurations for detectors, such as smaller distributed detectors or a structure around a black hole, to improve detection rates.
  • There is discussion about the challenges of creating single-graviton states and the current limitations in detecting such states, with references to the historical context of photon detection.
  • One participant mentions that demonstrating energy transfer in discrete steps does not require a single-graviton source, suggesting that current detectors could still show significant advancements.
  • Another point raised is the potential for inflation to probe the quanta of the gravitational field, though uniqueness of the signal may not be established.

Areas of Agreement / Disagreement

Participants express a range of views on the implications of graviton detection and the assumptions in proposed detection methods. There is no consensus on the feasibility of current detection methods or the theoretical implications for general relativity.

Contextual Notes

Participants highlight limitations in the assumptions made in the referenced paper, including the placement of detectors and the nature of detection mechanisms. The discussion also reflects uncertainty regarding the existence of single-graviton sources and the current state of quantum gravity theory.

KallaNikhil
If we were to able to detect gravitons then is it not that the basic assumption over which the general theory of relativity is flawed ?
 
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General relativity doesn't have gravitons. Yes.
It is expected that GR is only an approximation, the classical limit of some yet unknown theory of quantum gravity. This is similar to Newtonian mechanics which is an approximation of nonrelativistic quantum mechanics.
 
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KallaNikhil said:
If we were to able to detect gravitons

Note that we have not detected gravitons; we have only detected gravitational waves, which classical GR can and does predict and model.
 
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PeterDonis said:
Note that we have not detected gravitons
And we have no idea how to build a detector sensitive enough to see individual gravitons (unless there are extra dimensions or similar things).
 
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mfb said:
And we have no idea how to build a detector sensitive enough to see individual gravitons (unless there are extra dimensions or similar things).
Yes, I liked this paper on graviton detection: https://arxiv.org/abs/gr-qc/0601043
 
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An interesting paper. I'm a bit puzzled by the assumptions made there (e. g. to get equation 6.2). A Jupiter-sized detector is perfectly fine, but we can't get it closer than 100,000 light years to a black hole? Build it around the primordial black hole and you get R=100,000 km, a factor 1013 closer, or 1026 higher detection rate. Alternatively, you get the same detection rate with just 20 kg of detector material. The neutrino background stays a problem, of course.
The assumption that the detector readout happens at the surface of the Jupiter-sized detector only (p16) is odd as well.
 
mfb said:
An interesting paper. I'm a bit puzzled by the assumptions made there (e. g. to get equation 6.2). A Jupiter-sized detector is perfectly fine, but we can't get it closer than 100,000 light years to a black hole? Build it around the primordial black hole and you get R=100,000 km, a factor 1013 closer, or 1026 higher detection rate. Alternatively, you get the same detection rate with just 20 kg of detector material. The neutrino background stays a problem, of course.
The assumption that the detector readout happens at the surface of the Jupiter-sized detector only (p16) is odd as well.
Yeah, he is assuming we stay in the solar system, and that there do not happen to be any unusually close PBH.

As for the detector, through most of the paper, they do not assume only surface detectors. However, they do justify adding this constraint for more realism based on the mechanism of the proposed detector, and they then discuss ways to distribute detectors through a volume. Do you disagree with their electron mean free path discussion?
 
I don't disagree with the short mean free path, but if we have the methods to make such a large detector, we would instrument it in 3D like we do with current detectors. If we don't go closer to the source then there is no need to make a single large detector, multiple smaller ones would be fine. Closer to a source a ring around the source could work nicely, or some Dyson swarm like structure.
 
Another question I have is, how to create single-graviton states to begin with. Given the fact that not long ago it was pretty difficult to prepare single-photon states, and that "macroscopic electromagnetic waves" have been created and detected for more than 100 years now and we just are beginning to be able to detect macroscopic gravitational waves, I'd expect it to take some more decades to construct single-graviton sources and single-graviton detectors, provided either of them exist at all. Don't forget that we don't have a satisfying theory of quantum gravity yet!
 
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You don't need a single-graviton source to demonstrate that the energy is transferred only in discrete steps. As discussed in the paper, this is not the best possible demonstration of quantization of the radiation, but it would be a significant step beyond current detectors.
 
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  • #11
It has been argued that there is a sense in which inflation also probes the quanta of the gravitational field, but you wouldn't necessarily be able to show uniqueness (you could imagine different physics also contributing the same signal).

https://arxiv.org/abs/1309.5343
 

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