Decay through gravitional interaction

Click For Summary

Discussion Overview

The discussion revolves around the concept of particle decay through gravitational interaction, exploring theoretical implications, potential mechanisms, and the role of gravitons. Participants examine the feasibility of gravitational decay in the context of fundamental forces, particularly focusing on conditions under which such decay might occur, and the characteristics of particles involved in these processes.

Discussion Character

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

Main Points Raised

  • Some participants assert that the gravitational force is too weak for particle decay, while others propose that under certain conditions, such as high-energy states, gravitational decay could theoretically occur.
  • There is discussion about the emission of gravitons during decay processes, with some suggesting that angular momentum selection rules apply similarly to graviton emission as they do to photon emission.
  • One participant mentions specific decay processes, such as eta -> pi0 + G, that could occur gravitationally, although the rates are considered negligible.
  • Concerns are raised about the lack of evidence for changes in the strength of gravitational interactions over time, with some arguing that high-energy processes can occur today.
  • Participants discuss estimates of branching ratios for positronium decay to photons versus gravitons, noting that older estimates suggest a significant disparity in likelihood.
  • There is a question regarding the predictability of graviton emission despite gravitons being theoretical, with some participants suggesting that if gravity can be quantized, certain properties can be inferred.
  • One participant draws a parallel between the theoretical prediction of graviton emission and the earlier theoretical predictions of the Higgs boson.

Areas of Agreement / Disagreement

Participants express a mix of agreement and disagreement regarding the feasibility and implications of gravitational decay. While some acknowledge the theoretical possibility of such decay, others emphasize the practical insignificance and lack of empirical evidence supporting it. The discussion remains unresolved on several key points, particularly regarding the nature and role of gravitons in decay processes.

Contextual Notes

Limitations include the speculative nature of graviton emission, the dependence on theoretical frameworks for quantizing gravity, and the unresolved status of certain mathematical estimates related to decay rates.

Garlic
Gold Member
Messages
181
Reaction score
72
Hello,
I know that the gravitational force is the weakest of all forces (it is 10^-38 times weaker than the strong force), so it isn't possible a particle to decay through gravitational interaction. As far as I know, the strength of fundamental forces can change during different ages of the universe, because of the overall temperature of the universe etc. Let's say sometime the gravitational force (was/will be) strong enough that a particle can decay through gravitational interaction when given the right conditions, how would the decay equations look like?
When decaying through weak interaction, we see quark favours change themselves, during electromagnetical decay, photons can be emitted etc. Which attribute of a particle/an atom would change during gravitational decay? Would gravitons be emitted?

And are virtual gravitons predicted to be mediating force (for doing something) inside a nucleus?
Thank you
 
Physics news on Phys.org
The weakness is not the fundamental reason. There is also no known gravitational coupling that would change the particle type. Black holes are an exception, but calling that a "particle decay" can be questionable.

Virtual gravitons can mediate a tiny attractive force in a nucleus that has no relevance because it is so tiny.

Garlic said:
As far as I know, the strength of fundamental forces can change during different ages of the universe
There is no indication that the strength would have changed in any way. The strength depends on the energy scale, but high-energetic processes were not limited to the past, they happen today as well.
 
In principle, an atom or molecule can decay from an excited state to a lower-energy state by graviton emission, just like it can decay by photon emission. The rates are so small as to be completely negligible, but they are not zero in general. There are angular momentum selection rules that follow from the graviton having spin 2, just like there are angular momentum selection rules for photon emission that follow from the photon having spin 1.
 
As Avodyne points out, there are decays (eta -> pi0 + G would be one) that can proceed gravitationally. The rates are so small that in the entire history of the universe there has probably never been such a decay. On the issue of the strength of the gravitational interaction changing over time, there's no evidence of that, but in any event, it can't be tested by a process that, even though technically non-zero, as a practical matter doesn't occur.
 
Vanadium 50 said:
As Avodyne points out, there are decays (eta -> pi0 + G would be one) that can proceed gravitationally. The rates are so small that in the entire history of the universe there has probably never been such a decay.
I have seen the estimate of a branching ratio between positronium decay to photons and to gravitons as 1040. But that estimate was 50 years old. For comparison, the branching ratio between positronium decay to photons and to neutrinos was in the region of 1020.
Any more modern estimates?
 
The 10^40 should be about right. Roughly, the fine structure constant ##\alpha## gets replaced by ##Gm^2##, where ##G## is Newton's constant and ##m## is the electron mass, and I am using natural units with ##\hbar=c=1##. Roughly, ##Gm^2/\alpha \sim 10^{-20}##. The positronium decay rate to photons is proportional to ##\alpha^2##, so decay to gravitons should be smaller by ##10^{-40}##. But there are ##2\pi##'s to get right, and differing numerical factors from the different spins of the photon and graviton, etc.
 
How can graviton emission be predicted, even though gravitons are theoretical particles?
 
If gravity can be quantized we know some of its properties - it has to reproduce classical gravitational fields. We know the interaction strength, the spin of possible gravitons (2) and so on. Factors of 2 pi are up to the specific unknown theory but they won't change the result by many orders of magnitude.
 
How could Higgs boson production be predicted back when it was a theoretical particle?
 
  • Like
Likes   Reactions: mfb

Similar threads

  • · Replies 4 ·
Replies
4
Views
5K
  • · Replies 32 ·
2
Replies
32
Views
5K
  • · Replies 1 ·
Replies
1
Views
4K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 37 ·
2
Replies
37
Views
6K
  • · Replies 10 ·
Replies
10
Views
5K
  • · Replies 6 ·
Replies
6
Views
5K
  • · Replies 3 ·
Replies
3
Views
3K