Integral challenges physics beyond Einstein

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Discussion Overview

The discussion centers around the implications of results from the ESA's Integral gamma-ray observatory regarding the nature of space at quantum scales, particularly in relation to theories of quantum gravity, such as Loop Quantum Gravity (LQG) and String Theory. Participants explore the concept of 'graininess' of space and its potential limits, as well as the compatibility of various theoretical frameworks with these findings.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants highlight that Integral's observations suggest quantum graininess must be at scales smaller than 10^-48 m, which challenges existing theories like LQG that posit a minimal length at the Planck scale (10^-35 m).
  • Others express confusion over the implications of the results, noting that the ESA article does not clarify whether the graininess itself must be smaller or if the effects of such grains need to be smaller.
  • One participant mentions that while String Theory includes discrete grains in certain formulations, it does not necessarily violate Lorentz invariance, raising questions about the applicability of the results to various models.
  • Another participant suggests that Horava Gravity and possibly Causal Dynamical Triangulations (CDT) might be affected by the findings.
  • Concerns are raised regarding the clarity of the derivation of the 10^-48 m limit and its implications for discrete models of space.
  • Some participants reference earlier claims about LQG's predictions regarding vacuum dispersion, noting that current practitioners may not support those predictions anymore.

Areas of Agreement / Disagreement

Participants express differing interpretations of the implications of the Integral results, particularly regarding the relationship between quantum graininess and Lorentz invariance. There is no consensus on how these findings affect various theories of quantum gravity, indicating ongoing debate and uncertainty.

Contextual Notes

Participants note limitations in the clarity of the ESA article and the derivation of the 10^-48 m limit, as well as the potential for multiple interpretations of the results in relation to existing theories.

stevebd1
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ESA article

http://www.esa.int/esaCP/SEM5B34TBPG_index_0.html"

30 June 2011

'ESA’s Integral gamma-ray observatory has provided results that will dramatically affect the search for physics beyond Einstein. It has shown that any underlying quantum ‘graininess’ of space must be at much smaller scales than previously predicted.

Einstein’s General Theory of Relativity describes the properties of gravity and assumes that space is a smooth, continuous fabric. Yet quantum theory suggests that space should be grainy at the smallest scales, like sand on a beach.
One of the great concerns of modern physics is to marry these two concepts into a single theory of quantum gravity.

Now, Integral has placed stringent new limits on the size of these quantum ‘grains’ in space, showing them to be much smaller than some quantum gravity ideas would suggest...'
 
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Thanks for the link stevebd1

Let me quote the interesting part :
"Some theories suggest that the quantum nature of space should manifest itself at the ‘Planck scale’: the minuscule 10-35 of a metre, where a millimetre is 10-3 m.

However, Integral’s observations are about 10 000 times more accurate than any previous and show that any quantum graininess must be at a level of 10-48 m or smaller.
"

If I am right, in literature LQG defines minimal length to be 10-33cm (planck length). So if it is confirmed, that may be the first experimental result against LQG..

I have no idea if ST predicts any minimal length for space. Can anybody tell me ?
 
isnt it odd that the scale of space time grainess is smaller than the plank scale
 
I think there is some confusion here, that the ESA article doesn't help to clarify.

Even String Theory has discrete "grains" in Matrix theory versions. However Matrix theory is not Lorentz Violating.

I think what the result shows is, if your model has explicit lorentz violation then that violation must occur below 10^48m (although this length is only mentioned directly in the esa article).

So naive lattice models of space would have to have a finer graininess to be consistent with this result.

Most discrete models don't specify a scale at which lorentz violation would occur,so not sure if the result is that useful.
 
Sounds to me like this might relate to claims by Smolin and others a while back that LQG made definite predictions about the dispersion of the vacuum...? I don't think LQG practitioners believe these days that there is any such prediction.
 
Horava Gravity would likely be affected by this. And maybe CDT (apparently equiv to Horava gravity anyway).
 
Unfortunately we have two threads regarding the same topic; so I'll post my comment here as well:

I think the statement
It has shown that any underlying quantum 'graininess' of space must be at much smaller scales than previously predicted
is missleading b/c it suggests that the "grains" themselves must be much smaller - which is not necessarily the case. Instead the effects of these grains need to be much smaller. So if there is a theory which is compatible with Planck-space grains but w/o any violation or deformation of Lorentz invariance at all (like LQG) then this theory remains to be a perfectly valid candidate theory for quantum gravity.
 

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