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Observational Loop QG--your opinion.
Please read Bee Hossenfelder's recent post on this topic--you might also wish to glance at the papers/talks she discusses, if you haven't already done so.
http://backreaction.blogspot.com/2009/06/constraining-modified-dispersion.html
To what extent is the development of LQG (now primarily the spinfoam approach) being guided by astrophysics observations?
To what extent is it being tested by astro and collider experiments? Is LQG falsifiable at current collider energies?
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Guidance is a looser less restrictive idea than falsifiability, and less technically stringent.
It is pretty clear that Loop research is influenced by the connection with DSR (deformed special rel) and it's significant which type of DSR you make a bridge to. Recent observations of delayed high energy photons tend to favor the type of DSR in which very high energy particles see more bumps in the geometry and have a longer harder road to travel, so can be very very slightly delayed. Or more generally, for whatever reason, in those versions the high energy photons appear to propagate slower thru the quantum geometry.
On the other hand, recent observations make less interesting the version(s) of DSR where higher energy photons have an advantage and arrive sooner. This gives Loop researchers some valuable clues or guidance in relation to DSR, but of course nothing here is confirmed yet. A lot more gammaray bursts need to be observed in order to establish that there is or is not a dispersion effect.
Strict falsifiability by experiment is a more demanding and technical matter. Of course presentday LQG is empirically testable/falsifiable because it assumes there are no extra space dimensions accessible at any energy. I doubt that extra space dimensions will ever be detected (it seems like a silly made-up idea for which there is no evidence) but if they were then today's LQG theories would be instantly out the window. It's quite a robust test.
To clarify the point by way of contrast, string extra dimensions are not being empirically tested because if one finds no evidence for them at a given level of energy one can imagine that you just have to look at some higher energy and they will appear. There is no falsifiability involved.
But subjectively it seems a bit unsatisfactory because of the unliklihood of LQG being falsified this way. One would like a test that LQG has more chance of failing.
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So what do you think? I tend to agree with Bee Hossenfelder that what we are seen now is simple guidance. IOW that researchers in the field now have the potential to be guided by the gammaray observation data that is now coming in.
Here's an earlier PF thread about the main paper Bee talks about:
https://www.physicsforums.com/showthread.php?p=2248613#post2248613
Please read Bee Hossenfelder's recent post on this topic--you might also wish to glance at the papers/talks she discusses, if you haven't already done so.
http://backreaction.blogspot.com/2009/06/constraining-modified-dispersion.html
To what extent is the development of LQG (now primarily the spinfoam approach) being guided by astrophysics observations?
To what extent is it being tested by astro and collider experiments? Is LQG falsifiable at current collider energies?
============
Guidance is a looser less restrictive idea than falsifiability, and less technically stringent.
It is pretty clear that Loop research is influenced by the connection with DSR (deformed special rel) and it's significant which type of DSR you make a bridge to. Recent observations of delayed high energy photons tend to favor the type of DSR in which very high energy particles see more bumps in the geometry and have a longer harder road to travel, so can be very very slightly delayed. Or more generally, for whatever reason, in those versions the high energy photons appear to propagate slower thru the quantum geometry.
On the other hand, recent observations make less interesting the version(s) of DSR where higher energy photons have an advantage and arrive sooner. This gives Loop researchers some valuable clues or guidance in relation to DSR, but of course nothing here is confirmed yet. A lot more gammaray bursts need to be observed in order to establish that there is or is not a dispersion effect.
Strict falsifiability by experiment is a more demanding and technical matter. Of course presentday LQG is empirically testable/falsifiable because it assumes there are no extra space dimensions accessible at any energy. I doubt that extra space dimensions will ever be detected (it seems like a silly made-up idea for which there is no evidence) but if they were then today's LQG theories would be instantly out the window. It's quite a robust test.
To clarify the point by way of contrast, string extra dimensions are not being empirically tested because if one finds no evidence for them at a given level of energy one can imagine that you just have to look at some higher energy and they will appear. There is no falsifiability involved.
But subjectively it seems a bit unsatisfactory because of the unliklihood of LQG being falsified this way. One would like a test that LQG has more chance of failing.
================
So what do you think? I tend to agree with Bee Hossenfelder that what we are seen now is simple guidance. IOW that researchers in the field now have the potential to be guided by the gammaray observation data that is now coming in.
Here's an earlier PF thread about the main paper Bee talks about:
https://www.physicsforums.com/showthread.php?p=2248613#post2248613
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