Internal (gauge) symmetries and spacetime symmetries

In summary: Once this distinction is understood, the Coleman-Mandula theorem becomes more comforting, and less of a nuisance.In summary, the Coleman-Mandula theorem states that internal symmetries of the SM -U(1), SU(2), SU(3)- cannot be combined with spacetime symmetries. However, there is one loophole: fermionic charges. Using SUSY, one can combine spacetime symmetries and internal symmetries. Super-gravitation SUGRA is a result of gauging SUSY.
  • #36
martinbn said:
What exactly is abstract space and (I guess) non-abstract?
I'll let you in on a secret: they're all abstract. But don't tell anyone. :-)

It's curious how this subject tends to generate more heat than I would have expected.

Rotations act on space and they act on the wave functions as well. Does that make them both physical and unphysical?
No, it just means that the abstract group ##SO(3)## is being represented as operators on different vector spaces.
 
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  • #37
TrickyDicky said:
try switching on a B-field in the context of a Aharonov–Bohm effect kind of experiment and you'll measure a phase shift obviously related to the local EM gauge.
Not sure what you mean by "obviously related" here. The phase difference observed in an A-B setup does not depend on local EM gauge. The closed line integral therein is gauge-invariant.
 
  • #38
TrickyDicky said:
I simply meant there are many loopholes in the [Coleman-Mandula] theorem, at least according to wikipedia, so that it can easily be avoided.
"Many loopholes"?? I found only a reference to the use of SUSY algebras, and a reference to 2D systems which admit different spin-statistics rules. The latter is not relevant for 4D field theory of elementary particles, and recent LHC results now make the former seem very unlikely.
 
  • #39
TrickyDicky said:
Yes, that is how gauge symmetries are formally prescribed, although in practice I wouldn't use such definite terms, ...
But you should ;-)

TrickyDicky said:
... try switching on a B-field in the context of a Aharonov–Bohm effect kind of experiment and you'll measure a phase shift obviously related to the local EM gauge.
The Aharonov-Bohm effect is due to a non-trivial global structure of the gauge fibre bundle; it does not measure a local phase as can be seen by varying either the path or the gauge infinitesimally; only changing the global structure i.e. the winding number (or the flux = the B-field) changes the Aharonov-Bohm phase.

TrickyDicky said:
... if you had an observable completely invariant to rotations, based only on that observable it is quite obvious you couldn't perform an experiment to show symmetry breaking.
Correct, but usually we are talking about a complete set observables. Even this complete set of observables cannot detect any gauge structure b/c all observables must be gauge invariant i.e. must commute with the generators of gauge transformations.
 
  • #40
Regarding a rigorous formulation, propositions and loopholes of the Coleman-Mandula theorem I recommend http://arxiv.org/pdf/hep-th/9605147v1.pdf

One loophole could be the existence of the S-matrix itself; it's by no means clear that the S-matrix can be defined for the full theory, not just on special regimes, spacetime backgrounds etc.
 
  • #41
TrickyDicky said:
[...] what Alain Connes is trying to with his noncommutative SM. [...]
IIRC, Connes' model ran into conflict with experiment back in 2008 when his favored Higgs mass prediction was ruled out:

http://noncommutativegeometry.blogspot.com.au/2008/08/irony.html

He seems not to have given up all hope however. In response to the recent CERN Higgs announcement, he posted this:

http://noncommutativegeometry.blogspot.com.au/2012/07/habemus-higgs.html

but doesn't reconcile the enhanced models (with incorporate SUSY) with the LHC exclusion results regarding SUSY models.
 
  • #42
strangerep said:
No, it just means that the abstract group ##SO(3)## is being represented as operators on different vector spaces.

What do you mean "no"! That's what I am saying.
 
  • #43
strangerep said:
Not sure what you mean by "obviously related" here. The phase difference observed in an A-B setup does not depend on local EM gauge. The closed line integral therein is gauge-invariant.

tom.stoer said:
The Aharonov-Bohm effect is due to a non-trivial global structure of the gauge fibre bundle; it does not measure a local phase as can be seen by varying either the path or the gauge infinitesimally; only changing the global structure i.e. the winding number (or the flux = the B-field) changes the Aharonov-Bohm phase.

Ok, so you are making a distinction between global and local gauge, but they are both gauge symmetries, right? How are they related? This is what I meant, that the global EM gauge should be related to the local EM gauge. Surely the phase shift measured is the global one, that is because mathematically the local one can't be measured by definition.
 
  • #44
The difference is the global structure auf the fibre bundle. In trivial cases this is the direct product of 4-spacetime * gauge group. Locally this is always true, at each spacetime point you have a copy of the gauge group. But globally this can be complicated and there is a non-trivial topology of the fibre bundle. In the case of the Aharonov-Bohm effect this is due to the string-like defect in 3-space. Now there exists a winding number structure on the fibre bundle which means that gauge transformations fall into categories labelled by the winding number. Field configurations can now be related by small gauge transformations or by large ones; for large ones they be transformed continuously to each other by local transformations w/o violating the winding number.

Think about a circle S1 and a gauge group U(1) which is usually written as

[tex]U[\theta]= \exp(2\pi i \theta(x))[/tex]

with gauge function θ(x)

In contrast the the real line x is now an angle variable in the intervall [0,1]; the gauge group contains all gauge transformations which are periodic, i.e.

[tex]U[\theta(x+2\pi)] = U[\theta(x)] [/tex]

Other functions θ(x) would violate the topology of fields living on S1. Therfeore the (topology of the) gauge group is different for x living on a circle and x living on the real line!

Now think about a family of gauge functions

[tex]\theta_s(x) = s\,\theta(x)[/tex]

For small θ(x) this is an allowed family, i.e. every θs(x) is a valid gauge function.

But now look at the simple function

[tex]\theta(x) = x[/tex]

with
[tex]\theta(0) = 0[/tex]
[tex]\theta(1) = 1[/tex]

[tex]U[\theta(x=0)]=\exp(2\pi i \theta(0)) = \exp(0) = 1 = \exp(2\pi i) = \exp(2\pi i \theta(1)) = U[\theta(x=1)][/tex]

U is still periodic but θ isn't!

Nevertheless U is a valid gauge transformation b/c it respects the periodicity of S1.

But in that case the family

[tex]\theta_s(x) = s\,\theta(x) = sx[/tex]

is no longer a valid family of gauge functions; only s=0, s=±1, s=±2, ... are allowed!

These are exactly the representatives of different classes of gauge functions, one for each winding number n = 0, ±1, ±2, ... In general the functions

[tex]\theta_n(x) = nx[/tex]

are valid functions for integer n: going round the S1 circle from x=0 to x=1 exactly once the gauge transformation U[θn] runs around the circle n times:

[tex]U[\theta_n]= \exp(2\pi i \theta_n(x)) = \exp(2\pi i n x)[/tex]

For fixed winding number n small fluctuations of the gauge functions are still llowed, i.e. if you have small functions covering the n=0 case, an arbitrary gauge transformation can be written as

[tex]U[\theta_n]= \exp(2\pi i \theta_n(x)) = \exp(2\pi i (nx + \tilde{\theta}(x))[/tex]

where the second function is always a small one with winding number 0.

In the case of the Aharonov-Bohm effect the winding number becomes a physical observable whereas the small gauge transformations are still unphysical i.e. non-observable.
 
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  • #45
Thanks for all that info, Tom.
Some parts are over my head but I think I get the picture of the topological defect explanation of the effect.
Now, let us consider an alternative, or complementary, take on this. Instead of going directly to the fiber bundle structure of the circle group we could think that actually what we perceive as U(1) is not just U(1) but a broader group symmetry that has it as subgroup and that under certain set ups behaves like a global defect. This is the kind of approach I was thinking of in the OP.
 
  • #46
But my impression was that out of this broader symmetry group you may want to derive both spacetime and internal symmetries. This is - as far as we know - not possible for rather general conditions.

As I said: the Coleman-Mandula-theorem is derived in the context of the S-matrix. What happens if I have a theory which does not allow for the definition of an S-matrix in all its regimes?
 
  • #47
martinbn said:
What do you mean "no"! That's what I am saying.
My "no" was in answer to your question about whether "that makes [rotations] both physical and unphysical".
 
  • #48
tom.stoer said:
[...] the Coleman-Mandula-theorem is derived in the context of the S-matrix. What happens if I have a theory which does not allow for the definition of an S-matrix in all its regimes?
What exactly do you mean by "regimes" here?
 
  • #49
tom.stoer said:
But my impression was that out of this broader symmetry group you may want to derive both spacetime and internal symmetries. This is - as far as we know - not possible for rather general conditions.

As I said: the Coleman-Mandula-theorem is derived in the context of the S-matrix. What happens if I have a theory which does not allow for the definition of an S-matrix in all its regimes?

Yes, then you can combine internal and spacetime symmetries in a non-trivial way.
But then you'd need a non-SM theory, without mass gap and with a true spontaneous symmetry breaking (unlike the Higgs mechanism of symmetry breaking), correct?
 
  • #50
I do not want to identify specific loopholes for a given framework (quantum field theory on spacetime, operators, S-matrix, ...) but I want to question the framework itself!

QCD formulated in it's fundamental d.o.f. has a "confinement-regime" where an S-matrix for asymptotic quarks and gluon states does not exist. So strictly speaking the framework of the Coleman-Mandula theorem does not apply for QCD as a whole. I guess the same could be true for strongly coupled gravity in a deep quantum gravity regime where an S-matrix (for gravitons) may become meaningless.

Formulating theories for emergent or discrete spacetime like (colored) spin networks may render the concept for "S-matrix on spacetime" meaningless. The question then is whether you can still use this S-matrix approach which is restrcited to a certain regime to derive a no-go theorem for the whole theory. I doubt that this will work and therefore I expect that many of these no-go theorems will cease to exist when identifying a fundamental theory of quantum gravity. Besides the Coleman-Mandula theorem the Weinberg–Witten theorem is another candidate to fail.
 
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  • #51
tom.stoer said:
I do not want to identify specific loopholes for a given framework (quantum field theory on spacetime, operators, S-matrix, ...) but I want to question the framework itself!
Hey, didn't know you were so radical.:-p
tom.stoer said:
Formulating theories for emergent or discrete spacetime like (colored) spin networks may render the concept for "S-matrix on spacetime" meaningless. The question then is whether you can still use this S-matrix approach which is restrcited to a certain regime to derive a no-go theorem for the whole theory. I doubt that this will work and therefore I expect that many of these no-go theorems will cease to exist when identifying a fundamental theory of quantum gravity. Besides the Coleman-Mandula theorem the Weinberg–Witten theorem is another candidate to fail.

I share this view about no-go theorems.
 
  • #52
TrickyDicky said:
Hey, didn't know you were so radical.:-p
depends on the enemy ...
 
  • #53
tom.stoer said:
I doubt that this will work and therefore I expect that many of these no-go theorems will cease to exist when identifying a fundamental theory of quantum gravity.

Now I have a question bearing some level of radicalness :)

Is there an empirical reason to be led to believe that gravity is (or should be) quantized? Or is it principally a consistency in frameworks that one assumes should be accommodated?
 
  • #54
PhilDSP said:
Now I have a question bearing some level of radicalness :)

Is there an empirical reason to be led to believe that gravity is (or should be) quantized? Or is it principally a consistency in frameworks that one assumes should be accommodated?

I remember having read somewhere a physicist that claimed that gravity was already "quantized" in GR. I will try to find the reference because I can't remember what kind of arguments he used or what he meant.
 
  • #55
PhilDSP said:
Is there an empirical reason to be led to believe that gravity is (or should be) quantized? Or is it principally a consistency in frameworks that one assumes should be accommodated?
There is no direct experimental evidence for quantum gravity, so I would say that the indications are mostly due to theoretical and consistency reasons; but there are a lot ...
 

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