ranyart
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Originally posted by eigenguy
A rabbi and priest in a rowboat...
Indeed two 'Ed's' are better than one?

Originally posted by eigenguy
A rabbi and priest in a rowboat...
lemme see..Originally posted by Urs
Ok, here is a simple exercise that everybody who has followed our discussion should be able to solve:
start with Minkowski space, no background field:1) Consider the Nambu-Goto action in 1+0 dimensions, which describes the free relativistic particle in Minkowski space (alternatively, for those who enjoy a bigger challenge: the charged particle in curved space with an electromagnetic field turned on)
from the expression for the canonical momentum, we see that2) Compute the single constraint of the theory.
3) Do a Dirac quantization by promoting this single constraint to an operator equation. Discuss the resulting quantum equation.
Originally posted by Urs
You have derived the classical constraint. Quantize it. Then impose Dirac quantization of constraints. Alternatively, impose LQG quantization of constraints. What do you get?
Originally posted by eforgy
PPS: I'd have no idea how to loop quantize this and I HAVE been following this thread :)
Originally posted by Urs
Hi Eric -
yes, in your second post you demonstrate that exponentiating the KG constraint and demanding invariance yields the same thing as usual. The point is that LQG-like quantization allows you to exponentiate anything else, on any other Hilbert space and call it a quantization of the relativistic particle.
yeah, i think they saw the pion already in the 30sOriginally posted by selfAdjoint
And has anyone ever seen a KG particle, quantized or otherwise?
Originally posted by marcus
This is the main algebraic difference between the LQG "lowest-A-number"
reps and LE reps. This is an essential difference; in infinite
dimension, there is no Stone-von Neumann theorem that makes different
vacua equivalent.
--------------end of post-----------------
hmm... my knowledge of classical mechanics is a little insufficient here. the definition of "First class constraint" that i mentioned above is that it is a constraint which holds even if the equaiton of motion is not satisfied.Originally posted by Urs
By the way:
First-class constraints are those whose Poisson bracket closes on the set of constraints, i.e. is a linear combination of any of the constraints of the theory. Second class constraints are those whose Poisson brackte does not give another constraint.
OK, so you just impose the operator version of the constraint.Originally posted by Urs
As you said, the operator version of the single constraint of the free relativistic particle is obtained by the usual correspondence rule
p^\mu \to \hat p^\mu = -i \hbar \frac{\partial}{\partial x^\mu} and yields nothing but the Klein-Gordon equation
<br /> \partial^\mu \partial_\mu \phi = -m^2 \phi<br />
(up to factors of c,\hbar).
Now let's see how LQG tells us to quantize the free relativistic particle:
There we are told not to consider the constraint \varphi itself but the group which is generated by it by means of Poisson brackets. I.e. we are supposed to look at the group elements
<br /> U(\tau) = \exp\left([\phi,\cdot]_\mathrm{PB}\right)<br />
where [\cdot,\cdot]_\mathrm{PB} is the Poisson bracket and this guy is supposed to act on classical observables, i.e. functions on phase space.
OK, so they are considering representations of the group generated by the constraint, instead of the constraint itself.
But we could also choose something very different. This is the great ambiguity that I was referring to. For instance, if we followed the tretament by Ashtekar, Fairhurst and Willis of the LQG-like quantization of the 1d nonrelativistic particle, than we'd want to use a nonseparable Hilbert space on which the momentum operator \hat p is not representable. In this case, which is the precise analog of what Thomas Thiemann does in the 'LQG-string' the above choice for \hat U is not an option.
for some reason i thought there was some issue about imposing only the expectation value of the constraint, as in Gupta-Bleuler. but i guess not.
but in the relativistic theory, we don't have these canonical commutation relations, since there is no time operator,
hmm... why is this thing a group now? i guess the Poisson algebra of observables is a Lie algebra, so we might expect that exponentiating it would yield a group, but i believe that infinite dimensional Lie algebras do not always exponentiate to Lie groups, only with finite dimensional Lie algebras do we have this guarantee.
OK, so they are considering representations of the group generated by the constraint, instead of the constraint itself.
this is the same way the Stone-von Neumann theorem goes, right? it says that there is only one theory that satisfies the exponetiation of the canonical commutation relations (the Weyl relation, i think this is called?). but i have read on s.p.r that there can be inequivalent (and perhaps even physically relevant) representations of the commutation relations themselves
so it seems like the choice to only look at the group version loses you generality?
so this choice is what allows Thiemann to get rid of the anomoly?
so what do you mean that the Poisson bracket closes on the set of constraints?
i will check for a reference shortly, i am just talking out of my memory from class, so take it with a grain of salt, but i believe that the virasoro algebra does not generate a group. it generates conformal transformations in 2D, right? and something about there being local conformal transformations that do not have an inverse globally, and hence to not form a group.Originally posted by Urs
I am not aware of the problems that you are hinting at, do you have a reference? Note that in the case of the Virasoro algebra, which is infinite dimensional of course, the classical group does exist all right. In any case, this would not affect the KG particle, which clearly has a finite constraint algebra.
Originally posted by lethe
can we impose a more basis independent quantization procedure here?
i infer from this expression that you have an operator on your Hilbert space \hat x^0 that acts on states like multiplication by t. this is the straightforward application of the nonrelativistic quantization to the relativistic particle.Originally posted by Urs
I am not sure why you think so. We have
<br /> [\hat x^\mu , \hat p^\nu] \sim \eta^{\mu\nu}<br />
which translates to
<br /> [\partial_\mu , x^\nu] = \delta_\mu^\nu<br />
There is however a subtlety with defining the Hilbert space of physical states, since these do not live in L^2(M^4), obviously (since they don't decay in the time direction). There are many ways to handle this, the most elegant and advanced being gauige fixing by means of BRST methods. But for our discussion all this does not really matter.
Originally posted by Urs
Note that in the case of the Virasoro algebra, which is infinite dimensional of course, the classical group does exist all right. In any case, this would not affect the KG particle, which clearly has a finite constraint algebra.
Originally posted by Urs
lethe -
right, exponentiating a Lie algebra always only gives you the group locally.
yes, actually, i have read the paper you reference here, and i think that paper is exactly what i had in mind with my above comments.Originally posted by Urs
Yes! That's the point. But note that 'representing the constraints themselves' is usually accompanied by much more structure. We are not just looking for any set of operators which has the same algebra as the constraints. We want these operators to be built from the canonical data of the classical system, i.e. canonical coordinates and momenta, by some sort of 'correspondence rule'. All this information about the physical system is lost in the 'represent the group without the rest'-approach.
Stone-von Neumann says that iff the Weyl algebra is represented weakly continuously, then the canonical coordinates and momenta \hat x,\hat p do exist as operators, too, otherwise they do not. And if they exist the Weyl algebra elements are the exponetiations of the Heisenberg algebra elements. See http://citeseer.nj.nec.com/355097.html
see my above complaint. in short, there is only one rep of the exponentiated unitary form, and uncountably many reps of the self-adjoint non-exponentiated form of the CCR. so i conclude that the latter is more general, it allows for more systems. should i not conlcude that there is some ambiguity in choosing such a rep?No, it gives you too much generality. Using these strange reps it is possible to built strange theories.
Originally posted by Urs
For more details on the quantization of the KG particle and its relations to non-relativistic QM you might want to have a look at http://www-stud.uni-essen.de/~sb0264/TimeInQM.html
Originally posted by lethe
i infer from this expression that you have an operator on your Hilbert space \hat x^0 that acts on states like multiplication by t. this is the straightforward application of the nonrelativistic quantization to the relativistic particle.
but something that i have learned from reading s.p.r is that there is no such operator. since learning that fact, it has been a big question mark in my mind as to whether there actually exists a theory that could really be called relativistic quantum mechanics of a particle.
i have wanted to understand what is going on with that for a while. since we were doing quantization of the relativistic particle, i thought i would toss in a question about that for you, but i can certainly appreciate that it is a bit off topic for the current discussion.
hidden variable network? wtf?Originally posted by ranyart
When one moves from a Three Dimensional Relativistic network, down into the Quantum Mechanical 'Hidden-Variable-Network',
hidden variable network? wtf?
Originally posted by Urs
As far as I remember the argument is that there cannot, because two operators satisfying a CCR as will act like multiplication/differentiation with respect to each other's eigenvalues and hence be unbounded from below and from above. But the spectrum of a decent Hamiltonian is supposed to be bounded from below (have a ground state), so it cannot satisfy any CCR.
ok, this is interestingBut this argument doe not apply to systems which do not have an ordinary Hamiltonian. For instance the KG particle that we were discussing is governed by a constraint, not a Hamiltonian evolution. Here time is on par with the spatial dimenions.
i think i can see that now. thank you, that was very helpful for me.If you wish, you can regard the constraint of the KG particle as the Hamiltonian with respect to parameter evolution, where the parameter is an auxiliary variable along the worldline of the particle. This plays formally the role of time in non-relativistic QM and the above argument would show that there is not operator associated with the worldline parameter which has the CCR with the constraint.
before i think about your point here, I am confused as to what you are referring to when you say "Weyl algebra". i am thinking it should be the set of operators you get after exponentiation, but do these things form an algebra? i expect them to form a group, but i wouldn't expect the sum of two of these guys to be another one of these guys.Regarding your summary of the Stone-vonNeumann theorem I do not quite agree. I think the message is that there are many reps of the Weyl algebra and that if and only if these reps are weakly continuous does the Heisenberg algebra exist and then the Weyl rep is the exponentiation of the Heisenberg algebra.
LQG like approaches play with the possibility that even if the Heisenberg algebra does not have a rep still a rep of the Weyl algebra exists.
in short, the operators in the Weyl relation are the Lie group corresponding to the Lie algebra spanned by the operators in the canonical commutation relations (the Heisenberg algebra)
Originally posted by Urs
Maybe, maybe, maybe he is thinking of Smolin's latest attempt at merging Nelson's stochastic QM with quantum gravity
http://xxx.uni-augsburg.de/abs/gr-qc/0311059
where spin networks are indeed used as 'hidden variables' to produce QM dynamics from classical statistics.
Last time Lee Smolin tried the same with BFSS Matrix Theory
http://xxx.uni-augsburg.de/abs/hep-th/0201031 .
I used to consider this interesting,
http://groups.google.de/groups?selm=ahe52s$1a2q$1@rs04.hrz.uni-essen.de
though I am not so sure anymore.
Anyway, this is what ranyart's avant-garde poetry reminded me of. As with every piece of modern art, you have to search the answer within yourself. ;-)
QM from QG
Originally posted by ranyart
This paper has some relevence to this post.
http://arxiv.org/PS_cache/hep-th/pdf/0403/0403108.pdf
many-particle ... can you explain more?Originally posted by arivero
... the string is already by itself a many-particle entity
selfAdjoint said:"...at least in the case of the quantum oscillator the polymer state is unphysical." That seems to be the death-knell fot the Thiemann approach. I wasn't aware of the fierce properties of the polymer state (no momenta), which as the authors say, is much used in LQG derivations. Back to the drawing board.