Thursday, February 12, 2015

quantum mechanics - Is the boost operator conserved (in the context of QFT)?


Let Jμν be the generators of Lorentz transformations, so that Jij generates rotations, and J0i generates boosts. The algebra of the Poincaré Group contains [Pμ,Jαβ]=i(ημαPβημβPα)


The μ=0 component of this relation is the commutator of Jαβ with the Hamiltonian. For example, in the case of rotations, it implies [H,Jij]=0

so that angular momentum is conserved.



On the other hand, in the case of boosts, it implies [H,J0i]=iPi

so, apparently, the boost operators don't commute with the Hamiltonian. The only way to make J0i to be conserved is to assume that it is explicitly time-dependent, so that ˙J0i=i[H,J0i]+0J0i


If we take 0J0i=Pi, then we find that ˙J0i=0, and this operator is conserved.


Question. Is there any "first principles" reason as to why we should take 0J0i=Pi? Or are the boost operators not conserved in general?




I know that in the framework of canonical quantisation, we take the Jμν operators to be Jμν=dx xμPνxνPμ+spin part

so that we indeed have 0J0i=Pi. But this clearly relies on the existence of a Lagrangian, and on the assumption that the generators of the Poincaré Group must be those given by Noether's formula, and on all the details of canonical quantisation in general (which IMHO is justified only because of consistency, but there is no "first principles" reason to many of its ingredients). I am interested in the properties of the Poincaré Group without any reference to a Lagrangian or to "quantisation" of a classical system.



Answer



Let us suppose that G is a Lie group admitting some faithful unitary strongly continuous representation U on a Hilbert space H, so that we can interpret the elements a of the Lie algebra of G in terms of self-adjoint generators of one-parameter unitary groups,


U(exp(sa))=eisA.


The operators A are self-adjoint and are commonly defined in a dense subdomain called Garding space where they are essentially self-adjoint (another interesting domain is the one constructed by Nelson where the exponential in the right-hand side may be developed as in its standard Taylor series).


If G is the largest group of continuous symmetries of the quantum system, one of these one-parameter subgroups should represent the temporal evolution of the system. Let us suppose that it is the group generated by the element h of the Lie algebra of G. We therefore have



U(exp(th))=eitH


I changed the sign since the time evolution is the inverse operation of the time translation. H, by definition, is the Hamiltonian observable of the system. Obviously some physical requirements are necessary on H, first of all its spectrum must be bounded below etc...I do not stick on them here and I henceforth suppose that H is a well-behaved physical Hamiltonian.


Now we have two possibilities, if a is a generic element of the Lie algebra. One is ({,} is the standard Lie algebra commutator)


{h,a}=0.


As a consequence of Hausdorff - Baker - Campbell equality in G, we can exponentiate this identity to a group identity


exp(th)exp(sa)exp(th)=exp(sa)t,sR.

Applying the representation U: eitHesAeitH=esAt,sR.
Taking advantage of Stone theorem, taking the strong derivative in s we immediately obtain eitHAeitH=AtR.
(This identity is completely well-posed even regarding subtleties with domains.) This identity says nothing but that the Heisenberg evolution of the observable A is constant and thus A is a constant of motion.


What happens if instead {h,a}0?.

In this case we have exp(th)exp(sa)exp(th)=exp(sa(t))t,sR.
where we have used the natural action of gG over its Lie algebra, ag1ag
and we have defined the element of the Lie algebra a(t) a(t):=exp(th)aexp(th)tR.


Fixing a basis a1,,an of the Lie algebra, a=jcjajfor some reals cj

and thus a(t)=jcj(t)ajfor some real valued functions cj=cj(t)
the found identity can be rephrased to exp(th)exp(sa)exp(th)=exp(nj=1sa(t))t,sA.
Exploiting again the theorem by Stone we conclude that for an observable constructed out of the self-adjoint generators Aj (corresponding to the basis of the aj), A=jcjAjfor some reals cj
it holds eitHAeitH=nj=1cj(t)AjtR.
(This identity is valid on Garding space and can be extended into a true identity between self-adjoint opertators taking the closures of both sides). The physical content of the found identity is that,


even if the representative A of the Lie algebra of observables is not a constant of motion, its "à la Heisenberg" evolution is however described in terms of a linear combination of the generators and the time dependence affects the numerical coefficients only.


This is a highly non-trivial result. Actually, the result can be turned into a statement concerning existence of constants of motion parametrically depending on time. This is the standard procedure usually adopted in QFT, especially for the boost generator.



Assuming that (4) is valid, one define the observable parametrically depending on time in Schroedinger picture (and once again the dependence on time just appears in the coefficients)


AS(t):=nj=1cj(t)Aj


With this definition


AS(0):=A


and, from (4), where Ut:=eitH


AH(t):=UtAS(t)Ut:=AS(0)tR

which, formally, on some domain could be re-written tAH(t)+i[H,AH(t)]=0.


If G is the Poincare' group, the boost generators Kj are treated that way. One defines the time-parametrized boost operators KSj(t) in the Schroedinger picture which always take a form like this where j=1,2,3, KSj(t)=KjtZj

where Zj is a certain constant linear combination of the generators of the Lie algebra and K is the standard boost generator you get by the commutation relations. In QFT it has a contribution due to the spin and an orbital part. K is important because it is related with the relativistic position operator as it can be understood if performing the non relativistic limit (i.e. replacing the Poincaré group with Galilei's group) KSj(t)=mXjtPj,
where m is the mass of the system and Xj the position of its center of mass.


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