- First class constraint
In
Hamiltonian mechanics , consider asymplectic manifold "M" with a smooth Hamiltonian over it (for field theories, "M" would be infinite-dimensional).Poisson brackets
Suppose we have some constraints : for "n" smooth functions
:
These will only be defined chartwise in general. Suppose that everywhere on the constrained set, the "n" derivatives of the "n" functions are all
linearly independent and also that thePoisson bracket s:{ "f""i", "f""j" }
and
:{ "f""i", "H" }
all vanish on the constrained subspace. This means we can write
:
for some smooth functions
:"c""ij""k"
(there is a theorem showing this) and
:
for some smooth functions
:"v""i""j".
This can be done globally, using a
partition of unity . Then, we say we have an irreducible first-class constraint ("irreducible" here is in a different sense from that used inrepresentation theory ).Geometric theory
For a more elegant way, suppose given a
vector bundle over M, with "n"-dimensionalfiber "V". Equip this vector bundle with a connection. Suppose too we have asmooth section "f" of this bundle.Then the
covariant derivative of "f" with respect to the connection is a smoothlinear map Δ"f" from thetangent bundle "TM" to "V" which preserves thebase point . Assume this linear map is rightinvertible (i.e. there exists a linear map "g" such that (Δ"f")"g" is theidentity map ) for all the fibers at the zeros of "f". Then, according to theimplicit function theorem , the subspace of zeros of "f" is asubmanifold .The ordinary
Poisson bracket is only defined over , the space of smooth functions over "M". However, using the connection, we can extend it to the space of smooth sections of "f" if we work with thealgebra bundle with thegraded algebra of "V"-tensors as fibers. Assume also that under this Poisson bracket,:{ "f", "f" } = 0
(note that it's not true that
:{ "g", "g" } = 0
in general for this "extended Poisson bracket" anymore) and
:{ "f", "H" } = 0
on the submanifold of zeros of "f" (If these brackets also happen to be zero everywhere, then we say the constraints close
off shell ). It turns out the right invertibility condition and the commutativity of flows conditions are "independent" of the choice of connection. So, we can drop the connection provided we are working solely with the restricted subspace.Intuitive meaning
What does it all mean intuitively? It means the Hamiltonian and constraint flows all commute with each other on the constrained subspace; or alternatively, that if we start on a point on the constrained subspace, then the Hamiltonian and constraint flows all bring the point to another point on the constrained subspace.
Since we wish to restrict ourselves to the constrained subspace only, this suggests that the Hamiltonian, or any other physical
observable , should only be defined on that subspace. Equivalently, we can look at theequivalence class of smooth functions over the symplectic manifold which agree on the constrained subspace (thequotient algebra by theideal generated by the "f"'s, in other words).The catch is, the Hamiltonian flows on the constrained subspace depend on the gradient of the Hamiltonian there, not its value. But there's an easy way out of this.
Look at the orbits of the constrained subspace under the action of the
symplectic flow s generated by the "f"'s. This gives a localfoliation of the subspace because it satisfiesintegrability condition s (Frobenius theorem). It turns out if we start with two different points on a same orbit on the constrained subspace and evolve both of them under two different Hamiltonians, respectively. which agree on the constrained subspace, then the time evolution of both points under their respective Hamiltonian flows will always lie in the same orbit at equal times. It also turns out if we have two smooth functions "A"1 and "B"1 which are constant over orbits at least on the constrained subspace (i.e. physical observables) (i.e. {A1,f}={B1,f}=0 over the constrained subspace)and another two A2 and B2 which are also constant over orbits such that A1 and B1 agrees with A2 and B2 respectively over the restrainted subspace, then their Poisson brackets {A1, B1} and {A2, B2} are also constant over orbits and agree over the constrainted subspace.In general, we can't rule out "
ergodic " flows (which basically means that an orbit is dense in some open set), or "subergodic" flows (which an orbit dense in some submanifold of dimension greater than the orbit's dimension). We can't haveself-intersecting orbits.For most "practical" applications of first class constraints, we do not see such complications: the
quotient space of the restricted subspace by the f-flows (in other words, the orbit space) is well behaved enough to act as adifferentiable manifold , which can be turned into asymplectic manifold by projecting thesymplectic form of M onto it (this can be shown to bewell defined ). In light of the observation about physical observables mentioned earlier, we can work with this more "physical" smaller symplectic manifold, but with 2n fewer dimensions.In general, the quotient space is a bit "nasty" to work with when doing concrete calculations (not to mention nonlocal when working with
diffeomorphism constraint s), so what is usually done instead is something similar. Note that the restricted submanifold is abundle (but not afiber bundle in general) over the quotient manifold. So, instead of working with the quotient manifold, we can work with asection of the bundle instead. This is calledgauge fixing .The "major" problem is this bundle might not have a
global section in general. This is where the "problem" of global anomalies comes in, for example. SeeGribov ambiguity . This is a flaw in quantizing gauge theories which many physicists had overlooked.What have been described are irreducible first class constraints. Another complication is that Δf might not be
right invertible on subspaces of the restricted submanifold ofcodimension 1 or greater (which violates the stronger assumption stated earlier in this article). This happens, for example in thecotetrad formulation ofgeneral relativity , at the subspace of configurations where thecotetrad field and theconnection form happen to be zero over some open subset of space. Here, the constraints are the diffeomorphism constraints.One way to get around this is this: For reducible constraints, we relax the condition on the right invertibility of Δ"f" into this one: Any smooth function which vanishes at the zeros of "f" is the fiberwise contraction of "f" with (a non-unique) smooth section of a -vector bundle where is the
dual vector space to the constraint vector space "V". This is called the "regularity condition".Constrained Hamiltonian dynamics from a Lagrangian gauge theory
First of all, we will assume the action is the integral of a local
Lagrangian which only depends up to the first derivative of the fields. The analysis of more general cases, while possible is more complicated. When going over to the Hamiltonian formalism, we find there are constraints. Recall that in the action formalism, there areon shell andoff shell configurations. The constraints which hold off shell are called primary constraints while those which only hold on shell are called secondary constraints.Examples
Look at the dynamics of a single point particle of mass "m" with no internal degrees of freedom moving in a
pseudo-Riemannian spacetime manifold "S" with metric g. Assume also that the parameter τ describing the trajectory of the particle is arbitrary (i.e. we insist uponreparametrization invariance ). Then, itssymplectic space is thecotangent bundle T*S with the canonical symplectic form ω. If we coordinatize "T" * "S" by its position "x" in the base manifold "S" and its position within the cotangent space p, then we have a constraint:"f" = "m"2 −g("x")−1(p,p) = 0.
The Hamiltonian "H" is, surprisingly enough, "H" = 0. In light of the observation that the Hamiltonian is only defined up to the equivalence class of smooth functions agreeing on the constrained subspace, we can use a new Hamiltonian H'=f instead. Then, we have the interesting case where the Hamiltonian is the same as a constraint! See
Hamiltonian constraint for more details.Consider now the case of a
Yang-Mills theory for a realsimple Lie algebra "L" (with anegative definite Killing form η)minimally coupled to a real scalar field σ which transforms as anorthogonal representation ρ with the underlying vector space "V" under "L" in ("d" − 1) + 1Minkowski spacetime . For l in "L", we write:ρ(l) [σ]
as
:l [σ]
for simplicity. Let A be the "L"-valued
connection form of the theory. Note that the A here differs from the A used by physicists by a factor of "i" and also a "g". This agrees with the mathematician's convention. The action "S" is given by:
where g is the Minkowski metric, F is the
curvature form : (no "i"s or "g"s!) where the second term is a formal shorthand for pretending the Lie bracket is a commutator, "D" is the covariant derivative
:Dσ = dσ − A [σ]
and α is the orthogonal form for ρ.
"I hope I have all the signs and factors right. I can't guarantee it."
What is the Hamiltonian version of this model? Well, first, we have to split A noncovariantly into a time component φ and a spatial part . Then, the resulting symplectic space has the conjugate variables σ, πσ (taking values in the underlying vector space of , the dual rep of ρ), , , φ and πφ. for each spatial point, we have the constraints, πφ=0 and the
Gaussian constraint :
where since ρ is an
intertwiner :,
ρ' is the dualized intertwiner
:
(L is self-dual via η). The Hamiltonian,
:
Note that the last two terms are a linear combination of the Gaussian constraints and we have a whole family of (gauge equivalent)Hamiltonians parametrized by "f". In fact, since the last three terms vanish for the constrained states, we can drop them.
See also
Dirac bracket ,second class constraints ,BRST ,analysis of flows
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