From Classical Mechanics to Quantum Field Theory

(Romina) #1
A Short Course on Quantum Mechanics and Methods of Quantization 23

Denoting withXψthe constant vector fieldXψ≡(x, ψ), we can regardgof
Eq. (1.74) andωof Eq. (1.75) as (0,2) tensors by setting:


g(x)(Xψ,Xφ)≡g(ψ,φ), (1.87)
ω(x)(Xψ,Xφ)≡ω(ψ,φ). (1.88)

Also we can promoteJas defined in Eq. (1.76) to a (1,1) tensor field by setting:


J(x)(Xψ)=(x, Jψ), (1.89)

making, as we have already noticed before, the tensorial triple (g,J,ω) admissible
andHRa linear K ̈ahler manifold[ 36 ].
The (0,2)-tensorsgandωbeing non-degenerate, we can consider the invertible
maps ˆg,ˆω:THR→T∗HRsuch that, for anyX,Y ∈THR:g(X,Y)=ˆg(X)(Y)
andω(X,Y)=ˆω(X)(Y). Then we can define two (2,0) contravariant tensors
given respectively by a metric tensorGand a Poisson tensor Λ such that


G(ˆg(X),ˆg(Y)) =g(X,Y), Λ(ˆω(X),ωˆ(Y)) =ω(X,Y). (1.90)

We can now useGand Λ to define a Hermitean product between any twoα, β∈H∗R
(equipped with the dual complex structureJ∗):


〈α, β〉H∗R≡G(α, β)+iΛ(α, β). (1.91)

To make these structures more explicit, let us introduce an orthonormal basis
{ek}k=1,···,ninHand global coordinates (qk,pk)fork=1,···,ninHRsuch that
〈ek,x〉=(qk+ipk)(x),∀x∈H. Then, it is easy to see that:


g=dqk⊗dqk+dpk⊗dpk, (1.92)
ω=dqk⊗dpk−dpk⊗dqk, (1.93)

J=dpk⊗ ∂
∂qk

−dqk⊗ ∂
∂pk

, (1.94)

so that


G=


∂qk⊗


∂qk+


∂pk⊗


∂pk, (1.95)

Λ=


∂qk



∂pk



∂pk



∂qk

. (1.96)

As a convenient shorthand notation, we can introduce complex coordinates:zk≡
qk+ipk, ̄zk≡qk−ipk, so that we can write


G+i·Λ=4∂
∂zk

⊗ ∂

∂ ̄zk

, (1.97)
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