Canonical quantization 2026-10-05
Canonical quantization promotes canonical variables to operators and their Poisson brackets to canonical commutation relations. Composite observables require an ordering prescription, and quantum anomalies can modify their algebra.
Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 306 1 i Solution Created 2026-10-03 Updated 2026-10-05
Use the Minkowski metric and units with speed of light one. The contractions are and ; and pair a vector with a covector without another metric. The Lagrange multipliers impose the two first-class constraintsThey generate worldsheet diffeomorphisms, so the phase space contains both constrained directions and gauge redundancy. Two first-class constraints remove two canonical pairs, leaving physical degrees of freedom per point.
In Monge gauge, and . Write the transverse canonical variables as and . Solving the first-class constraints givesThe negative root selects positive energy. Substitution into the phase-space action gives the Hamiltonian reductionFor a static segment, , its proper length element is , and . Thus the string tension is the rest energy per unit proper length. In particular a straight resting segment has . Monge gauge is a local choice on a string embedding map for which is a valid coordinate; it need not cover folded strings or all endpoint configurations.
Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 306 2 iii Solution Created 2026-10-03 Updated 2026-10-05
For covariant quantization of the bosonic string,All other commutators between independent canonical variables vanish. The covariant Fock vacuum obeys for every and every . Normal ordering moves these annihilating string oscillators to the right and givesThen . Its commutator grades a Fock state basis by , although its inner product is indefinite because of the timelike oscillator.
The quantum Virasoro algebra has central charge :The Virasoro central extension comes from commutators needed to order infinite oscillator sums; it is a quantum effect absent from the classical Poisson brackets. Replacing a classical Poisson bracket by a commutator cannot recover that term without a regularized ordering calculation.
If a state were annihilated by every nonzero , the commutator would imply . The commutator would then imply . For , only the zero vector is annihilated by all nonzero Virasoro constraints. This explains why only positive modes annihilate a physical string state.
The vacuum is a physical string state when . At level one all states have the form . Since , the positive-mode Virasoro constraints giveThus the complete level-one conditions and norm arewith the common vacuum normalization suppressed.
For , choose spacelike momentum , . A purely timelike polarization has and norm . Hence a negative-norm physical string state exists when .
For , the mass-shell condition gives . In a rest frame, forces , leaving positive-norm vector-particle polarizations, those of a massive vector.
For and nonzero null momentum, leaves a null direction . The corresponding null string state is . It is orthogonal to every physical string state because annihilates them. Quotienting by this gauge redundancy, , leaves positive vector-particle polarizations. Thus the level-one spectrum agrees with light-cone gauge in string theory at . This level-one argument alone does not establish consistency or absence of negative norms at all higher levels.
Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 306 2 i Solution Created 2026-10-03 Updated 2026-10-05
The real canonical variables describe the center-of-mass position and total momentum of the open string. The nonzero string oscillators are complex Fourier modes with ; the Lagrange multipliers obey . The Virasoro constraints satisfy , so the multiplier term is real.
For each , the oscillator kinetic term differs from the manifestly real expressionby . Thus the written action is real up to a boundary term, which does not change its symplectic form or bulk dynamics. Adding the corresponding endpoint term makes reality exact.
The independent nonzero Poisson brackets areAll brackets between these independent center-of-mass and oscillator variables vanish. The dependent zero mode is , so, if it is used, .
The Fourier coefficients of the Virasoro constraints areTheir Poisson brackets areThey form the classical Witt algebra, with no Virasoro central extension. In particular they are first-class constraints, closing on the constraint surface, and generate the remaining worldsheet diffeomorphisms rather than independent physical excitations.
Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 306 3 b Solution Created 2026-10-03 Updated 2026-10-05
The Jacobi identity for the Poisson bracket impliesFor first-class constraints with linearly independent differentials this gives , the Jacobi identity for the structure constants of the constraint algebra. Independence is an implicit assumption: for constraints obeying identities or vanishing identically, only the contracted identity follows, and arbitrary coefficients multiplying such constraints need not satisfy a Lie algebra identity.
With and , the canonical variables transform asTo fix the sign convention, vary the phase-space action directly:Thus action invariance requires . For , the Faddeev-Popov determinant is that ofUsing anticommuting Faddeev-Popov ghost fields, the invariant-convention result isThe original PDF has a sign error in the stated multiplier transformation; the TeX transcription has the consistent plus sign. Keeping the PDF's displayed minus sign mechanically would instead give . That expression exponentiates the determinant of the printed transformation, but that transformation does not preserve the stated action with the canonical convention above. It cannot be used as the invariant result without changing another convention consistently.
As for the particle, constant multiplier moduli and any residual zero mode in field theory must be handled separately; the constant gauge fixing is understood locally on the gauge orbit.
Phase-space action 2026-10-05
A phase-space action treats canonical variables as independent fields. Varying them gives Hamilton's equations; Lagrange multipliers can impose constraints.