Past exam of the mathematics course of the University of Cambridge 2014 iii Paper 46 1 Solution Created 2026-10-03 Updated 2026-10-06
Use the mostly-plus Minkowski metric, and write for equality on the constraint surface. Assume that the mechanical constraints are locally independent. They are first-class constraints whenThus their Poisson brackets vanish on the constraint surface, and their Hamiltonian flows preserve that surface. The structure functions of a constraint algebra may depend on the phase space point. The finite real span of the constraints is a Lie algebra if it closes with constant structure coefficients, in a suitable choice of generators. The Jacobi identity then gives the usual conditions on the structure constants of a Lie algebra. With general structure functions the finite real span need not close, even though the Poisson bracket of all smooth functions is itself a Lie bracket.
To see the gauge invariance directly, let generate a canonical gauge transformation:The variation of the phase-space action integrand isThe second term cancels without using the equations of motion. Taking to vanish at the temporal boundaries leaves the action invariant. Arbitrary functions therefore relate different descriptions of the same physical motion. This reasoning also works with structure functions; constant structure coefficients are only needed for the finite-dimensional Lie algebra claim.
For a closed string, choose and periodic fields. A convenient Nambu-Goto phase-space action isHere and are Lagrange multipliers. The Nambu–Goto phase-space constraints are and , with canonical Poisson bracketsLet . Differentiating the periodic Dirac delta function givesThe opposite signs in and cancel these terms, so . Replace the original constraints by the equivalent chiral densitiesTheir mixed Poisson brackets vanish. Choose opposite Fourier orientations for the two sectors:The chiral constraint algebra of a closed string isEach is the Witt algebra: the vector fields on a circle satisfy . Fourier expansion identifies each real algebra, with , with the Lie algebra of vector fields on the circle. The two commuting copies give , not a quantum central extension.
For an open string, allowed boundary conditions must remove the endpoint term in the variation of the action, consistently with the allowed endpoint variations. The spatial boundary term isIt expresses the open-string endpoint momentum flux. In the temporal gauge for a string , take a boundary-adapted parametrization with at the ends. Fixing gives , a Dirichlet boundary condition. At the other end allow arbitrary spatial variations; for nonzero these require , a Neumann boundary condition. Also in this temporal gauge for a string, so . The constraint at this free-end string boundary condition reduces to . Hamilton's equation consequently gives there. Since , the free endpoint has spatial speed one. This is the null motion of a free string endpoint.
A straight rotating string with one fixed endpoint supplies the required solution in at least two spatial dimensions. Set , , andTake . The Hamilton's equations become , which holds because both second derivatives give . The Nambu–Goto phase-space constraints are satisfied byThe endpoint at stays at the origin, while at and the endpoint moves around a circle of radius with angular speed . At each time the whole string lies on a straight radial segment. Its spatial proper length isThe velocity is everywhere perpendicular to the segment, so this also equals the sum of local rest-frame lengths. The induced worldsheet metric becomes degenerate at the null free endpoint, as expected for the limiting free-end solution.
Past exam of the mathematics course of the University of Cambridge 2016 iii Paper 306 1 i Solution Created 2026-10-03 Updated 2026-10-06
Work away from , where the inverse-square potential is singular. Variation of the phase-space action givesThe last equation is the constraint imposed by the Lagrange multiplier . The canonical momentum conjugate to is , not . Consequently the nonzero canonical Poisson brackets areIn particular,With the convention , the Noether charge generating is . Equivalently, the conserved physical energy is ; a convention that calls the energy the time-translation charge absorbs this minus sign into its parameter.
For the dilation charge,on the constraint surface. Its infinitesimal canonical transformations areFor constant , extending this by preserves the action: the kinetic terms are invariant and scales oppositely to . Thus the dilation acts on time and position with their nonrelativistic relative scaling. Its Poisson bracket with the energy is
Put . Direct variation of the Hamiltonian givessoThe supplied transformations are generated by the special conformal charge of inverse-square mechanicsChooseThen even for a time-dependent parameter. Expanding the kinetic-term variation, keeping the terms in , givesHenceFor a constant parameter only the boundary term remains, identifying as the Noether charge. Independently, the equations of motion giveUsing the same canonical Poisson bracket convention,Together, , and form the sl2R Lie algebra of conformal mechanics. These are time translation, dilation and special conformal transformation. A useful normalization check is the Casimir elementon the constraint surface.
For the extended canonical variables with and , the charge generates a special conformal transformation. Its time derivative is , so it is conserved on the constraint surface. With a time-dependent parameter , the multiplier varies as and the action variation is .