Past exam of the mathematics course of the University of Cambridge 2014 iii Paper 48 1 Solution Created 2026-10-03 Updated 2026-10-06
The fields constitute an RNS string coupled to two-dimensional worldsheet supersymmetry. The zweibein and worldsheet gravitino impose constraints; they do not supply extra propagating string polarizations. Worldsheet diffeomorphisms, local frame rotations and Weyl transformations put the metric locally in conformal gauge, . Local supersymmetry together with super-Weyl symmetry removes the worldsheet gravitino, giving superconformal gauge . On a general closed worldsheet, moduli and spin structures remain and must still be summed or integrated over; gauge fixing is not a declaration that every surface is globally a flat cylinder.
Variation with respect to the metric and worldsheet gravitino before gauge fixing gives the stress-tensor and supercurrent constraints and . The remaining matter consists of free and their worldsheet fermions. In covariant quantization, these become the N=1 super-Virasoro algebra physical-state conditions: positive Virasoro and supercurrent modes annihilate a physical state, , and the R sector also has the zero-mode condition . Null gauge states are quotiented out. Equivalently, physical states are BRST cohomology classes, so BRST-exact operators do not represent additional physical states.
The diffeomorphism ghosts have central charge , while the bosonic superconformal ghosts have charge . Matter contributes . Therefore quantum gauge consistency requiresThis is the critical dimension of the RNS superstring. In light-cone gauge in string theory, choose nonzero , make linear in worldsheet time and set . The stress-tensor and supercurrent constraints solve for the longitudinal and oscillators. Only eight transverse bosons and eight transverse fermions remain, with positive norm. This explicitly eliminates the time-like and longitudinal unphysical states.
In a chiral sector the fermions have half-integral modes in the NS sector and integral modes in the R sector. The normal-ordering constant of a string is and . The GSO projection retains odd fermion-excitation parity in the NS sector, removing its tachyonic vacuum. In the R sector it keeps one chirality of the zero-mode spinor, with oscillator parity included in the projection. The Ramond zero-mode Clifford algebra then leaves eight ground-state polarizations in light-cone gauge in string theory.
Worldsheet supersymmetry alone does not imply spacetime supersymmetry. The GSO projection makes the spinorial worldsheet currents mutually local with the retained vertex operators and pairs their NS and R states. More explicitly, let be an RNS spin field and the bosonized superghost scalar. The spacetime supercharges are generated byand similarly in the other chiral sector. The spin field has conformal weight , and its superghost factor has weight , so the current has weight one. Its operator products generate the spacetime translation operator; schematically . This is the spacetime supercharge from an RNS spin field. For type IIA superstring theory, the left and right Ramond projections select opposite ten-dimensional Majorana-Weyl chiralities, giving 32 real supercharges and a nonchiral spacetime theory.
The massless physical states are best counted with the transverse little group . Choose the left Ramond ground representation and the right one . ThenThe NS-NS sector supplies the graviton, Kalb–Ramond field and dilaton, with , and polarizations. The RR sector supplies a one-form potential and a three-form potential, with and polarizations. The mixed sectors supply two gravitinos of opposite chirality, each with polarizations, and two dilatinos, each with . Covariantly the dilatino has chirality opposite to its corresponding supersymmetry parameter; the two chirality sets are both present. Thus the massless type IIA spectrum hasThese fields form the massless type IIA supergravity multiplet.
For the first massive level of a chiral RNS sector, restore throughThe first positive value is one. The NS states therefore have level . A complete transverse basis after GSO projection isAll contain odd fermion-excitation parity. Their respective dimensions are , and , so the NS count is . These are the first massive GSO-projected Neveu–Schwarz states. The middle family decomposes into . Together the families assemble into the massive representations : a symmetric traceless rank-two tensor and a three-form, since and .
In the R sector, the first massive level is . If the retained right-moving ground spinor is , its two families areThe Ramond spinors have opposite zero-mode chiralities in these two families: inserting one fermionic oscillator reverses the oscillator contribution to the GSO condition, so the second family must use the opposite zero-mode chirality. Each family has states. HenceThese first massive GSO-projected Ramond states form the gamma-traceless vector-spinor representation of , of dimension . Its transverse branching is . The right-moving sector therefore contains bosons and fermions, a massive chiral superstring supersymmetry multiplet.
For the closed string, closed-string level matching requires the left and right shifted levels to agree. Both chiral sectors at this first massive mass have NS states and R states. The bosons lie in the NS-NS sector and RR sector, while the mixed sectors are fermionic. ConsequentlyTheir total is . A massive ten-dimensional state with 32 real supercharges and no central charges has sixteen fermionic creation operators in its rest-frame supersymmetry algebra, giving a long multiplet of this size. Thus the chiral equality, the four closed sectors and level matching are consistent with the first massive type IIA long supermultiplet, rather than merely matching an isolated number of right-moving states.
Past exam of the mathematics course of the University of Cambridge 2017 iii Paper 306 4 Solution Created 2026-10-03 Updated 2026-10-05
A Majorana spinor equals its charge conjugation, , with conventional phase choices absorbed into . The two-component worldsheet Majorana fermion therefore has no independent complex conjugate components; in a Majorana representation its components can be real Grassmann variables. The same condition applies to the constant supersymmetry parameter. Grassmann statistics matter in the variation: replacing the spinors by commuting numerical vectors would give the wrong bilinear interchange signs.
The displayed rigid transformation is understood in flat conformal gauge. Take , , and chooseHere is a valid invariant charge-conjugation form: and . These concrete matrices make all signs checkable; equivalent Majorana conventions give the same result with their consistently transformed bars.
Let and , so . Suppressing the common factor in the action, the flat kinetic density isThe rigid variations have and . The supersymmetry variation is even, so its product rule has no extra graded sign. From the Majorana Grassmann bilinear interchange identities,For example the last identity follows by moving the Grassmann-odd parameter through , then using and the transpose relations twice. No equation of motion has been used.
The two kinetic variations areThe Clifford algebra turns the first fermionic term plus the bosonic variation into . In the second term, commute the partial derivatives and use the same algebra: the antisymmetric gamma product drops out, leaving . Together they are precisely the rigid worldsheet supersymmetry boundary term:Therefore . It vanishes on a closed or periodic worldsheet, for compactly supported changes, or under compatible supersymmetric endpoint conditions. The local total-derivative identity is off shell; the boundary assumptions are needed to call the integrated action invariant.
The flat-gauge qualification is substantive. On an arbitrary curved worldsheet, spinors need a zweibein and spin connection and a constant spinor parameter need not exist. A fully covariant locally supersymmetric action also involves the worldsheet gravitino; the isolated ordinary-derivative expression does not prove rigid invariance for arbitrary . We have proved the intended rigid symmetry of its flat gauge-fixed action, with the fermionic term inside the same integral and overall normalization. If the displayed last term were read as outside the integral, it would not even define an action.
For phenomenology, bosonic string theory has no spacetime fermions and its usual vacuum contains a tachyon. The spinning string has a Ramond sector, whose fermionic zero modes form a spacetime Clifford algebra and give spacetime spinor states, as well as a Neveu–Schwarz sector. In suitable consistent theories the GSO projection removes the tachyonic NS ground state and keeps the appropriate Ramond chirality. The critical dimension of the RNS superstring is 10 rather than 26: bosons and real fermions have matter central charge per chiral sector, while the reparameterization and superconformal ghosts contribute , so the total anomaly cancels at .
Suitable GSO-projected superstrings admit spacetime fermions and a tachyon-free spectrum, making them more promising for particle physics than the bosonic string. Rigid worldsheet supersymmetry alone does not establish a tachyon-free spacetime theory or realistic phenomenology. The projection, consistent sectors and compactification in string theory are additional input; spacetime supersymmetry and a realistic four-dimensional spectrum are not automatic consequences of this classical action.
Spin connection Created 2026-10-05 Updated 2026-10-07
In an orthonormal frame, the spin connection is the Lorentz connection acting on spinors. With , its covariant derivative is . The metric connection determines when torsion conditions are specified. A zweibein gives its two-dimensional form; omitting it on a curved worldsheet generally destroys covariance.