Past exam of the mathematics course of the University of Cambridge 2005 iii Paper 54 3 Solution Created 2026-10-03 Updated 2026-10-14
The Polyakov action has independent worldsheet metric and embedding fields . Varying the metric before imposing a gauge givesWorldsheet diffeomorphisms and Weyl transformations allow conformal gauge locally. The Weyl factor then cancels out of the classical action, leavingThese are free two-dimensional scalar fields, but the surviving metric equations requireEquivalently, and . Gauge fixing does not license dropping these Virasoro constraints.
For an ordinary open string, the boundary conditions relate the two chiral sectors. With , their independent Fourier generators areThe classical oscillator Poisson brackets give the classical Virasoro constraint algebraThus they are first-class constraints. In the quantum theory one applies normal ordering to the product and uses . The oscillator commutator givesFor example, for the extra vacuum term is . This exhibits the Virasoro central extension rather than concealing it in a classical constraint equation. The matter central charge is ; the worldsheet ghost fields have charge . Quantum consistency sets and the string intercept to one.
In old covariant string quantization the physical-state Virasoro conditions for an open string arePhysical string states are then identified modulo physical null string states. One does not impose both positive and negative generators as annihilation conditions: their central extension would obstruct that prescription. The resulting null-state quotient of a string agrees with the transverse light-cone spectrum at nonzero momentum.
At , the oscillator vacuum is a single spacetime scalar field with : the bosonic tachyon. At , write . The zero-mode equation gives , and gives . The null descendant identifies . This leaves 24 physical polarizations of a massless gauge vector.
At , use the level-two open-string polarization decompositionThe mass is . The oscillator commutators give all the nontrivial positive-mode conditions:Higher positive modes annihilate this level. To see the quotient explicitly, the 25 transverse-parameter null states , with , shiftThe additional level-two scalar Virasoro null state shiftsSubstitution into the two physical equations verifies the null-state conditions; the second residual is . Because is timelike, these null shifts span all components of , so choose a representative with . The physical conditions then say and . In the rest frame this is a traceless second-rank tensor in 25 spatial dimensions, with polarizations. The light-cone basis independently gives states and symmetric states . Hence
For the fermionic extension, an explicit convention prevents ambiguity in the signs. Keep worldsheet signature and useTake and the constant parameter to be real Grassmann-odd Majorana components, with . Put . Apart from the common factor , the combined Lagrangian isThe rigid transformations can be writtenor, in components,For the part, the bosonic variation is , while the fermionic variation is . Anticommuting the constant parameter past the fermion is essential in the second term. The first terms cancel. The other chiral component works in the same way, giving the chiral proof of rigid worldsheet supersymmetryThus the action is invariant off shell up to a boundary term. The transformation is a genuine supersymmetry: on its commutator for parameters is the translationOn the same translation follows using and ; the remaining cross terms are proportional to these Dirac equations. This is on-shell closure of rigid worldsheet supersymmetry. On a surface with boundary, compatible endpoint conditions must make the boundary flux vanish. On a compact worldsheet, a constant parameter must preserve the spin structure; the local identity alone does not make a constant transformation compatible with every antiperiodic sector.
The fermions contribute to the worldsheet stress-energy tensor and produce a fermionic superconformal current. In holomorphic normalization with ,The free-field contractions give and conformal weight for , where . Consequently the modes obey the N=1 super-Virasoro algebraDropping the central terms gives the classical graded constraint algebra. Integer gives the Ramond sector; half-integer gives the Neveu–Schwarz sector. In the displayed conformal-plane convention in the Ramond sector. Shifting to the Ramond vacuum-normal-ordered zero mode gives the usual Ramond supercurrent zero-mode square .
Rigid symmetry of matter already supplies these currents, but promoting their vanishing to new gauge constraints requires coupling to worldsheet supergravity and varying its worldsheet gravitino. In superconformal gauge one retains . The fermionic current constraints and their physical-state conditions extend the bosonic Virasoro conditions. The ghost charges are , so cancellation with gives the critical dimension of the RNS superstring ; the NS and Ramond intercepts are respectively and zero. This distinguishes the global supersymmetry established above from its locally gauged string completion.
Past exam of the mathematics course of the University of Cambridge 2007 iii Paper 54 4 Solution Created 2026-10-03 Updated 2026-10-14
Take on the strip . Varying the Grassmann-odd worldsheet Majorana fermions gives , and, up to the orientation of the strip boundary, the surface termAt each endpoint it vanishes if with , with the same relation on variations. A common sign can be absorbed by redefining one chiral field, so set . Since and , the second endpoint imposes . Equal endpoint signs give the periodic Ramond sector, and opposite endpoint signs give the antiperiodic Neveu–Schwarz sector:These gluing choices preserve the Neumann-endpoint worldsheet supersymmetry conditions and give integer or half-integer worldsheet Majorana fermion modes, respectively.
First fix a normalization issue in the original PDF. With its stated canonical string oscillator algebra, the standard superconformal current mode iswithout the printed factor . To check the Ramond supercurrent zero-mode square directly, pair positive and negative integer modes:The zero-mode Clifford relations give . Different anticommute, and so do with the zero-mode term. The two same-sign terms in vanish by antisymmetry of the fermions and symmetry of the bosonic product. The cross terms giveThe second term comes from commuting through , so the frequency factor is essential. ThereforeHere uses vacuum-annihilating Ramond normal ordering; its string intercept is zero. A plane-to-cylinder central shift must be included consistently if a different zero-mode convention is used.
For the mode actually printed, the algebra instead gives . Already the oscillator-free term gives , whereas . Thus the requested identity is not valid with both that prefactor and the supplied string oscillator algebra. Removing the prefactor gives the identity just derived. Renaming as would fix this isolated equality but would spoil the usual Virasoro normalization and the subsequent mass formula. We use the standard normalized modes in the remaining physical constraints; their vanishing is unaffected by a common nonzero rescaling.
The RNS string physical-state conditions in the two sectors areThe last condition is the fermionic zero-mode constraint; its square implies the Ramond mass-shell condition. Physical null string states are quotiented. Matter central charge is , while the reparameterization worldsheet ghost fields and superconformal ghosts contribute . Thus is the critical dimension of the RNS superstring, with and .
To solve the constraints, choose , so , and work on a patch with . In light-cone gauge in string theory fix all nonzero and all to zero. For the Ramond sector, the printed restriction to nonzero fermion modes is not by itself complete: one must also reduce the longitudinal fermionic zero modes using the zero-mode supersymmetry constraint. The usual reduced light-cone description sets the remaining to zero as well and retains the transverse Clifford algebra. Covariantly this reduction is the Dirac equation on the ground-state particle polarization; it is not an extra unconstrained canonical string oscillator.
With this reduction the string oscillator generators have the formRepeated runs over the eight transverse directions. The coefficient in comes from the fermion worldsheet stress tensor ; for , positive and negative combine to give the occupation energy . Thus the light-cone super-Virasoro constraints are explicitly solved byHere is in the NS sector and zero in the R sector. The zero-mode equation says . All longitudinal excitations are consequently determined by transverse bilinears. The critical dimension and string intercepts are necessary for the resulting quantum theory to preserve the target Lorentz algebra.
The frequency-weighted Neveu–Schwarz level operator isThe PDF's displayed number operator omits the fermion frequency weights and the term. With the stated anticommutators that cannot be a level operator: it would assign no level to the first fermionic excitation. The bosonic term already includes its frequency through , whereas the fermionic term must include its frequency explicitly.
One independent way to obtain the string intercept is the transverse zero-point energy. Each periodic boson contributes . Each antiperiodic real fermion contributes , with the minus sign due to fermionic normal ordering. For example a common exponential cutoff givesSubtracting the local divergent terms leaves , so the NS string intercept is . In the Ramond sector the integer fermions instead contribute per component and cancel the bosonic contribution, giving .
The unprojected NS sector oscillator vacuum has andIt is a spacetime scalar tachyon. The first excitation has and is massless, with eight vector particle polarizations. Covariantly its particle polarization obeys modulo the longitudinal null particle polarization, leaving the same eight degrees of freedom.
The R sector oscillator vacuum is also massless, but it is degenerate because . The operators give the target Clifford algebra, and becomes . At nonzero null momentum this Dirac equation leaves sixteen unprojected on-shell spinor states. Equivalently the eight transverse zero modes give the sixteen-dimensional spin representation of . Thus the Ramond ground state describes spacetime fermions, not a single scalar oscillator vacuum.
To define the GSO projection explicitly, let count excited NS fermions and give its vacuum even parity. ThenIt retains odd fermion number, removes the tachyon, and retains the eight massless vector particle polarizations. In the Ramond sector let be transverse chirality and count nonzero-mode fermions. Choose one consistent chirality sign and useEach operator squares to itself. At the ground level retains one eight-dimensional spinor chirality, so the retained spectrum has eight massless bosonic and eight massless fermionic states. The parity convention can instead assign the NS vacuum odd parity and write a plus projector; the retained states are identical.
Equality continues at every mass level. Let count , suppressing common momentum and endpoint-label factors, and set . The projected string oscillator generating functions areThe Ramond factor eight follows because either chirality projector selects eight ground states for every nonzero-oscillator parity. The Jacobi abstruse identity makes the bracket equal to , soThis proves level-by-level equality of bosonic and fermionic multiplicities. The appropriate spacetime supercharge from an RNS spin field relates the two sectors; the projection ensures that it acts within the retained state space. These sector and chirality conventions agree with the primary superstring lecture notes. Equal total counts alone are not the definition of the projection; they follow from the stated parity selection and the string oscillator identity.
Past exam of the mathematics course of the University of Cambridge 2012 iii Paper 51 3 Solution Created 2026-10-03 Updated 2026-10-07
A Majorana spinor equals its transform under charge conjugation, so its spinor components are not independent of their conjugates. In a real two-dimensional gamma matrix representation it can be taken real, with anticommuting Grassmann variables as components. Each target index labels a separate worldsheet Majorana fermion; it is not itself a target-space spinor.
Use worldsheet signature and the real gamma matricesTake with . Define the chirality matrix with the chosen worldsheet orientation byIt squares to one and anticommutes with each gamma matrix. Chirality is its eigenvalue, selected by the chiral projectors. Its overall sign is conventional.
Writing , the fermion equation of motion becomesHenceThe first profile travels toward increasing , and the second toward decreasing . Thus the choice of chirality orientation realizes the requested worldsheet chirality and propagation direction correspondence; reversing the orientation interchanges the labels.
For the rigid worldsheet supersymmetry variation, let be a constant Grassmann-odd Majorana spinor. With the displayed conventions,The minus sign follows from . A second identity from the Majorana Grassmann bilinear interchange is . Keeping these Grassmann signs is essential.
The bosonic kinetic variation is . The two fermionic kinetic variations, using the two identities above, give the full resultFor the second equality use and symmetry of the second embedding derivative. No field equation has been used. Thus the variation is an off-shell total derivative:This is the rigid worldsheet supersymmetry boundary term. It vanishes when the boundary flux vanishes, for example on a closed worldsheet with compatible fields and variations. On a spatial circle, a constant supersymmetry parameter must also respect the chosen spin structure. Periodic fermions allow this rigid transformation; antiperiodic fermions and a constant parameter would give an antiperiodic and fail to preserve a periodic bosonic embedding. The local action identity remains valid, but global symmetry requires compatible boundary data. This is the spin-structure obstruction to constant worldsheet supersymmetry.
For the spectrum, assume the usual critical RNS string, physical-state constraints, a nonzero null target momentum, and the supersymmetric GSO projection. Analyze just one chiral sector. Its matter central charge is ; the bc system and superconformal ghosts contribute . Therefore gives the critical dimension of the RNS superstring . Light-cone gauge in string theory leaves eight transverse bosonic and eight transverse fermionic string oscillator directions.
In the Neveu–Schwarz sector, the normal-ordering intercept is . The massless level is and has statesThe GSO projection retains these eight transverse vector polarizations while removing the tachyonic ground state. They are spacetime bosons, although the creating string oscillator is a worldsheet fermion. In covariant language transversality and the longitudinal null-state quotient leave polarizations.
In the Ramond sector, bosonic and fermionic zero-point energies cancel, so and the ground states are massless. The eight transverse fermion zero modes obeyThis Ramond zero-mode Clifford algebra acts on a sixteen-dimensional ground-state space. Its two chirality subspaces each have dimension eight. The GSO projection keeps one, an or spinor of , the rotation subgroup of the massless little group. These are spacetime fermions. Equivalently a ten-dimensional Majorana-Weyl spinor has sixteen real components before the massless Dirac equation reduces the physical polarization count to eight.
Consequently the massless chiral RNS spectrum after GSO projection satisfiesThe GSO projection is essential: without it, the transverse Ramond sector would retain both eight-dimensional spinor chiralities. These are counts for one chiral sector, not the tensor-product counts of the full closed-string spectrum.
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.