Critical dimension of the RNS superstring Created 2026-10-05 Updated 2026-10-07
Each of embedding bosons contributes one to the chiral central charge, and each real worldsheet Majorana fermion contributes one half. The reparameterization bc system contributes , and the superconformal ghosts contribute . Vanishing total worldsheet Weyl anomaly therefore requires , or . This differs from the critical dimension 26 of the bosonic string, which has no worldsheet fermions or superconformal ghosts.
Neveu–Schwarz fermionic oscillator 2026-10-06
Antiperiodic worldsheet Majorana fermions give transverse modes , , with . Positive modes annihilate the oscillator vacuum; negative modes are fermionic creation operators.
Neveu–Schwarz sector Created 2026-10-05 Updated 2026-10-06
Antiperiodic worldsheet Majorana fermions have half-integer modes in this sector.
Past exam of the mathematics course of the University of Cambridge 2001 iii Paper 64 5 Solution Created 2026-10-03 Updated 2026-10-14
Introduce anticommuting matter fields as worldsheet Majorana fermions, transforming as target-spacetime vectors and two-dimensional spinors. The RNS string pairs them with through worldsheet supersymmetry. In flat superconformal gauge the matter action is, up to the conventional fermion normalization,and the field equations split into left- and right-moving components. The supersymmetry constraints include both the stress tensor and the supercurrent, so unphysical polarizations are removed rather than interpreting every fermionic worldsheet component as a physical particle.
The possible spin structures produce two sectors. On the closed chiral circle, or the doubled open string, the Neveu–Schwarz sector has and half-integer modes . The Ramond sector has periodic and integer modes , including . Canonical quantization replaces the classical Grassmann variables by operators satisfyingIn particular obeys . This is the Ramond zero-mode Clifford algebra in covariant form. Its ground-state space must carry a representation of the Clifford algebra of the target metric, and hence transforms as a spinor, not a scalar vacuum. Indeed the zero-mode Lorentz generators proportional to act on it as the spin representation. This is the essential mechanism converting anticommuting worldsheet matter into spacetime spinorial states.
The zero-mode supercurrent constraint on a Ramond ground state is proportional to . It becomesthe momentum-space Dirac equation. The Ramond level operator has zero intercept, so the ground state is massless. Exciting bosonic or nonzero fermionic oscillators gives tensor-spinor excitations; the Clifford ground-state factor is retained. In the Neveu–Schwarz sector there is no fermionic zero-mode degeneracy. Its ground state is a scalar and its excited states carry integer-spin tensor representations, despite the anticommuting oscillator construction. Thus worldsheet fermionic oscillators do not by themselves make every target-space state a fermion.
Consistent projection also matters. The GSO projection removes the NS tachyon and selects a definite Ramond chirality in the standard supersymmetric spectrum. At the critical dimension ten, the projected massless NS vector has eight transverse polarizations, while the projected Ramond ground state has eight physical spinor polarizations after the massless Dirac constraint and the Majorana-Weyl spinor conditions. The projection permits their organization into spacetime supersymmetry multiplets. The assignment of spacetime fermionic statistics is compatible with spinorial transformation, vertex-operator locality and the Spin-statistics theorem; it is not just a relabeling of the Grassmann variables in the classical action.
For a closed string the left and right sectors can be chosen independently subject to level matching and the consistent spin-structure sum. The NS-NS sector and Ramond–Ramond sector have bosonic spacetime representations; a pair of Ramond spinors produces integer-spin fields. The mixed NS-R sector and R-NS sector instead carry one spinor factor and yield spacetime fermions, including gravitino and dilatino states. Opposite versus equal chiralities of the two Ramond sectors distinguish the type IIA superstring theory and type IIB superstring theory choices.
Quantum consistency of this RNS matter-plus-gauge system requires : its matter central charge is , the reparameterization ghosts contribute and the commuting superconformal ghosts contribute , so the total is . Spacetime fermions arise through Ramond matter zero modes, their Clifford/spinor representations and the physical-state/projection conditions. The anticommuting gauge-fixing ghosts already present in the bosonic path integral are not such matter fields and do not create physical spacetime fermions.
Past exam of the mathematics course of the University of Cambridge 2002 iii Paper 67 5 Solution Created 2026-10-03 Updated 2026-10-14
The RNS string adds worldsheet Majorana fermions to the coordinate fields . The new fields are spinors on the worldsheet but vectors under the target Lorentz group; this distinction matters when interpreting their oscillator states. In a flat target, a convenient Lorentzian convention for the free gauge-fixed action iswhere are two-dimensional gamma matrices. The bosonic and fermionic kinetic terms are related by worldsheet supersymmetry. Before fixing local worldsheet supersymmetry, one introduces a worldsheet gravitino along with the worldsheet metric. After superconformal gauge fixing, the residual matter constraints are the Virasoro constraints and the constraints generated by the superconformal current .
Each real worldsheet Majorana fermion contributes to the chiral central charge, while each coordinate contributes one. The reparameterization bc system contributes , and fixing local worldsheet supersymmetry also produces commuting superconformal ghosts of weights , with central charge . ThusIn light-cone gauge in string theory there are eight physical transverse coordinate fields and eight transverse worldsheet Majorana fermions.
On the doubled spatial interval of an open string, the two allowed fermionic periodicities areThey arise from the relative signs of the left-right fermion gluing conditions at the two ends. Thus the Ramond sector has integer-mode oscillators , including , and the Neveu–Schwarz sector has half-integer oscillators , , without zero modes. In either sector,A closed string has independent left- and right-moving periodicities, giving four sector choices rather than two.
The Ramond zero-mode Clifford algebra isHence its ground states carry a Spinor representation of the Lorentz group. The zero-mode supercurrent constraint reduces on a ground state to the Dirac equation . In the Neveu–Schwarz sector the oscillator vacuum instead carries a scalar representation. Consequently the open string NS sector describes spacetime bosons, while the R sector describes spacetime fermions. Exciting a target-vector oscillator does not change this statistics assignment.
The string intercepts follow from the transverse zero-point energy. Per boson the integer-mode contribution is . Per fermion it is the negative of the corresponding half-sum. Since , the eight transverse pairs giveThus , , and the open string mass formula is . This distinguishes the lowest states explicitly:
- In the NS sector, the level-zero scalar is a tachyon with . At level , is a massless vector. The supercurrent and Virasoro constraints give and the equivalence . There are eight physical vector polarizations.
- In the R sector, the level-zero states are massless spacetime spinors satisfying the Dirac equation. Before the GSO projection, the two chiralities together give 16 on-shell polarizations; they split into the two eight-dimensional transverse spinor representations.
The supersymmetric GSO projection keeps odd oscillator fermion number in the NS sector. Defining so that the NS vacuum has , its projector isIt removes the scalar tachyon and keeps the massless vector. In the R sector, fermion parity contains the zero-mode chirality operator, so one may writeHere counts nonzero-mode fermionic excitations. On the ground states, this keeps one Majorana-Weyl spinor chirality: 16 real covariant components, or eight on-shell polarizations after the Dirac equation. The projected massless open-string states are an eight-polarization gauge vector and an eight-polarization gaugino. The compatible projected tower exhibits spacetime supersymmetry; unprojected worldsheet supersymmetry by itself did not eliminate the tachyon or equalize these massless counts.
For a closed string, both chiral zero-mode constraints must hold:This shifted closed-string level matching is particularly important in the mixed sectors. The lowest states and their spacetime nature are as follows.
- The NS-NS sector is bosonic. Before projection, is a scalar tachyon with . The GSO projection on each side removes it. The surviving lowest level is , with transverse states . Decomposing their tensor product into symmetric traceless, antisymmetric and trace parts gives the graviton, Kalb–Ramond field and dilaton, with physical polarizations.
- The RR sector is bosonic, since it combines two spacetime spinors. Its lowest states have and are massless. The two Dirac equations on the bispinor polarizations identify them with on-shell differential-form field strengths. After projection they supply 64 bosonic polarizations. The actual form degrees depend on the two chosen Ramond sector chiralities.
- The NS-R sector and R-NS sector are fermionic. Their respective lowest level-matched pairs are and , not two oscillator vacua. A vector tensored with a chiral spinor decomposes into its gamma-traceless vector-spinor and gamma trace. These give a massless gravitino and dilatino, with polarizations in each mixed sector. The vacuum pair would fail the shifted closed-string level matching, so it cannot be counted as a mixed-sector tachyon.
For type IIA superstring theory, the two R sector ground-state chiralities are opposite. The Ramond–Ramond potentials can be represented by , with transverse counts . The two mixed-sector gravitinos have opposite chiralities, and the ten-dimensional theory is nonchiral. For type IIB superstring theory, the two R sector chiralities agree; the Ramond–Ramond potentials are , with self-dual five-form field strength, giving . Its two gravitinos have the same chirality. Thus both projected type II theories have 128 massless bosonic and 128 massless fermionic polarizations and no tachyon, while their chiralities and form spectra differ.
If unoriented open strings are included in the complete theory, the supersymmetric example is type I string theory. Worldsheet orientation reversal projects the closed type IIB superstring theory spectrum and identifies the two mixed sectors; the surviving closed fields include the graviton, dilaton, a Ramond–Ramond potential , and one gravitino and dilatino. The open states form vector and gaugino multiplets with Chan-Paton factors; tadpole and anomaly cancellation select . This is an additional orientation projection, not part of the GSO projection itself. The heterotic string instead pairs one supersymmetric chiral side with a bosonic chiral side carrying an internal gauge sector; it does not have a Ramond choice on both sides.
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 2015 iii Paper 49 2 Solution Created 2026-10-03 Updated 2026-10-06
Solving the massive subsidiary conditions. In light-cone coordinates, use and write . The divergence condition readsThus, when is invertible,First apply this with , then with , and finally with ; symmetry supplies the mixed components already determined. The trace condition becomesThe independent components are , and the trace-free part of . Under transverse rotations they form a scalar representation, a vector representation, and a symmetric traceless rank-two tensor. ThereforeThis is the light-cone decomposition of a massive spin-two field for . In , the trace and divergence give and . The massive wave equation then forces , so there are no polarizations, consistent with the zero value of the printed count. The massive particle little group is , and its symmetric traceless square branches asThe mixed components with the extra direction give the vector; one independent trace combination gives the scalar. These are exactly the polarizations of a massive spin-two field. The remaining independent components retain the massive Klein-Gordon equation.
Transverse bosonic modes and mass levels. The variables are Fourier amplitudes of the physical transverse open-string mode expansion. Classically, reality requires . The symplectic term in the action fixes their quantum commutators:With string tension convention , the zero mode of the constraint givesThe longitudinal nonzero modes have already been removed in light-cone gauge in string theory. Quantum normal ordering introduces the string intercept , giving the open bosonic string mass spectrumEach bosonic occupation number is a nonnegative integer, so is a nonnegative integer weighted by oscillator frequency.
Suppressing the common momentum label, the lowest light-cone levels of an open bosonic string areThe oscillator vacuum is annihilated by every positive . At level one there are only vector polarizations. For a Lorentz-consistent vector, these are the transverse polarizations of a massless particle, transforming under the rotation part of its massless particle little group. A massive vector would need polarizations, including a scalar under that is absent here. Thus the first bosonic vector level must be massless, fixing .
At level two the commuting creation operators give a symmetric square. Its scalar trace and symmetric traceless square, together with the mode-two vector, are the massive-spin-two decomposition above. In the consistent bosonic theory they form one massive spin-two field with . The covariant equations describe its propagation while eliminating the redundant components. For the transverse counts are , the symmetric traceless rank-two tensor dimension of .
Half-integer fermionic modes. The Neveu–Schwarz sector has antiperiodic worldsheet Majorana fermions. Its Neveu–Schwarz fermionic oscillators obeyThe oscillator vacuum satisfies for and for . A negative fermion mode is a fermionic creation operator for a transverse worldsheet excitation. The Neveu–Schwarz level operator and mass condition areThe smallest positive frequency is , so the only first-excited states areThe same vector-polarization argument requires them to be massless in Lorentz-consistent quantization, fixing .
At , is a vector, while is the exterior square: interchanging the indices changes the sign and equal indices give zero. Together they branch from an antisymmetric tensor:Thus the Neveu–Schwarz level-one massive tensor has polarizations and mass squared . It differs from spin two because the two-fermion tensor is antisymmetric and has neither the symmetric trace-free representation nor its scalar trace. At , the count is , compared with for a massive spin-two field. The specified states are before the GSO projection; the usual tachyon-removing GSO projection also removes this integer level.
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.
Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 306 3 c Solution Created 2026-10-03 Updated 2026-10-05
Use the classically equivalent Polyakov action, fix worldsheet diffeomorphisms and Weyl invariance, and perform a Wick rotation of the string worldsheet. In complex coordinates, the worldsheet ghost action for the closed string isThe worldsheet ghost fields are anticommuting. Their conformal weights are , and , . The two chiral sectors are counted separately.
In either chiral sector, each embedding coordinate is a free boson conformal field theory with central charge one. For the bc system, putting in gives . Cancellation of the worldsheet Weyl anomaly requiresThe antiholomorphic sector gives the same equation, rather than doubling the required critical dimension of string theory. This dimension count assumes flat target spacetime with just the embedding fields; more general internal conformal field theories change the matter accounting.
For the spinning string, the worldsheet Majorana fermions have conformal weight . At , the complex anticommuting bc system has ; a real Majorana spinor contributes half of this. Hence real worldsheet Majorana fermions contribute per chiral sector. Ramond sector versus Neveu–Schwarz sector changes their mode numbers and vacuum energies, not this local central charge.
The additional local worldsheet supersymmetry has a fermionic gauge parameter, so its superconformal ghosts are commuting fields forming a beta-gamma system, with conformal weights and in the holomorphic sector. Commuting statistics reverse the sign of the bc system formula, givingTogether with the reparameterization worldsheet ghost fields, their total central charge is . ThusThese cancellations make the string worldsheet gauge symmetries compatible with quantization; in the BRST symmetry formulation they enter the nilpotence condition for the BRST operator.
Ramond sector Created 2026-10-05 Updated 2026-10-06
Spinning string Created 2026-10-05 Updated 2026-10-06
The spinning string adds worldsheet Majorana fermions and local worldsheet supersymmetry to the embedding coordinates. Its gauge-fixed quantum description is the Ramond–Neveu–Schwarz formulation of the superstring.
Before the GSO projection, the Neveu–Schwarz sector has string oscillator levels , with physical multiplicities in ten-dimensional light-cone gauge in string theory. The eight transverse worldsheet Majorana fermions supply eight single states. Level one has eight states and pairs of distinct modes. Level has single modes, mixed boson–fermion modes and triples. Their squared masses are respectively . In the Ramond sector, the Ramond zero-mode Clifford algebra gives a sixteen-dimensional ground space. At level one, and each provide states, hence multiplicities at squared masses . No half-integer Ramond levels occur. The GSO projection keeps odd NS fermion number and one total Ramond chirality, giving bosons and fermions at zero mass, then of each at the first massive level.
Worldsheet gravitino Created 2026-10-05 Updated 2026-10-06
The worldsheet gravitino is the fermionic vector-spinor gauge field for local worldsheet supersymmetry, paired with the worldsheet metric in two-dimensional supergravity. In a locally supersymmetric string action it couples to the worldsheet supercurrent. Fixing its gauge and the bosonic conformal gauge leaves the usual flat rigid transformations on embeddings and worldsheet Majorana fermions; it should not be silently omitted when claiming an arbitrary curved-worldsheet locally supersymmetric action.
Worldsheet supersymmetry 2026-10-05
Local supersymmetry on a string worldsheet relates embedding coordinates to their worldsheet Majorana fermion partners. Fixing this fermionic gauge symmetry introduces commuting superconformal ghosts.