Zero-rest-mass field equations and the spinor form of Maxwell, Weyl, and Dirac fields
Anchor (Master): Penrose-Rindler 1984 *Spinors and Space-Time, Vol. 1* (Cambridge) Ch. 5 §§5.7-5.8 (zero-rest-mass fields, Buchdahl condition); Buchdahl 1958 *Nuovo Cimento* 10, 96-103; Stewart 1990 *Advanced General Relativity* (Cambridge) Ch. 2
Intuition Beginner
A massless particle moves at the speed of light, and there is no frame in which it sits still. That single fact reshapes how its field is described. A particle with rest mass, like an electron, can be brought to rest and turned slowly in your hands; you can ask which way its spin points in any direction. A massless particle never stops, so its spin can only be read along its direction of travel. The two readings you ever get are "spinning the way a right-handed screw advances" or the left-handed mirror image. This single, sign-carrying number is called the helicity.
Spinors are the natural language for this story. A spinor is the squarest-possible root of a direction in spacetime: where a velocity arrow needs four numbers, a spinor needs two complex ones, and a velocity along the light cone is built by squaring a spinor. Light-cone directions and spinors fit together perfectly, which is why massless fields look simplest when written with spinors.
The punchline of this unit is that one compact spinor equation, with a tower of indices whose length records the spin, contains the source-free Maxwell equations, the equation for a massless spin-half particle, and (with a small twist) the Dirac equation, all at once.
Visual Beginner
Alt text: At the centre sits a single equation reading "spinor divergence of a symmetric spinor with 2s indices equals zero." Three arrows point outward to boxes. The spin-one arrow reaches Maxwell, a light ray with a dial reading plus or minus one for the photon's two helicities. The spin-one-half arrow reaches Weyl, a single light ray with a dial reading plus or minus one half. The third arrow reaches Dirac, drawn as two linked spinor symbols joined by a mass term, showing that a massive particle needs two coupled fields. The figure shows how varying the index count s reproduces three field theories, each labelled by helicity.
Worked example Beginner
Take the electromagnetic field. In the usual telling it is six numbers: a three-component electric field and a three-component magnetic field, packaged into the antisymmetric field tensor with components . Counting carefully, an antisymmetric pair of four-valued indices has six independent slots, matching the six numbers.
Now repackage. The six real numbers can be rewritten as three complex numbers, namely the electric field plus times the magnetic field. These three complex numbers are exactly the independent components of a symmetric spinor with two lower indices, written , which also has three slots because a symmetric pair of two-valued indices has three. The dictionary is a clean match: six real becomes three complex becomes the spinor .
What this buys us: the four Maxwell equations, in empty space, collapse into the single statement that a certain spinor derivative of is zero. The two source-free Maxwell equations that say the divergence and the curl behave correctly are repackaged into one tidy spinor equation. The same trick, with a shorter or longer tower of indices, handles spin one half and spin two.
Check your understanding Beginner
Formal definition Intermediate+
We work on Minkowski space (and later a curved Lorentzian -manifold) equipped with the two-spinor calculus of 03.02.41: a complex rank-two spin space with symplectic form , its complex conjugate with primed indices, and the soldering isomorphism between complexified tangent vectors and elements of . Indices are raised and lowered with , (and their primed versions) by the conventions , . The spinor covariant derivative is the soldered form of the Levi-Civita connection, annihilating .
Definition (zero-rest-mass field). A zero-rest-mass free field of spin ( a positive integer) is a totally symmetric spinor field $$ \phi_{AB\cdots L} = \phi_{(AB\cdots L)}, \qquad n = 2s \ \text{indices}, $$ satisfying the zero-rest-mass field equation $$ \nabla^{AA'}\phi_{AB\cdots L} = 0 . $$ The derivative is contracted against the first index; by total symmetry the choice of contracted index is immaterial. The conjugate field describes the opposite helicity. The number of unprimed versus primed indices is the helicity grading: with unprimed indices has helicity , and has helicity .
The Maxwell spinor (). A real antisymmetric two-form decomposes, via the dictionary of 03.02.41, as
$$
F_{ab} = \phi_{AB},\varepsilon_{A'B'} + \bar\phi_{A'B'},\varepsilon_{AB},
\qquad \phi_{AB} = \tfrac12 F_{ab},\varepsilon^{A'B'} = \phi_{(AB)},
$$
where is the Maxwell spinor. The first term is the anti-self-dual part of and the second its self-dual part (the complex conjugate); the split of a real two-form into plus complex conjugate is the (anti-)self-dual decomposition. The source-free Maxwell equations and together read, in spinor form, — the case of the master equation.
The Weyl (neutrino) field (). A single unprimed spinor field obeying
$$
\nabla^{AA'}\phi_A = 0
$$
is the Weyl field, the massless spin-half field of one definite helicity. This is the chiral, two-component reduction of the Dirac field at zero mass 12.11.01.
The Dirac field as a coupled pair. A Dirac -spinor splits into a pair — an unprimed and a primed two-spinor, the two chiral halves 12.11.01. With mass parameter (in natural units) the Dirac equation becomes the coupled first-order pair
$$
\nabla^{AA'}\phi_A = \mu,\chi^{A'}, \qquad \nabla_{AA'}\chi^{A'} = \mu,\phi_A .
$$
Setting decouples the pair into two independent Weyl equations, recovering the massless case for each chirality.
Counterexamples to common slips
- Symmetry is not optional. A solution of with not totally symmetric is not a spin- zero-rest-mass field; its antisymmetric parts carry lower-spin content and obey different equations. The symmetric projection is part of the definition.
- Helicity is the index imbalance, not the index count. A field with equal numbers of primed and unprimed indices (a tensor field) has helicity zero in this grading; helicity is the difference of unprimed and primed counts, halved. Doubling all indices does not double the helicity if you add them symmetrically on both index types.
- The massive case needs two fields. One cannot write the massive Dirac equation as a single symmetric spinor equation. Mass couples the two chiralities, so a primed partner is mandatory; a lone with a mass term on the right is inconsistent unless a is supplied to receive it.
Key theorem with proof Intermediate+
Theorem (Maxwell recovery and helicity). Let be a Maxwell spinor on Minkowski space and let be the associated real two-form. Then the single spinor equation is equivalent to the full set of source-free Maxwell equations and . Moreover the positive- and negative-helicity photon states correspond to and respectively.
Proof. Apply to the decomposition of . In two-spinor form the divergence and the exterior-derivative parts of are governed by the symmetric and antisymmetric parts of in the index . Compute and split it on the free unprimed index and free primed index . The contraction is a spinor with one lower unprimed index and one upper primed index , hence corresponds to a covector , and the real and imaginary parts of the equation are precisely the divergence equation and the Bianchi/curl equation . Concretely, writing and using together with , the four-vector equals , which vanishes for all iff ; the homogeneous Maxwell pair is the conjugate statement, automatically included because is real. The two-to-one correspondence between and the pair shows the field carries exactly the two photon polarisations, the self-dual part and the anti-self-dual part , which are the helicity and states.
This is the prototype: a tensor field equation has been turned into a contracted-derivative condition on a symmetric spinor, and the (anti-)self-dual split that is awkward in tensor language is the plain real-and-imaginary split of .
Bridge. This recovery builds toward the unified spin- picture and appears again in the linearised gravity case , where the same contracted-derivative equation governs the Weyl spinor of 03.02.18. The foundational reason the spinor form is cleaner is that the irreducible pieces of a Lorentz tensor are exactly the totally symmetric spinors, so the (anti-)self-dual decomposition is dual to the split of into itself and its conjugate; this is exactly the pattern by which the Maxwell field, the Weyl neutrino, and the linearised graviton become a single equation graded by index count. Putting these together, the central insight is that helicity is read directly off the imbalance between primed and unprimed indices, and the zero-rest-mass equation generalises the source-free Maxwell system to every half-integer spin.
Exercises Intermediate+
Advanced results Master
The full spin- tower and conserved currents. For each the equation on Minkowski space admits a positive-frequency solution space carrying the irreducible massless helicity- representation of the Poincaré group [Penrose-Rindler §5.7], matching the Wigner classification 07.07.06. The field carries a conserved, symmetric stress-energy-type current quadratic in ; for this is the Maxwell stress tensor, and for the linearised Bel-Robinson tensor of 03.02.18. The contour-integral solution via the Penrose transform produces exactly these helicity- fields as cohomology classes on twistor space 03.07.14, so the present equation is the spacetime shadow of that complex-analytic construction.
Maxwell as and linearised gravity as . The Maxwell spinor and its equation reproduce source-free electromagnetism, with the principal null directions of (the spinors with ) marking the special null directions of the field. For , the totally symmetric is the linearised Weyl curvature spinor, and is the linearised vacuum Bianchi identity; its four principal null spinors and their coincidence pattern are the Petrov classification of 03.02.18. The peeling behaviour at null infinity — the falloff sorted by Petrov type — is a statement about this spinor field along outgoing null geodesics.
The Buchdahl consistency condition. In a general curved Lorentzian background the equation for is overdetermined: cross-differentiating and applying the spinor Ricci identities yields an algebraic constraint coupling to the conformal curvature spinor . For this Buchdahl condition generically forces to vanish unless the background is algebraically special or conformally flat [Buchdahl 1958]. Thus higher-spin massless fields do not propagate freely on a generic curved metric — a genuine obstruction with no analogue for , where Maxwell and Weyl theory remain consistent on any background.
The massive case and the Dirac pair. Mass is the off-diagonal coupling , . Eliminating gives the spinor wave equation up to a curvature term, recovering the Klein-Gordon mass shell . The same coupling pattern generalises to higher-spin massive fields as towers of symmetric spinors linked by mass terms, the spinor incarnation of the Bargmann-Wigner equations.
Synthesis. The zero-rest-mass equation is the foundational reason a single object unifies three classical field theories: this is exactly the statement that the irreducible content of a massless relativistic field is a totally symmetric spinor, graded by helicity. Putting these together, Maxwell () generalises to the linearised graviton () and reduces to the Weyl neutrino (), while the massive Dirac field is dual to a coupled primed-unprimed pair whose decoupling at zero mass returns the Weyl case. The central insight is that helicity is the primed-versus-unprimed index imbalance, the (anti-)self-dual split is the real-imaginary split of the field spinor, and the Buchdahl obstruction shows precisely where this clean picture breaks under curvature for — the bridge from flat-space field theory to curved-space relativity, and the spacetime end of the twistor correspondence of 03.07.14.
Full proof set Master
Proposition (component count and helicity content). The totally symmetric spinor with indices has independent complex components, and the solution space of carries helicity (its conjugate, helicity ).
Proof. A symmetric spinor in two-valued indices is determined by how many of its indices equal (the rest equal ), giving the values , hence complex components. For the helicity, decompose a plane-wave solution with a null covector (this is the general null-datum ansatz). The field equation forces on the wave, i.e. the propagation direction is the repeated principal spinor; the response of to a rotation about multiplies it by , the defining transformation of helicity . The conjugate field transforms by .
Proposition (Maxwell equivalence). For real , the system holds iff .
Proof. Using , the four-vector in spinor form is , where the soldering identifies the free indices with the covector index . Its vanishing is the condition . The homogeneous pair is the complex conjugate of the same spinor equation, automatically holding because is real and is symmetric: the antisymmetric part of on the indices vanishes by symmetry of , leaving only the symmetric part, whose reality content is the inhomogeneous equation and whose imaginary content is the Bianchi equation. Hence the single complex spinor equation encodes both Maxwell pairs.
Proposition (Buchdahl obstruction for ). On a curved background, with implies the algebraic identity , where is the Weyl conformal spinor.
Proof. Apply to the field equation and antisymmetrise the two unprimed derivative indices to form the spinor curvature operator . The spinor Ricci identities give acting on a spinor index as a contraction with (the conformally invariant part) plus a Ricci-spinor term that cancels in vacuum or by the trace structure. Feeding the field equation in to remove the symmetric-derivative part leaves the purely algebraic curvature contraction; total symmetry of projects it onto . For this is a nonempty constraint, the Buchdahl condition [Buchdahl 1958]; for the symmetrisation kills it and no obstruction arises.
The detailed spinor Ricci identities and the full Bargmann-Wigner generalisation to massive higher-spin fields are stated above without proof — see Penrose-Rindler [Penrose-Rindler §5.8] and Wald [Wald §13.2].
Connections Master
The two-spinor calculus and the spinor-tensor dictionary
03.02.41. That unit (co-produced in this wave) builds the -spinor, the soldering form , and the decomposition of an antisymmetric two-form that this unit uses to write Maxwell as . The spinor covariant derivative appearing in every field equation here is the soldered Levi-Civita connection defined there.The Newman-Penrose spin-coefficient formalism
03.02.43. That unit (co-produced in this wave) turns the abstract into component equations along a null tetrad, expressing the Maxwell scalars and the Weyl scalars and their NP-equation dynamics; the present equation is the covariant statement that the NP formalism makes computational.The Dirac equation, relativistic spin
12.11.01. This unit recasts the four-component Dirac equation built there as the coupled two-spinor pair , , and identifies the massless chiral halves with the Weyl field. The chiral projectors there become the split into primed and unprimed spinors here.Free Maxwell and the Proca field
12.05.06. The source-free Maxwell system established there is exactly the case ; the photon's two helicities are the Maxwell spinor and its conjugate, and the electric-magnetic duality rotation is the phase freedom of .The Petrov classification and the Weyl spinor
03.02.18. The field is the linearised Weyl spinor classified there; its four principal null directions and their coincidences are the Petrov types, and the peeling theorem describes this spinor field at null infinity.
Historical & philosophical context Master
The spinor form of the massless field equations grew out of the van der Waerden two-spinor calculus of the late 1920s and reached its mature, geometrically explicit form in the work of Roger Penrose and Wolfgang Rindler, whose Spinors and Space-Time, Vol. 1 (Cambridge University Press, 1984) devotes its fifth chapter to the zero-rest-mass fields and presents the equation as a single object subsuming Maxwell, Weyl, and (in coupled form) Dirac [Penrose-Rindler §5.7]. The viewpoint that helicity is the fundamental label of a massless field — and that this label is read directly off the imbalance of primed and unprimed spinor indices — became the conceptual seed of the twistor programme, in which these fields are repackaged as cohomology on a complex projective space.
The obstruction to propagating higher-spin massless fields on a curved background was identified by H. A. Buchdahl, whose 1958 paper in Il Nuovo Cimento showed that the wave equations for particles of spin greater than one are inconsistent in a general gravitational field unless an algebraic curvature condition holds [Buchdahl 1958]. This result anticipated the modern no-go theorems for interacting higher-spin fields and sharpened the special status of spins , , and — the spins realised by the known fundamental fields. Wald's General Relativity (University of Chicago Press, 1984) and Stewart's Advanced General Relativity (Cambridge University Press, 1990) gave the now-standard textbook treatments tying the spinor field equations to the tetrad and Newman-Penrose machinery [Wald §13.2].
Bibliography Master
@book{PenroseRindler1984,
author = {Penrose, Roger and Rindler, Wolfgang},
title = {Spinors and Space-Time, Volume 1: Two-Spinor Calculus and Relativistic Fields},
publisher = {Cambridge University Press},
year = {1984},
note = {Chapter 5, especially \S\S5.7--5.8 (zero-rest-mass fields, Buchdahl condition)}
}
@article{Buchdahl1958,
author = {Buchdahl, H. A.},
title = {On the compatibility of relativistic wave equations for particles of higher spin in the presence of a gravitational field},
journal = {Il Nuovo Cimento},
volume = {10},
pages = {96--103},
year = {1958}
}
@book{Wald1984,
author = {Wald, Robert M.},
title = {General Relativity},
publisher = {University of Chicago Press},
year = {1984},
note = {Chapter 13 (spinors), \S13.2 (massless fields)}
}
@book{Stewart1990,
author = {Stewart, John},
title = {Advanced General Relativity},
publisher = {Cambridge University Press},
year = {1990},
note = {Chapter 2 (spinors and the spinor form of the field equations)}
}
@book{ODonnell2003,
author = {O'Donnell, Peter},
title = {Introduction to 2-Spinors in General Relativity},
publisher = {World Scientific},
year = {2003}
}
@article{NewmanPenrose1962,
author = {Newman, Ezra and Penrose, Roger},
title = {An approach to gravitational radiation by a method of spin coefficients},
journal = {Journal of Mathematical Physics},
volume = {3},
pages = {566--578},
year = {1962}
}