nLab Seiberg-Witten equations

Contents

Context

Quantum field theory

Super-Geometry

Contents

Idea

The Seiberg-Witten equations are partial differential equations for connections of principal U(1)-bundles and smooth sections of their spinor bundles. Their moduli space is used to define the Seiberg-Witten invariants capable to study smooth structures on 4-manifolds. Since the gauge group of the Seiberg-Witten equations is abelian, many calculations could be simplified with new methods provided by them.

Basics

Let MM be a compact orientable Riemannian 4-manifold with a Riemannian metric gg and spinᶜ structure 𝔰\mathfrak{s}. Both always exist. In particular the latter is a lift of the classifying map τ:MBSO(4)\tau\colon M\rightarrow BSO(4) of the tangent bundle TMτ *γ 4TM\cong\tau^*\gamma_\mathbb{R}^4 to a map 𝔰:MBSpin c(4)\mathfrak{s}\colon M\rightarrow BSpin^\mathrm{c}(4). Because of the exceptional isomorphism:

Spin c(4)U(2)× U(1)U(2)={A ±U(2)|det(A )=det(A +)} Spin^\mathrm{c}(4) \cong U(2)\times_{U(1)}U(2) =\{A^\pm\in U(2)|det(A^-)=det(A^+)\}

the spinᶜ structure 𝔰\mathfrak{s} consists of two complex plane bundles W ±MW^\pm\twoheadrightarrow M, called associated spinor bundles, with same determinant line bundle L=det(W ±)L=det(W^\pm). Since it preserves the first Chern class one has c 1(L)=c 1(W ±)H 2(M,)c_1(L)=c_1(W^\pm)\in H^2(M,\mathbb{Z}). Furthermore let W=W W +W=W^-\oplus W^+ be the Whitney sum of the spinor bundles.

Seiberg-Witten equations

Covariant derivatives:Γ (L)Γ (T *ML)\nabla\colon\Gamma^\infty(L)\rightarrow\Gamma^\infty(T^*M\otimes L) on the determinant line bundle LL, which are linear and fulfill the Leibniz rule, induce principal connections on the frame bundle Fr U(L)Fr_U(L), which is a principal U(1)-bundle, using the following isomorphisms:

Hom(Γ (L),Γ (T *ML))Γ Hom̲(L,T *ML)Γ (T *ML *L)Γ (T *MEnd̲(L))Ω 1(M,End̲(L))Ω 1(M,AdFr U(L))Ω Ad 1(Fr U(L),𝔲(1)) \Hom(\Gamma^\infty(L),\Gamma^\infty(T^*M\otimes L)) \cong\Gamma^\infty\underline{Hom}(L,T^*M\otimes L) \cong\Gamma^\infty(T^*M\otimes L^*\otimes L) \cong\Gamma^\infty(T^*M\otimes\underline{End}(L)) \cong\Omega^1(M,\underline{End}(L)) \cong\Omega^1(M,Ad Fr_U(L)) \cong\Omega_{Ad}^1(Fr_U(L),\mathfrak{u}(1))

(In particular, since LL is a line bundle, one has End̲(L)𝔲(1)̲\underline{End}(L)\cong\underline{\mathfrak{u}(1)}, which can be seen with the fact that the identity provides a global section.)

Since the first unitary group U(1)U(1) is abelian, the Seiberg-Witten equations obtain a strong simplification compared to the Yang-Mills equations, which are usually considered with non-abelian gauge groups. In particular this can be seen for the curvature form simplifying to F A=dAF_A=d A. Its self-dual part is then given by:

F A +=12(F A+F A)=12(dA+dA). F_A^+ =\frac{1}{2}(F_A+\star F_A) =\frac{1}{2}(d A+\star d A).

Smooth sections of W W^-, whose space is denoted Γ (W )\Gamma^\infty(W^-) (or short Γ(W )\Gamma(W^-)), are called antiselfdual spinor fields (or short ASD spinor fields). Smooth sections of W +W^+, whose space is denoted Γ (W +)\Gamma^\infty(W^+) (or short Γ(W +)\Gamma(W^+)), are called selfdual spinor fields (or short SD spinor fields). A connection like above induces a Dirac operator D A:Γ (W +)Γ (W )D^A\colon\Gamma^\infty(W^+)\rightarrow\Gamma^\infty(W^-). Furthermore the Riemannian metric induces scalar products ,:W ±W ±̲\langle-,-\rangle\colon W^\pm\oplus W^\pm\rightarrow\underline{\mathbb{R}}.

Now the Seiberg-Witten equations are partial differential equations for a connection AΩ 1(M,𝔲(1))A\in\Omega^1(M,\mathfrak{u}(1)) and a self-dual spinor field ϕΓ (W +)\phi\in\Gamma^\infty(W^+), often given as undisturbed Seiberg-Witten equations without and disturbed Seiberg-Witten equations with a self-dual form ηΩ + 2(M,𝔲(1))\eta\in\Omega_+^2(M,\mathfrak{u}(1)) as:

D Aϕ=0; D^A\phi =0;
F A ++τ(ϕ)+η=0. F_A^+ +\tau(\phi) +\eta =0.

Considering the undisturbed Seiberg-Witten equations with a vanishing spinor field ϕ=0\phi=0 yields the anti self-dual Yang-Mills equations (ASDYM equations) F A +=0F_A^+=0.

References

See also:

Last revised on August 8, 2025 at 23:26:17. See the history of this page for a list of all contributions to it.