In heterotic string theory, the Strominger's equations are the set of equations that are necessary and sufficient conditions for spacetime supersymmetry. It is derived by requiring the 4-dimensional spacetime to be maximally symmetric, and adding a warp factor on the internal 6-dimensional manifold. Consider a metric ω {\displaystyle \omega } on the real 6-dimensional internal manifold Y and a Hermitian metric h on a vector bundle V. The equations are:
The 4-dimensional spacetime is Minkowski, i.e., g = η {\displaystyle g=\eta } . The internal manifold Y must be complex, i.e., the Nijenhuis tensor must vanish N = 0 {\displaystyle N=0} . The Hermitian form ω {\displaystyle \omega } on the complex threefold Y, and the Hermitian metric h on a vector bundle V must satisfy,
∂ ∂ ¯ ω = i Tr F ( h ) ∧ F ( h ) − i Tr R − ( ω ) ∧ R − ( ω ) , {\displaystyle \partial {\bar {\partial }}\omega =i{\text{Tr}}F(h)\wedge F(h)-i{\text{Tr}}R^{-}(\omega )\wedge R^{-}(\omega ),}
d † ω = i ( ∂ − ∂ ¯ ) ln | | Ω | | , {\displaystyle d^{\dagger }\omega =i(\partial -{\bar {\partial }}){\text{ln}}||\Omega ||,} where R − {\displaystyle R^{-}} is the Hull-curvature two-form of ω {\displaystyle \omega } , F is the curvature of h, and Ω {\displaystyle \Omega } is the holomorphic n-form; F is also known in the physics literature as the Yang-Mills field strength. Li and Yau showed that the second condition is equivalent to ω {\displaystyle \omega } being conformally balanced, i.e., d ( | | Ω | | ω ω 2 ) = 0 {\displaystyle d(||\Omega ||_{\omega }\omega ^{2})=0} . The Yang–Mills field strength must satisfy,
ω a b ¯ F a b ¯ = 0 , {\displaystyle \omega ^{a{\bar {b}}}F_{a{\bar {b}}}=0,}
F a b = F a ¯ b ¯ = 0. {\displaystyle F_{ab}=F_{{\bar {a}}{\bar {b}}}=0.}
These equations imply the usual field equations, and thus are the only equations to be solved. However, there are topological obstructions in obtaining the solutions to the equations;
The second Chern class of the manifold, and the second Chern class of the gauge field must be equal, i.e., c 2 ( M ) = c 2 ( F ) {\displaystyle c_{2}(M)=c_{2}(F)}
A holomorphic n-form Ω {\displaystyle \Omega } must exists, i.e., h n , 0 = 1 {\displaystyle h^{n,0}=1} and c 1 = 0 {\displaystyle c_{1}=0} . In case V is the tangent bundle T Y {\displaystyle T_{Y}} and ω {\displaystyle \omega } is Kähler, we can obtain a solution of these equations by taking the Calabi–Yau metric on Y {\displaystyle Y} and T Y {\displaystyle T_{Y}} . Once the solutions for the Strominger's equations are obtained, the warp factor Δ {\displaystyle \Delta } , dilaton ϕ {\displaystyle \phi } and the background flux H, are determined by
Δ ( y ) = ϕ ( y ) + constant {\displaystyle \Delta (y)=\phi (y)+{\text{constant}}} ,
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