Abstract
The heat flow for Dirac-harmonic maps on Riemannian spin manifolds is a modification of the classical heat flow for harmonic maps by coupling it to a spinor. It was introduced by Chen, Jost, Sun, and Zhu as a tool to get a general existence program for Dirac-harmonic maps. For source manifolds with boundary they obtained short time existence, and the existence of a global weak solution was established by Jost, Liu, and Zhu. We prove short time existence of the heat flow for Dirac-harmonic maps on closed manifolds.
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Notes
Note that \(ind _{f^*TN}(M)\) depends on the choice of a topological spin structure on M, but doesn’t depend on the Riemannian metrics on M and N. Moreover, \(ind _{g^*TN}(M)=ind _{f^*TN}(M)\) for any g in the homotopy class of f.
Parametrized on [0, 1]
For this chain of equations one has to be a little careful, since we argue with the curvature of \(F^*TN\), but F is only a \(C^1\)-mapping. However, all the expressions exist (e.g. in the sense that the exist in local coordinates) and all the equalities hold.
If \(m\not \equiv 3 \text { }(mod 4)\), then the spectrum of is symmetric w.r.t. zero. This can be shown analogously to [13, Theorem 1.3.7 iv)].
Here we use that \(p\ge 0\) and \(\int _M p(x,y,t)\,dV(y)=1\) for all \((x,t)\in M\times (0,\infty )\). Moreover, we use that there exists \(C>0\) s.t. \(\int _{0}^{t}\int _M|\nabla _x p(x,y,s)|\,dV(y)ds\le C \sqrt{t}\) for all \((x,t)\in M\times [0,1]\). The latter is not difficult to show. It follows directly from the construction of the heat kernel (see e.g. [5]). It is shown in detail in [11] or [30].
To show that \(W^{1,2,p}((0,T)\times M)\subset C^{0,1,\alpha }((0,T)\times M)\) for p large enough (the spaces are defined as in [27]) one needs the Sobolev embedding and interpolation theory.
Note that here \(T>0\) is just some T s.t. Theorem 1 holds. It does not need to be related to the T we constructed in the first step.
This can be seen as follows: we write \(u=u^i\). Since \(u\in C^{1,2,\alpha }((0,T)\times M)\subset C^{0,\frac{\alpha }{2}}((0,T);C^2(M))\) (c.f. [27]) we have in particular that \(u,\nabla u:(0,T)\rightarrow C^0(M)\) are \(\frac{\alpha }{2}\)-Hölder continuous. (In the case of \(\nabla u\) we write \(C^0(M)\) as target space shortly for \(\varGamma (TM)\) with the \(C^0\)-norm.) Hence \(u,\nabla u:(0,T)\rightarrow C^0(M)\) are uniformly continuous and can therefore be continuously extended to \(u,\nabla u:[0,T]\rightarrow C^0(M)\). Hence \(u(t,.)\rightarrow u_0\) in \(C^0(M)\) as \(t\rightarrow 0\) and there exists a vector field \(V\in \varGamma (TM)\) s.t. \(\nabla u(t,.)\rightarrow V\) in \(C^0(M)\) as \(t\rightarrow 0\). We show \(V=\nabla u_0\). To that end, notice that for every \(X\in \varGamma (TM)\) we have
$$\begin{aligned} \int _M\langle \nabla u(t,.),X\rangle =-\int _Mu(t,.)div (X)\xrightarrow {t\rightarrow 0} -\int _M u_0div (X)=\int _M\langle \nabla u_0,X\rangle , \end{aligned}$$and
$$\begin{aligned} \int _M\langle \nabla u(t,.),X\rangle \xrightarrow {t\rightarrow 0}\int _M\langle V,X\rangle . \end{aligned}$$Since and , we can assume w.l.o.g. that \(\psi ^1_{T_0}=\psi ^2_{T_0}\). Otherwise we replace \(\psi ^2\) by \(\psi ^2h\), where \(h\in \mathbb {K}\) has unit length with \(\psi ^1_{T_0}=\psi ^2_{T_0}h\).
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Acknowledgements
I would like to thank Bernd Ammann and Helmut Abels for their ongoing support and many fruitful discussions. I am also grateful to Ulrich Bunke for his valuable input. My work was supported by the DFG Graduiertenkolleg GRK 1692 “Curvature, Cycles, and Cohomology”.
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Wittmann, J. Short time existence of the heat flow for Dirac-harmonic maps on closed manifolds. Calc. Var. 56, 169 (2017). https://doi.org/10.1007/s00526-017-1270-1
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DOI: https://doi.org/10.1007/s00526-017-1270-1