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A backward \(\lambda \)-lemma for the forward heat flow

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Abstract

The inclination or \(\lambda \)-lemma is a fundamental tool in finite dimensional hyperbolic dynamics. In contrast to finite dimension, we consider the forward semi-flow on the loop space of a closed Riemannian manifold \(M\) provided by the heat flow. The main result is a backward \(\lambda \)-lemma for the heat flow near a hyperbolic fixed point \(x\). There are the following novelties. Firstly, infinite versus finite dimension. Secondly, semi-flow versus flow. Thirdly, suitable adaption provides a new proof in the finite dimensional case. Fourthly and a priori most surprisingly, our \(\lambda \)-lemma moves the given disk transversal to the unstable manifold backward in time, although there is no backward flow. As a first application we propose a new method to calculate the Conley homotopy index of \(x\).

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Notes

  1. Note that the difference lies in \(X^-\), hence in \(C^\infty \). Therefore it makes sense to take the \(C^1\) norm.

  2. Hence \(f\circ \xi :(0,T]\rightarrow Y\) is continuous and, by the Lipschitz Lemma 1, bounded.

  3. Otherwise, choose \(\rho _0>0\) smaller. This leads to a smaller \({\varepsilon }\) in Hypothesis 1 (a). Condition (18) is used in step 4 and in the proof of Theorem 2, both concerning \(C^1\).

  4. The definition of \(T_1\) ensures in step 2 the second of the two endpoint conditions (21).

  5. The conditions on \(T_2\) will be used in step 6, in particular in (39).

  6. The argument relies on the right boundary of the \(t\)-interval running to \(-\infty \), as \(T\rightarrow \infty \). Therefore the right boundary of \(II\) needs to be strictly smaller than \(T\), but at the same time be element of \([0,T]\) whichever \(T\) we pick. Thus any \(\alpha T\) with \(0<\alpha <1\) is a good choice.

  7. Exponential decay is achieved, if the left boundary of \(\textit{III}\) is of the form \(\alpha T\) with \(\alpha >\frac{1}{2}\).

  8. Here and throughout \(\left( \int _a^b +\int _c^d\right) f\) abbreviates \(\int _a^b f+\int _c^d f\).

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Acknowledgments

For hospitality I would like to thank Universität Bielefeld where foundations were laid. In this respect I am most grateful to Helmut Hofer for the right words in a difficult moment. Many thanks to André de Carvalho and Pedro Salomão for building the bridge to a new continent and, in particular, the excellent research conditions provided by IME USP and FAPESP. Last, not least, the paper would not exist without Dietmar Salamon teaching me for many years his way of solving complex problems. I owe him deeply.

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Correspondence to Joa Weber.

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Research supported by Universität Bielefeld and Fundação de Amparo à Pesquisa do Estado de São Paulo, FAPESP grants 2011/01830-1 and 2013/20912-4.

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Weber, J. A backward \(\lambda \)-lemma for the forward heat flow. Math. Ann. 359, 929–967 (2014). https://doi.org/10.1007/s00208-014-1026-6

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