Abstract
We study the perfect conductivity problem with closely spaced perfect conductors embedded in a homogeneous matrix where the current-electric field relation is the power law \(J=\sigma |E|^{p-2}E\). The gradient of solutions may be arbitrarily large as \(\varepsilon \), the distance between inclusions, approaches to 0. To characterize this singular behavior of the gradient in the narrow region between two inclusions, we capture the leading order term of the gradient. This is the first gradient asymptotics result on the nonlinear perfect conductivity problem.
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Hongjie Dong was partially supported by the NSF under agreement DMS-2055244. Zhuolun Yang was partially supported by Simons Foundation Institute Grant Award ID 507536 and the AMS-Simons Travel Grant. Hanye Zhu was partially supported by the NSF under agreement DMS-2055244.
Appendix A
Appendix A
In the first part of the appendix, we prove Proposition 4.2. The proof essentially follows those of [26, Proposition 2.1] and [15, Lemma 5.1]. Our estimate is sharper due to a better estimate on \(|Du_0|\) (Proposition 2.2).
Proof of Proposition 4.2
Similar to the proof of Theorem 2.5, for small \(r \in (0,1/2)\), we take a smooth surface \(\eta \) so that \(\mathcal {D}_1^\varepsilon \) is surrounded by \(\Gamma _{-,s}^0 \cup \eta \). See Fig. 1. We denote the surface
Since \(\int _{\partial \mathcal {D}_1^{0}} |D u_{0}|^{p-2} D u_{0} \cdot \nu = \mathcal {F}\) and \(\int _{\partial \mathcal {D}_1^{\varepsilon }} |D u_{\varepsilon }|^{p-2} D u_{\varepsilon } \cdot \nu =0\), by integration by parts, we have
and
Note that the minus signs appear because \(\nu \) on \(\Gamma _{-,r}^0\) and \(\Gamma _{-,r}^\varepsilon \) are defined to be pointing upwards, while \(\nu \) on \(\eta \) and \(\Sigma _r^\varepsilon \) are pointing away from \(\mathcal {D}_1^\varepsilon \). By (2.5), we have \(|D u_0(x)| \le C_1 e^{-\frac{C_2}{r}}\) in \(\overline{\Omega _{r}^0}\), and hence
for some positive \(\varepsilon \)-independent constants \(C_1\) and \(C_2\). By Theorem 2.5, we have
By (2.7), we have \(|D u_\varepsilon (x)| \le C (\varepsilon + |x'|^2)^{-1} \) in \({\Omega _{1/2}^0}\). Therefore,
Finally, (4.7) follows directly from (A.1)–(A.5). Proposition 4.2 is proved. \(\square \)
In the following, we verify (4.12).
Lemma A.1
(4.12) holds when \(p \ge (n+1)/2\).
Proof
We only give the proof for the case when \(n \ge 3\). The case \(n = 2\) follows similarly and is simpler. After a rotation of coordinates if necessary, we may assume that
First, we replace \(\delta (y)\) in the denominator with the quadratic polynomial \(\varepsilon + \sum _{i=1}^{n-1} \lambda _i y_i^2/2\). By (1.8), (1.9), and the fact that \(h_1,h_2\) are \(C^2\), we estimate
where h(r) is the modulus of continuity of \(D_{x'}^2 (h_1 - h_2)\), and hence \(h(r) \rightarrow 0\) as \(r \rightarrow 0\), and C is some positive constant independent of \(\varepsilon \) and r. Therefore, it suffices to show that for any \(r > 0\),
In the spherical coordinates, for \(y' \in \mathbb {R}^{n-1}\), we write
where \(s \in [0, \infty )\), \(\theta _1,\theta _2,\ldots ,\theta _{n-3}\in [0,\pi ]\) and \(\theta _{n-2}\in [0,2\pi )\). For convenience of notation, we denote \(\Sigma :=[0,\pi ]^{n-3}\times [0,2\pi )\). By this change of variables,
where
and
Note that
When \(p > (n+1)/2\), \(\Theta (\varepsilon ) = \varepsilon ^{\frac{2p-n-1}{2(p-1)}}\). By the change of variables \(t = \varepsilon ^{-1}s^2\), the right-hand side of (A.7) becomes
Since \((n-3)/2 - (p-1) = (n-2p-1)/2 < -1\), the integral converges as \(\varepsilon \rightarrow 0\). Therefore,
where B is the beta function. Recalling the identities
and plugging them into (A.8), we have proved (A.6) for the case when \(p > (n+1)/2\).
When \(p = (n+1)/2\), \(\Theta (\varepsilon ) = |\ln \varepsilon |^{-\frac{1}{p-1}}\). By the change of variables \(w = \varepsilon ^{-1/2}s\), the right-hand side of (A.7) becomes
By direct computations,
Therefore, by (A.9),
To estimate \(\textrm{II}\), we split the integral over \((0, \frac{r}{\varphi (\theta )\sqrt{\varepsilon }})\) into (0, 1) and \((1, \frac{r}{\varphi (\theta )\sqrt{\varepsilon }})\), and denote them by \(\textrm{II}_1\) and \(\textrm{II}_2\), respectively. It is easily seen that \(|\textrm{II}_1| \le C|\ln \varepsilon |^{-1}\). To estimate \(\textrm{II}_2\), we have
By the mean value theorem, there exists a \(\xi \in (w^2, 1+w^2)\), such that
Note that \((w^2, 1 + w^2) \subset (w^2, 2w^2)\) when \(w \ge 1\). Therefore,
which implies \(|\textrm{II}_2| \le C|\ln \varepsilon |^{-1}\). Hence, by (A.10) and the estimate \(|\textrm{II}_1| + |\textrm{II}_2| \le C|\ln \varepsilon |^{-1}\), we have proved (A.6) for the case when \(p = (n+1)/2\). \(\square \)
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Dong, H., Yang, Z. & Zhu, H. Asymptotics of the solution to the perfect conductivity problem with p-Laplacian. Math. Ann. (2024). https://doi.org/10.1007/s00208-024-02876-y
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DOI: https://doi.org/10.1007/s00208-024-02876-y