Strichartz estimates for the Schrödinger equation with a measure-valued potential
By M. Burak Erdoğan, Michael Goldberg, and William R. Green
Abstract
We prove Strichartz estimates for the Schrödinger equation in $\mathbb{R}^n$,$n\geq 3$, with a Hamiltonian $H = -\Delta + \mu$. The perturbation $\mu$ is a compactly supported measure in $\mathbb{R}^n$ with dimension $\alpha > n-(1+\frac{1}{n-1})$. The main intermediate step is a local decay estimate in $L^2(\mu )$ for both the free and perturbed Schrödinger evolution.
1. Introduction
The dispersive properties of the free Schrödinger semigroup $e^{it\Delta }$ are described in many ways, with one of the most versatile estimates being the family of Strichartz inequalities
over the range $2 \leq p,q \leq \infty$,$\frac{2}{p} + \frac{n}{q} = \frac{n}{2}$, except for the endpoint $(p,q) = (2,\infty )$. There is a substantial body of literature devoted to establishing Strichartz inequalities and other dispersive bounds for the linear Schrödinger evolution of perturbed operators $H = -\Delta + V(x)$.Reference 8Reference 15Reference 21 prove Strichartz inequalities for the free evolution. The latter two of these as well as Reference 19 create a framework for extending them to perturbed Hamiltonians so long as the Schrödinger semigroup has suitable $L^1\to L^\infty$ dispersive bounds or $L^2(\mathbb{R}^n\times \mathbb{R})$ smoothing. This strategy has been used to establish Strichartz estimates for the Schrödinger evolution for electric Reference 13, magnetic Reference 6 and time-periodic Reference 9 perturbations. Most commonly $V(x)$ is assumed to exhibit pointwise polynomial decay or satisfying an integrability criterion such as belonging to a space $L^r_{loc}(\mathbb{R}^n)$ for some $r \geq \frac{n}{2}$. Our goal in this paper is to show that Strichartz inequalities hold for a class of short-range potentials $V(x)$ that include measures $\mu (dx)$ as admissible local singularities.
Measure-valued potentials are often considered in one dimension; the operator $-\frac{d^2}{dx^2} + c\delta _0$ is often the subject of exercises in an introductory quantum mechanics course. In higher dimensions there are several plausible generalizations of this example. The three-dimensional Schrödinger operator $H = -\Delta + \sum c_j \delta (x_j)$ is studied in Reference 3 and Reference 4, and in two dimensions in Reference 2. Here, the singularity of the potential imposes boundary conditions at each point $x_j$ for functions belonging to the domain of $H$. As an eventual consequence, linear dispersive and Strichartz inequalities hold only on a subset of the range described above.
The potentials considered in this paper are less singular than a delta-function in $\mathbb{R}^n$, but still not absolutely continuous with respect to Lebesgue measure. The surface measure of a compact hypersurface $\Sigma \subset \mathbb{R}^n$ is a canonical example of an admissible potential we consider. More generally we work with compactly supported fractal measures (on $\mathbb{R}^n$) of a sufficiently high dimension. The exact threshold will be determined in context. Arguments regarding the self-adjointness of $H$ require a dimension greater than $n-2$ so that multiplication by $\mu$ remains compact relative to the Laplacian. We are forced to increase the threshold dimension to $n - (1+ \frac{1}{n-1})$ in the proof of the local decay and Strichartz estimates. Under these conditions, and a modest assumption about the spectral properties of $H$, we prove that the entire family of Strichartz inequalities Equation 1.1 is preserved with the possible exception of the $(p,q)=(2, \frac{2n}{n-2})$ endpoint.
With $B(x,r)$ a ball of radius $r$ centered at $x\in \mathbb{R}^n$, we say that a compactly supported signed measure $\mu$ is $\alpha$-dimensional if it satisfies
$$\begin{equation} |\mu |(B(x,r)) \leq C_\mu r^{\alpha } \ \ \text{for all } r>0 \text{ and } x \in \mathbb{R}^n. \cssId{texmlid15}{\tag{1.2}} \end{equation}$$
Nontrivial $\alpha$-dimensional measures exist for any $\alpha \in [0, n]$.
The first obstruction to Strichartz estimates with a Hamiltonian $H = -\Delta + V$ is the possible existence of bound states, functions $\psi \in L^2(\mathbb{R}^n)$ that solve $H\psi = E \psi$ for some real number $E$. Each bound state gives rise to a solution of the Schrödinger equation $e^{itH}\psi (x) =e^{itE}\psi (x)$, which satisfies Equation 1.1 only for $(p,q) = (\infty , 2)$ and no other choice of exponents.
Our main result asserts that the perturbed evolution $e^{itH}$ satisfies Strichartz estimates once all bound states of $H$ are projected away. We impose additional spectral assumptions that all eigenvalues of $H$ are strictly negative, and that there is no resonance at zero. In this paper we say a resonance occurs at $\lambda$ when the equation
has nontrivial solutions belonging to the Sobolev space $\dot{H}^1(\mathbb{R}^n)$ but not to $L^2$ itself.
Thanks to the compact support of $\mu$, one can easily show that resonances are impossible at $\lambda < 0$, and can only occur at $\lambda = 0$ in dimensions 3 and 4. We show in Section 3 that resonances do not occur when $\lambda > 0$. Eigenvalues at zero are possible provided the negative part of the potential is large enough. Positive eigenvalues are known to be absent for a wide class of potentials (see Reference 16) covering some (but not all) of the measures considered here; see Remark 3.2.
To state our results, we define the following $L^p$ spaces. For $\mu$ a signed measure on $\mathbb{R}^n$, we define
for $1\leq p< \infty$. With the natural, minor modification one can define $L^\infty (\mu )$. It is worthwhile to note that multiplication by $\mu$ is an isometry from $L^p(\mu )$ to $L^{p'}(\mu )^*$ with $p'$ the Hölder conjugate of $p$ for any $1\leq p\leq \infty$. This can be seen easily by using the natural duality pairing. Throughout the paper we will take particular advantage of the fact that multiplication by $\mu$ maps $L^2(\mu )$ to its dual space. Finally, let $P_{ac}$ denotes projection onto the continuous spectrum of $-\Delta + \mu$.
The second author considered $L^1 \to L^\infty$ dispersive estimates in $\mathbb{R}^3$ (under the same set of assumptions when $n=3$, including $\alpha > \frac{3}{2}$) in Reference 10. Strichartz inequalities in this case follow as a direct consequence by Reference 15. The results presented here in $\mathbb{R}^n$,$n \geq 4$, are new and rely in part on recent advances in Fourier restriction problems such as Reference 5Reference 17. In particular the improved decay of spherical Fourier means allows us to capture the physically relevant $\alpha = n-1$ case where the potential might be supported on a compact hypersurface in higher dimensions. It is known for dimensions $n>3$ that $L^1\to L^\infty$ dispersive estimates need not hold even for compactly supported potentials $V$ if $V$ is not sufficiently differentiable; see Reference 7Reference 12. Whereas the smoothness is not required for Strichartz estimates to hold in higher dimensions. Our argument works in dimensions $n\geq 3$; technical issues in dimension $n=2$ (for example with the use of $\dot{H}^1(\mathbb{R}^n))$ would require different methods.
$\alpha$-Dimensional measures also satisfy a strong Kato-type property that for any $\gamma < \alpha$,
Furthermore, since $\mu$ has compact support, the integral over the entire space $x \in \mathbb{R}^n$ is bounded uniformly in $y$. These integral bounds will be proved as Lemma 2.2. The choice $\gamma = n-2$ is significant due to its connection with the Green’s function of the Laplacian in $\mathbb{R}^n$ when $n\geq 3$.
We also characterize potentials in terms of the global Kato norm, defined on signed measures in $\mathbb{R}^n$ by the quantity
One can see that every element with finite global Kato norm is an $(n-2)$-dimensional measure with $C_\mu \leq \|\mu \|_{\mathcal{K}}$, by comparing $|x-y|^{2-n}$ to the characteristic function of a ball. The converse is false; however the Kato class contains all compactly supported measures of dimension $\alpha > n-2$. We examine this relationship in Lemma 2.2. We follow the naming convention in Rodnianski-Schlag Reference 19 where the global Kato norm is applied to dispersive estimates in $\mathbb{R}^3$, as opposed to the local norms considered in Schechter Reference 20.
There is a now well-known strategy to obtain the Strichartz estimates Equation 1.6. One uses the space-time $L^2$ estimates Equation 1.4 and Equation 1.5 and the argument of Rodnianski-Schlag Reference 19. There is a minor modification to the Rodnianski-Schlag framework in that instead of factorizing the operator corresponding to multiplication by $\mu$, we instead apply it directly as a bounded map from $L^2_tL^2(\mu )$ to its dual space.
The resolvent operators $(-\Delta -\lambda )^{-1}$ and $(-\Delta +\mu -\lambda )^{-1}$ are well defined for $\lambda$ in the resolvent sets. We define the limiting resolvent operators
Following Kato’s derivation Reference 14, $L^2$ estimates such as Equation 1.4 and Equation 1.5 are valid precisely if there are uniform bounds of the resolvent operators. We prove the following mapping bounds for the resolvents $R_0^\pm (\lambda )$ and $R_\mu ^\pm (\lambda )$.
Due to the different challenges of establishing these bounds when the spectral parameter is close to $\lambda =0$ (small energy) or bounded away from zero (large energy), we require different tools in each regime. We bound the low energy contribution in Section 3 in Lemma 3.1, while the large energy is controlled in Section 4. Once the resolvent bounds are established at all energies, we assemble the results to prove Theorem 1.1.
2. Self-adjointness and compactness
For any perturbation $V(x)$ which is not a bounded function of $x$ there are well known difficulties identifying the domain of $-\Delta + V$ and its adjoint operator. The main goal of this section is to prove Proposition 2.1. Along the way, we will prove some compactness results that will be useful for describing the spectral measure of $-\Delta + \mu$.
The first step is to check that $\mu$ satisfies both a local and global “Kato condition.”
By choosing $\gamma = n-2$, it follows that $\|\mu \|_\mathcal{K}< \infty$.
Given a point $z \in \mathbb{R}^n$, define the translation operator $\tau _z f(x) \coloneq f(x-z)$. Translation operators are not bounded on $L^2(\mu )$ in general, but they behave quite well when restricted to the subspace $\dot{H}^1$. Let $j: \dot{H}^1(\mathbb{R}^n) \to L^2(\mu )$ be the natural inclusion operator.
3. Low energy estimates
At this point we establish a uniform bound on the low energy perturbed resolvent as an operator on $L^2(\mu )$. Specifically, we show
4. High energy estimates
The estimates for $R_0^+(\lambda ^2)\mu$ in the preceding sections are adequate for finite intervals of $\lambda$; however the sharp weighted $L^2(\mathbb{R}^n)$ resolvent bound from Reference 1 only implies that
At high energy one needs to take advantage of the fact that for $f \in L^2(\mu )$,$\mu f$ is not a generic element of $\dot{H}^{-1}(\mathbb{R}^n)$. Our main observation at high energy is that the free resolvent in fact has asymptotic decay as an operator on $L^2(\mu )$.
There are close connections between the free resolvent $R_0^+(\lambda ^2)$ and the restriction of Fourier transforms to the sphere $\lambda \mathbb{S}^2$. We make use of a Fourier restriction estimate proved by Du and Zhang Reference 5. Theorem 2.3 of Reference 5 asserts that for a function $f \in L^2(\mathbb{R}^{n-1})$ with Fourier support in the unit ball, and a measure $\mu _R = R^{\alpha } \mu (\,\cdot \,/R)$,
for sufficiently large $R$. The Schrödinger evolution $e^{it\Delta }f$ is the inverse Fourier transform (in $\mathbb{R}^n$) of the measure $\hat{f}\in L^2(\mathbb{R}^{n-1})$ lifted onto the paraboloid $\Sigma = \{\xi _n = |\xi _1|^2 + \cdots + |\xi |_{n-1}^2\}$. The theorem is then equivalent to the statement
for functions $g \in L^2(\Sigma \cap B(0,1))$. The use of forward versus inverse Fourier transform does not affect the inequality.
It is well known that the bounded subset of the paraboloid $\Sigma$ can be replaced with any other uniformly convex bounded smooth surface. In this case we wish to apply the result to the unit sphere instead. For any $g \in L^2(S^{n-1})$,
Now we reverse some of the scaling relations. Given $f \in L^2(\mu )$, let $f_R(x) = R^{-\frac{\alpha }{2}}f(x/R)$ so that $\|f_R\|_{L^2(\mu _R)} = \|f\|_{L^2(\mu )}$. Then $\widehat{\mu _Rf_R}(\xi ) = R^{\frac{\alpha }{2}} \widehat{\mu f}(R\xi )$. It follows that
Thanks to the compact support of $\mu$, the $L^2(\mu )$ norm of $(1+ |x|)f$ is comparable to that of $f$. That allows for control of the derivatives of $\widehat{\mu f}$ with the same restriction bound as in Equation 4.2. In particular we can bound the outward normal gradient of $\widehat{\mu f}$ as
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