Abstract
This paper concerns harmonic analysis of the Ornstein–Uhlenbeck operator L on the Euclidean space. We examine the method of decomposing a spectral multiplier \(\phi (L)\) into three parts according to the notion of admissibility, which quantifies the doubling behaviour of the underlying Gaussian measure \(\gamma \). We prove that the above-mentioned admissible decomposition is bounded in \(L^p(\gamma )\) for \(1 < p \le 2\) in a certain sense involving the Gaussian conical square function. The proof relates admissibility with E. Nelson’s hypercontractivity theorem in a novel way.
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1 Introduction
1.1 General background
This article is a continuation of [8], regarding analysis of the Ornstein–Uhlenbeck operator
which on the Euclidean space \({\mathbb {R}}^n\) is associated with the Gaussian measure
In [8], a certain class of spectral multipliers \(\phi (L)\) was studied by means of anadmissible decomposition—an integral representation, which takes into account thenon-doubling behaviour of \(\gamma \). This representation allows us to express the multiplier as a sum of three parts (admissible, intermediate, and non-admissible):
where c is a constant and u arises from f. An \(L^1\)-estimate was then obtained in terms of an admissible conical square function Sf, namely,
but the third estimate with a logarithmic weight and a maximal function Mf is clearlyunsatisfactory. This shortcoming calls into question whether the admissibledecomposition is at all suitable for studying boundedness of spectral multipliers. On the other hand, such problems do not seem to appear in [14], from which the decomposition originates in connection with the Riesz transform \(\nabla L^{-1/2}\).
The role of this article is to justify the above-mentioned approach, and to serve as an intermediate step towards a fully satisfactory \(L^1\)-estimate. Indeed, we show here that for \(1 < p \le 2\) we have
Interestingly, the proof of the third estimate invokes the hypercontractivity theorem of Nelson [13], and relies on its subtle interplay with the concept of admissibility. The ultimate aim of this square function approach is to provide a metric theory of Gaussian Hardy spaces to complement the existing atomic theory [11].
1.2 Admissible conical square function
Recall that the admissibility function
quantifies the extent to which \(\gamma \) is doubling:
See [1, 10, 11] for more details.
The admissible conical square function is then defined by
where the diffusion semigroup
is given by the Mehler kernel
The origins of this Gaussian square function can be found in [9, 14]. The Ornstein–Uhlenbeck semigroup \((e^{-tL})_{t>0}\) is a prototypical example of a symmetric, contractive, and conservative diffusion semigroup in the sense of [16]. For more information, see the (old, but not obsolete) survey [15].
1.3 Class of spectral multipliers
We will consider spectral multipliers of the form
where \(\Phi : (0,\infty ) \rightarrow \mathbb {C}\) is twice continuously differentiable and satisfies
As explained in [8], these are a special kind of ‘Laplace transform type’ multipliers.
Moreover, we will refer to the following two extra conditions.
-
Condition D:
$$\begin{aligned} \int _1^\infty (|\Phi '(t)| + t|\Phi ''(t)|) \, dt < \infty . \end{aligned}$$ -
Condition P: There exists an integer N such that
$$\begin{aligned} |\Phi '(t)| + t|\Phi ''(t)| \lesssim t^N, \quad t\ge 1 . \end{aligned}$$
Notice, however, that the main result is already interesting for the prototypical imaginary powers \(\phi (L) = L^{i\tau }\), \(\tau \in \mathbb {R}\), with \(\Phi (t) = t^{-i\tau } / \Gamma (2 - i\tau )\) (or for their damped versions with \(\Phi (t) = t^{-i\tau } \chi (t)\), where \(\chi \) is a smooth cutoff with \(1_{(0,1]} \le \chi \le 1_{(0,2]}\)).
1.4 Admissible decomposition
The analysis is greatly simplified by switching to the discretized version of the admissibility function
and to the associated admissible region \(D = \{ (y,t)\in {\mathbb {R}}^n \times (0,\infty ) : 0< t < \widetilde{m}(y) \}\).
Let then \(\phi \) and \(\Phi \) be as in Sect. 1.3 and let f be a polynomial with \(\int f \, d\gamma = 0\). The special form of our spectral multipliers allows us to use the following integral representation with \(\delta , \delta ' > 0\) and \(\kappa \ge 1\):
where \(u(\cdot , t) = 1_D(\cdot , t) t^2L e^{-\delta t^2L}f\) and \(\widetilde{\Phi } (t) = \Phi ((\delta '+\delta )t)\). The role of the technical parameters \(\delta , \delta '\) and \(\kappa \) is more visible in [8] than in this paper.
1.5 Main result
The first part of Proposition 5 refines the previous analysis of \(\pi _3\) from [8], and shows that the maximal operator
can be disposed of, i.e. that
for multipliers satisfying Condition D. As a consequence, for all \(f\in L^1(\gamma )\) it then holds that
The second part of Proposition 5 (together with Propositions 2 and 4) leads to the main result of the article:
Theorem
Let \(1 < p \le 2\). For multipliers satisfying Condition P, there exist values of parameters \(\delta , \delta '\) and \(\kappa \) so that
Corollary
Let \(1 < p \le 2\). For spectral multipliers \(\phi \) of Sect. 1.3 satisfying Condition P we have
Such spectral multipliers are well known to be bounded on \(L^p(\gamma )\) for all \(1< p < \infty \), also in vastly more general settings [3, 4, 16]. The vertical square function that istypically used in their analysis seems, however, to be somewhat ill-suited for \(p=1\) and thecorresponding Hardy space theory. Developments of an abstract semigroup approach to Hardy spaces nevertheless exist, see [7, 12]. Recall also the relations between vertical and conical objects in [2, Proposition 2.1], showing how conical square functions dominate the vertical ones for \(p\le 2\). Moreover, it is curious to note that a local square function such as ours is sufficient for the analysis of an operator with a spectral gap (between the lowest two eigenvalues in \(\sigma (L) = \{ 0,1,2,\ldots \}\)). The intriguing question whether \(\Vert Sf \Vert _p \lesssim \Vert f \Vert _p\) for \(p > 1\) is a topic of ongoing research.
2 Proof
Throughout the proof we assume that f is a polynomial with \(\int f \, d\gamma = 0\), and therefore a finite linear combination of Hermite polynomials—the eigenfunctions of L. The three parts of the admissible decomposition (2) are studied separately in the following three subsections.
2.1 Admissible part
Let us first recall the definition of tent spaces (see [1, 10]).
Definition
Let \(1\le p \le 2\). The Gaussian tent space \({\mathfrak {t}}^p(\gamma )\) is defined to consist of functions u on the admissible region \(D = \{ (y,t)\in {\mathbb {R}}^n \times (0,\infty ) : 0< t < \widetilde{m}(y) \}\) for which
Here \(\Gamma (x) = \{ (y,t)\in D : |y-x| < t \}\) is the admissible cone at \(x\in {\mathbb {R}}^n\).
Consider the admissible part
for functions u in a Gaussian tent space.
Curiously, due to the non-uniformity of the admissibility function, the case \(p=2\) is not quite as straightforward as one might expect.
Proposition 1
For \(\kappa \ge 1\) and \(0 < \delta ' \le 1\) we have \(\Vert \pi _1 u \Vert _2 \lesssim \Vert u \Vert _{{\mathfrak {t}}^2(\gamma )}\).
Proof
The proof does not rely on admissibility in the sense that \(\widetilde{m}(x)/\kappa \) can be replaced by any function with values in (0, 1]. Hence we may abbreviate \(\widetilde{m}(x) / \kappa = m(x)\).
Write \(\chi _t(x) = 1_{(0,m(x))}(t)\). Given a \(g\in L^2(\gamma )\), we argue by duality:
and so it suffices to show that
Now the uniform \(L^2\)-boundedness of \((t^2L)^{1/2} e^{-\frac{\delta '}{2}t^2L}\) guarantees that
where the last step relies on the self-adjointness and non-negativity of \((t^2L)^{1/2}e^{-\delta ' t^2L}\). Expressing \(t^2Le^{-\delta ' t^2L}\) in terms of the kernel \((2\delta ')^{-1}t\partial _t M_{\delta ' t^2}(x,y)\) we therefore see that
where in the last step we made use of the maximal inequality. This finishes the proof. \(\square \)
Proposition 2
Let \(1 < p \le 2\). For \(\kappa \ge 1\) and sufficiently small \(\delta ' > 0\), we have \(\Vert \pi _1 u \Vert _p\lesssim \Vert u \Vert _{{\mathfrak {t}}^p(\gamma )}\). Moreover, for \(0 < \delta \le 1\), the function \(u(\cdot , t) = 1_D(\cdot , t) t^2L e^{-\delta t^2L} f\) satisfies \(\Vert u \Vert _{{\mathfrak {t}}^p(\gamma )} \lesssim \Vert Sf \Vert _p\).
Proof
The first part of the statement follows by interpolation of Gaussian tent spaces [1, Theorem 3.3 and Corollary 3.5]. Indeed,
Therefore, \(\pi _1\) is also bounded \({\mathfrak {t}}^p(\gamma ) \rightarrow L^p(\gamma )\), i.e. \(\Vert \pi _1 u \Vert _p \lesssim \Vert u \Vert _{{\mathfrak {t}}^p(\gamma )}\).
The second part of the statement follows by a straightforward modification of thecorresponding argument in [8, Proposition 2]. Indeed, by change of aperture on \({\mathfrak {t}}^p(\gamma )\) (see [1, Theorem 3.3]) we obtain
where \(D' = \{ (y,s)\in \mathbb {R}^n \times (0,\infty ) : s < \sqrt{\delta } \widetilde{m}(y) \}\). The desired estimate \(\Vert u \Vert _{{\mathfrak {t}}^p(\gamma )} \lesssim \Vert Sf \Vert _p\) now follows from the pointwise inequality (see [8, Proposition 2])
\(\square \)
2.2 Intermediate part
Let us begin by presenting two \(L^p\)-estimates for the operators \(tLe^{-tL}\).
Lemma 3
The family \((tLe^{-tL})_{t>0}\) is uniformly bounded on \(L^p(\gamma )\) for all \(p > 1\), that is,
Moreover, for \(1\le p \le 2\) we have
whenever \(E,E'\subset {\mathbb {R}}^n\).
Proof
The boundedness of \(tLe^{-tL}\) on \(L^p(\gamma )\) (when \(p>1\)) is the content of [6, Theorem 5.41], and the uniformity in \(t>0\) follows by careful inspection of the proof.
The off-diagonal estimate for \(1_{E'}tLe^{-tL}1_E\) is an immediate consequence of [8, Lemma 3] and follows by Hölder’s inequality. \(\square \)
Let us then turn to
Proposition 4
Let \(1 < p \le 2\). For \(\kappa \ge 4\) and sufficiently small \(\delta , \delta ' > 0\) we have \(\Vert \pi _2 f \Vert _p\lesssim \Vert f \Vert _p\).
Proof
As in [8, Proposition 5] we have
where \(C_{k+l-1} := B(0,2^{k+l-1}){\setminus } B(0,2^{k+l-2})\).
The distance between \(B(0,2^{k-2})\) and \(C_{k+l-1}\) is at least \(2^{k+l-3}\). We make use of Lemma 3 to see that, for \(2^{-k-1} < t \le 2^{-k}\) we have
when \(\delta ' < 4^{-3}\).
The right-hand side of (3) is therefore dominated by
\(\square \)
Notice that for \(p > 1\) the proof was simpler than for \(p = 1\) because of the uniform \(L^p\)-boundedness of \(tL e^{-tL}\).
2.3 Non-admissible part
We begin by recalling the following key result. See [6, Chapter V] and [5] for more references.
Hypercontractivity Theorem
(Nelson [13]) Let \(1< p \le q < \infty \). Then
Let us remark, that most proofs of this result use a different scaling/normalization of the Gaussian measure. The easiest way to convince oneself of the validity of this version is probably by the equivalence between hypercontractivity and a logarithmic Sobolev inequality (see [5]). Also note that our L is ‘one half’ of a usual Dirichlet form operator.
The following reformulation of the hypercontractivity theorem will be convenient for us:
Let \(p > 1\). Then for any \(t>0\),
Finally, let us consider
Proposition 5
For sufficiently small \(\delta , \delta ' > 0\) and large enough \(\kappa \) we have:
-
If \(\Phi \) satisfies Condition D, then \(\Vert \pi _3 f \Vert _1 \lesssim \Vert (1 + \log _+ |\cdot |) \, f \Vert _1\).
-
If \(\Phi \) satisfies Condition P, then \(\Vert \pi _3 f \Vert _p \lesssim \Vert f \Vert _p\) for \(1 < p \le 2\).
Proof
We will consider the two statements side by side.
Part I: Recall the pointwise estimate from [8, Proposition 7]:
We will estimate the \(L^p\)-norms of the three terms on the right-hand side separately.
For \(1\le p \le 2\) and \(\kappa \) large enough we have
by an immediate generalization of [8, Lemma 6]. Together with the general assumption (1) on \(\Phi \), this takes care of the first two terms of (5).
The range \(\int _1^\infty dt\) in the third term in (5) is dealt with Conditions D and P separately. For \(p=1\), Condition D guarantees that
For \(1 < p \le 2\) we may use interpolation to see that \(\Vert e^{-tL} f \Vert _p \lesssim e^{-\theta _p t} \Vert f \Vert _p\) (recall that f is a polynomial with zero mean). Indeed, denoting by \(E_0\) the spectral projection onto the kernel of L, we have \(\Vert e^{-tL} (I-E_0) \Vert _{2\rightarrow 2} = e^{-t}\) and \(\Vert e^{-tL}(I-E_0) \Vert _{1\rightarrow 1} \le 1\). Hence we obtain the claim with \(\theta _p = 2 - 2/p\). Now Condition P implies that
It remains to consider the range \(\int _{\widetilde{m}(\cdot )^2/\kappa ^2}^1 dt\) in the third term in (5). By the assumption (1), \(\sup _{0< t \le 1} (t|\Phi '(t)| + t^2|\Phi ''(t)|) < \infty \), and so for \(1\le p \le 2\) we have
which is analyzed further below.
Part II (setup): We will then examine the remaining integral over annuli andseparate the off-diagonal and on-diagonal parts. More precisely, let us write \(C_0 = B(0,1)\) and \(C_k = B(0,2^k){\setminus } B(0,2^{k-1})\) for \(k\ge 1\), and let \(C_0^* = B(0,2)\), \(C_1^* = B(0,4)\), and \(C_k^* = B(0,2^{k+1}){\setminus } B(0,2^{k-2})\) for \(k\ge 2\). Then, for \(1\le p \le 2\), we have
Part II (off-diagonal terms): Let \(1\le p \le 2\) for the time being. We choose \(\delta , \delta ' > 0\) such that \(8(\delta ' + \delta ) \le 4^{-3}\) and take care of the first two annuli with \(k = 0,1\) simply by
For the general case with \(k \ge 2\) we write
Observing that \(d(C_k , B(0,2^{k-2})) = 2^{k-2}\), we use Lemma 3 to obtain for \(t \le 1\) the estimate
Furthermore, since \(d(C_k , C_{k+l}) = 2^{k+l-2}\), Lemma 3 implies that for \(t \le 1\) we have
We are now ready to estimate the off-diagonal terms for \(k\ge 2\):
so that the sum of the off-diagonal terms in (6) is under control
Part II (on-diagonal terms): We then consider the on-diagonal terms in (6).
Let us begin with \(p=1\) and estimate for \(k\ge 0\) simply as follows:
For the sum of the on-diagonal terms we then obtain
as required.
Let then \(p > 1\) and choose \(\kappa \) to be a power of 4 and write \(N(k) = k-1+ 2\log _4 \kappa \) so that \(4^{-k+N(k)+1}/\kappa ^2 = 1\) for each \(k\ge 0\). We start by partitioning the time integral as follows:
For each \(k,j\ge 0\) let us denote by q(k, j) the hypercontractive exponent (cf. (4)) from time \((\delta ' + \delta ) 4^{-k+j} / \kappa ^2\), i.e. \(q(k,j) = 1 + (p-1)e^{2(\delta ' + \delta ) 4^{-k+j}/\kappa ^2}\). Then, using Hölder’s inequality, we have for \(t \ge 4^{-k+j}/\kappa ^2\),
where the decay factor from the last inequality will be justified next. Firstly,
Secondly,
Hence,
as was claimed.
Returning to the sum of the on-diagonal terms in (7),
This finishes the proof. \(\square \)
Remark
As is clear from the proof above, if one could show that there exists an \(\alpha > 1\) such that for all \(k\ge 0\) and all \(0\le j \le N(k)\),
then the desired inequality \(\Vert \pi _3 f \Vert _1 \lesssim \Vert f \Vert _1\) would follow (for multipliers satisfyingCondition D).
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Acknowledgements
The author would like to thank the organizers of the Probabilistic Aspects of Harmonic Analysis conference in Bedlewo, Poland, in May 2016. The key steps of the proof were completed there in the inspiring environment of the Banach Center.
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Kemppainen, M. Admissible decomposition for spectral multipliers on Gaussian \(L^p\) . Math. Z. 289, 983–994 (2018). https://doi.org/10.1007/s00209-017-1984-y
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DOI: https://doi.org/10.1007/s00209-017-1984-y