Abstract
In this paper, for a certain range of parameters, we prove that there exist symbols in the Hörmander class \(S_{1,0}^{0}\) which do not define bounded operators on \(M\big ({\dot{K}}_{q}^{\alpha ,p}{F_{\beta }^{s}}\big )\). To do these, we need the characterization of Herz–Besov spaces by ball means of differences and some properties of pointwise multipliers for Herz–Triebel–Lizorkin spaces.
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Appendix
Appendix
Here, we present the proof of Theorem 2.9 and Proposition 4.4.
Proof of Theorem 2.9
We split it into three steps.
Step 1. Let \(f\in {\dot{K}}_{q}^{\alpha ,p}B_{\beta }^{s}\). Since \(s>0\), we see that
Step 2. We put
After a change of variable \(t=2^{-y}\), we get
Then
Let \(\left\{ \varphi _{j}\right\} _{j}\) be a smooth dyadic resolution of unity. Obviously we need to estimate
and
in \(\ell ^{\beta }\)-norm. Using the same arguments of [32, 2.5.10] we get
if \(0\leqslant j\leqslant k\), \(x\in \mathbb {R}^{n}\) and \(\left| h\right| \leqslant 2^{-k}\), with \(c>0\) independent of j, k, h and x, which yields that
if \(0\leqslant j\leqslant k,k\in \mathbb {N}_{0}\) and \(x\in \mathbb {R}^{n}\). Since \(s<M\) , (5.1) in \(\ell ^{\beta }\)-norm does not exceed
by Theorem 2.5. Let \(j>k\). Recalling the definition of \( d_{2^{-k}}^{M}(\Lambda _{j}f)\) and observe that
if \(j,k\in \mathbb {N}_{0},i\in \{0,\ldots ,M\},\left| h\right| \leqslant 2^{-k}\) and \(x\in \mathbb {R}^{n}\). Therefore,
for any \(j>k\) and \(x\in \mathbb {R}^{n}\). Hence
Using Lemma 3.2, we obtain that (5.2) in \(\ell ^{\beta } \)-norm can be estimated from above by
where we used Lemma 3.4.
Step 3. Let \(\Psi \) be a function in \({\mathcal {S}}(\mathbb {R}^{n})\) satisfying \(\Psi (x)=1\) for \(|x|\leqslant 1\) and \(\Psi (x)=0\) for \( |x|\geqslant \frac{3}{2}\), in addition radialsymmetric. We make use of an observation made by Nikol’skij [26] (see also [29]). We put
The function \(\psi \) satisfies \(\psi \left( x\right) =1\) for \(\left| x\right| \leqslant 1/M\) and \(\psi \left( x\right) =0\) for \(\left| x\right| \geqslant 3/2\). Then, taking \(\varphi _{0}\left( x\right) =\psi \left( x\right) ,\varphi _{1}\left( x\right) =\psi \left( x/2\right) -\psi \left( x\right) \) and \(\varphi _{j}\left( x\right) =\varphi _{1}\left( 2^{-j+1}x\right) \) for \(j=2,3,\ldots \), we obtain that \(\left\{ \varphi _{j}\right\} \) is a smooth dyadic resolution of unity. This yields that
is an norm equivalent in \({\dot{K}}_{q}^{\alpha ,p}{B_{\beta }^{s}}\). Let us prove that the last expression is bounded by
Obviously from (2.2)
Moreover, it holds for \(x\in \mathbb {R}^{n}\) and \(j=1,2,\ldots \)
with \({\widetilde{\Psi }}\left( \cdot \right) ={\mathcal {F}}^{-1}\Psi \left( \cdot \right) -2^{-n}{\mathcal {F}}^{-1}\Psi \left( \cdot /2\right) \). Now, for \(j\in \mathbb {N}\) we write
Obviously we need only to estimate the second term. We have
where \({\overline{C}}_{i}=\{x\in \mathbb {R}^{n}:2^{i}<\left| x\right| \leqslant 2^{i+1}\}\), \(i\in \mathbb {N}_{0}\) and \(N>0\) is at our disposal, and we have used the properties of the function \({\widetilde{\Psi }}\),
for any \(y\in \mathbb {R}^{n}\) and any \(N>n\). Now the right-hand side of (5.5) in \(\ell _{\beta }^{s}({\dot{K}}_{q}^{\alpha ,p})\)-norm is bounded by
where
The sum (5.6) can be rewritten as
Clearly
where \(c>0\) is independent of k. Now let us estimate \(S_{k}^{_{2}}\). We obtain
Taking N large enough such that \(N>s+n\), we estimate the right-hand side of (5.5) in \(\ell _{\beta }^{s}({\dot{K}}_{q}^{\alpha ,p})\) -norm by
This finishes the proof. \(\square \)
Proof of Proposition 4.4
The proof is based on [1]. Observe that \(g_{\tau ,\alpha }\in {\dot{K}}_{q}^{\alpha ,p}\), because of \(\tau +\frac{n}{q}>0\). We need to prove that
since
We will present the proof into several steps.
Step 1. \(\alpha =0\). Since \(\tau >-\frac{n}{q}\), for any \( 1<p\leqslant q\) we have \(\tau >-\frac{n}{p}\). From Theorem 2.6 we obtain
if \(p\leqslant q\). Now if \(p>q\) we have
Step 2. \(-\frac{n}{q}<\alpha <0\). Can be covered by the similar arguments used in Step 1.
Step 3. \(0<\alpha <\tau +\frac{n}{q}\).
Substep 3.1. We prove that \(g\in {\dot{K}}_{q}^{\alpha ,p}B{ _{\infty }^{\tau +\frac{n}{q}}}\) if \(0<\tau +\frac{n}{q}\leqslant 1\).
Substep 3.1.1. We consider the case of \(0<\tau +\frac{n}{q }<1\). Clearly,
We estimate each term on the right separately. First notice that
\(\bullet \) Estimation of \(H_{1}\). Obviously \(T_{2,k}(h)=0\) if \( 2^{k}<2\left| h\right| ,h\in \mathbb {R}^{n}\ \)and \(k\in \mathbb {Z}\). Therefore, we need only to estimate \(T_{1,k}(h)\). Observe that
and
which yields
since \(\alpha <\tau +\frac{n}{q}\) where \(c>0\) is independent of k and h. Therefore
because of \(\alpha >0\).
\(\bullet \) Estimation of \(H_{2}\). As before one finds that
since again \(\alpha <\tau +\frac{n}{q}\) where \(c>0\) is independent of k and h. By the mean value theorem;
we obtain
This yields that
since \(\tau +\frac{n}{q}<1\). Therefore,
Substep 3.1.2. We consider the case of \(\tau +\frac{n}{q}=1\). We have,
Observe that
\(\bullet \) Estimation of \(I_{1}\). Obviously \(V_{2,k}(h)=0\) if \( 2^{k}<2\left| h\right| ,h\in \mathbb {R}^{n},k\in \mathbb {Z}\). Therefore, we need only to estimate \(V_{1,k}(h)\). We have
and
which yields
since \(\alpha <\tau +\frac{n}{q}=1\) where \(c>0\) is independent of k and h . Therefore
because of \(\alpha >0\).
\(\bullet \) Estimation of \(I_{2}\). As before one finds
where \(c>0\) is independent of k and h. Again by the mean value theorem;
we obtain
This yields that
Therefore,
Step 4. \(\tau +\frac{n}{q}>1\). Using the same arguments of [39, Theorem 4.5]
is an equivalent quasi-norms on \({\dot{K}}_{q}^{\alpha ,p}{B_{\infty }^{\tau + \frac{n}{q}}}\). Let us prove by induction that \(g^{(\lambda )}\in {\dot{K}} _{q}^{\alpha ,p}{B_{\infty }^{\tau +\frac{n}{q}-m}}\) for any \(|\lambda |\leqslant m\) with \(m=-[-\tau -\frac{n}{q}]-1\). The case \(m=0\) is covered by the above steps. Observe that
and \(g^{(\lambda )}\) is a linear combination of
where \(\Theta \in C^{\infty }\left( \mathbb {R}^{n}\backslash \{0\}\right) \) is homogeneous of degree 0 and \(\omega \in {\mathcal {D}}(\mathbb {R}^{n})\). Since \(j<\tau +\frac{n}{q}\), it follows that \(g_{j}\in {\dot{K}}_{q}^{\alpha ,p}\). If \(j\ne 0\), then by induction
Now if \(j=0\), then by the fact that \(\tau +\frac{n}{q}>m\geqslant 1\),
Since \({\dot{W}}_{q,1}^{\alpha ,p}={\dot{K}}_{q}^{\alpha ,p}F_{2}^{1}\), see [24], we obtain
The proof of Proposition 4.4 is complete. \(\square \)
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Djeriou, A., Drihem, D. On the Continuity of Pseudo-Differential Operators on Multiplier Spaces Associated to Herz-type Triebel–Lizorkin Spaces. Mediterr. J. Math. 16, 153 (2019). https://doi.org/10.1007/s00009-019-1418-7
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DOI: https://doi.org/10.1007/s00009-019-1418-7