We may recall here that the Landau equation reads as the evolution equation of the density of particles
where $Q_L$ is the so-called Landau collision operator
here, $a(y)$ is a symmetric nonnegative matrix depending on a parameter $y\in R^3 $ ,
and
The original Landau collision operator describing collisions among charged particles interacting with Coulombic force. As in the Boltzmann equation, it is well-known that Maxwellians are steady states to the Landau equation $\mu(y)=e^{-\frac{|y|^2}{2}}$ and we linearize the Landau equation around $\mu$ by posing $f=\mu+\mu^{\frac{1}{2}}u$ the perturbation $u$ satisfies the equation
We consider the Landau-type operator with external potential
In the linear homogeneous case, Fokker-Planck equations, Landau equations and Boltzmann equations equations have then a parabolic behavior, and the study of the local smoothing properties in the velocity variable is rather direct. In the non-homogeneous case, the regularization in space variable is not so easy, but occurs anyway thanks to the so-called hypoelliptic structure of the equation. In this article, we are interested in global estimates of the following Landau operator
where $D_x=-i \partial_x$ , $D_y=-i \partial_y$ , and $x\in\mathbb R^3$ is the space variable and $y\in\mathbb R^3$ is the velocity variable, and $X\cdot Y$ stands for the standard dot-product on $\mathbb R^3$ . The real-valued function $V(x)$ of space variable $x$ stands for the macroscopic force, $M(y)$ is a metric and the functions $a(y)$ , $b(y)$ and $p(y)$ of the variable $y$ in the diffusion are smooth and real-valued with the properties subsequently listed below.
(1) There exists a constant $c>0$ such that
with $\gamma\in[0, 1]$ and $\left\langle y \right\rangle =\left( 1+|y|^2 \right)^{1/2}$ .
(2) For any $\alpha\in\mathbb Z_+^3$ , there exists a constant $C_\alpha$ such that
(3) $M(y)$ is a positive definite matrix with
here we can substitute $D_y\cdot F(y)D_y$ for $D_y\cdot M(y)D_y$ with $F(y)\gtrsim \left\langle y \right\rangle ^{\gamma}$ . It is sometimes convenient to rewrite the operator as the form
where the matrix $B(y)$ is given by
and $\left( B(y)D_{y} \right)^*=D_y B(y)^T$ with $B^T$ the transpose of $B$ , is the formal adjoint of $B(y)D_{y}$ . By (1.2) and (1.3), one has, for any $y, \eta\in \mathbb R^3$ and any $\alpha\in\mathbb Z_+^3$ ,
Denoting by $(\xi, \eta)$ the dual variables of $(x, y)$ , we notice that the diffusion only occurs in the variables $(y, \eta)$ , but not in the other directions; and that the cross product term $y\wedge D_y$ improves this diffusion in specific directions of the phase space. In [3], the authors gave a estimate of the main term to the operator $\mathcal{L}$ . In this work, we aim at dealing with the low order terms to linear Landau-type operators and giving a similar results. Our main results can be stated as follows.
Theorem 1.1 Let $V\in C^2(\mathbb R^3;~\mathbb R)$ satisfy that
then there exists a constant $C$ such that for any $u\in C_0^\infty(\mathbb R^6)$ , one has
Estimates of the type given in Theorem 1.1 can be analyzed through different point of views. At first they give at least local regularity estimates in the velocity direction, according to the term $|D_y|^2$ appearing in (1.9). Now one of the goal of this article was to give global estimates in order to identify the good functional spaces associated to the problems.
The second main feature of this result is to reflect the regularizing effect in space variable $x$ , thanks to the hypoelliptic structure, which leads to terms involving e.g. $|D_x|^{2/3}$ . Recall that the exponent $2/3$ here is optimal.
Now similarly to the case of elliptic directions, it may be interesting to get global weighted estimates in space direction. In [7, 9], the authors studied the Fokker-Planck case, in particular with a potential. In this direction, the work [4] also gave a first subelliptic global (optimal) estimate, concerning the Landau operator in the case when there is no potential; the main feature of that work was to show that subellipticity in space direction occured with anisotropic weights of type $ \left\langle y \right\rangle ^{\gamma} y \wedge D_x$ . In the present article, we first give complete form of operator and recover the same type of behavior, with additional terms also involving wedges linked with the potential $V$ .
The present work is a natural continuation of [1, 3, 4], and as there we will make a strong use of pseudodifferential calculus.
We first list some notations used throughout the paper. Denote respectively by $\left( \cdot, ~\cdot \right)_{L^2}$ and $||\cdot||$ the inner product and the norm in $L^2(\mathbb R^{n})$ . For a vector-valued functions $U=\left( u_1, \cdots, u_n \right)$ the norm $||U||_{L^2}$ stands for $\left( \sum\limits_j||u_j||_{L^2}^2 \right)^{1/2}$ .
To simplify the notation, by $A\lesssim B$ we mean there exists a positive constant $C$ , such that $A\leq C B$ , and similarly for $A\gtrsim B$ . While the notation $A\approx B$ means both $A\lesssim B$ and $B\lesssim A$ hold.
Now, we introduce some notations of phase space analysis and recall some basic properties of symbolic calculus, and refer to [8] and [11] for detailed discussions. Throughout the paper let $g$ be the admissible metric $|dz|^2+|d\zeta|^2$ and $m$ be an admissible weight for $g$ (see [8] and [11] for instance the definitions of admissible metric and weight). Given a symbol $p(z, \zeta)$ , we say $p\in S\left( m, ~g \right)$ if
with $ C_{\alpha, \beta}$ a constant depending only on $\alpha, \beta$ . For such a symbol $p$ we may define its Weyl quantization $p^w$ by
The $L^2$ continuity theorem in the class $ S\left( 1, ~g \right)$ , which will be used frequently, says that if $p\in S\left( 1, ~g \right)$ then
We shall denote by $Op (S(m, g))$ the set of operators whose symbols are in the class $S(m, g)$ . Finally, let's recall some basic properties of the Wick quantization, and refer the reader to the works of Lerner [11] for thorough and extensive presentations of this quantization and some of its applications. Using the notation $Z= (z, \zeta)\in \mathbb R^{2n}$ , the wave-packets transform of a function $u \in\mathcal S\left( \mathbb R^{n} \right)$ is defined by
with $ \varphi_Z(v)=2^{n/4}e^{-\pi|v-z|^2}e^{2i\pi(v-z/2)\cdot\eta}, ~~ v\in\mathbb R^n, $ then one can verify that $W$ is an isometric mapping from $L^2(\mathbb R^{n})$ to $L^2(\mathbb R^{2n})$ ,
Moreover the operator $\pi_{\mathcal H}=WW^*$ , with $W^*$ the adjoint of $W$ , is an orthogonal projection on a closed space in $L^2$ whose kernel is given by
We define the Wick quantization of any $L^\infty$ symbol $p$ as $p^{\rm Wick} =W^* p W.$ The main property of the Wick quantization is its positivity, i.e.,
According to Proposition 2.4.3 in [11], the Wick and Weyl quantizations of a symbol $p$ are linked by the following identities
with
We also recall the following composition formula obtained in the proof of Proposition 3.4 in [10]
with $T$ a bounded operator in $L^2(\mathbb R^{2n})$ , when $p\in L^{\infty}(\mathbb R^{2n})$ and $q$ is a smooth symbol whose derivatives of order $\geq2$ are bounded on $\mathbb R^{2n}$ . The notation $\left\{p, q\right\}$ denotes the Poisson bracket defined by
In this section, we are mainly concerned with the estimate in weighted $L^2$ norms, that is
Proposition 3.1 Let $V(x)\in C^2(\mathbb R^3;~\mathbb R)$ satisfy condition (1.8), then
In order to prove the proposition, we begin with
Lemma 3.2 Considerate the operator $\mathcal{L}$ in (1.5), in the elliptic direction we have an estimate. For all $u\in C_0^{\infty}(R^3)$ ,
where $\left( \cdot, ~\cdot \right)_{L^2}$ and $||\cdot||_{L^2}$ standing for the inner product and norm in $L^2(\mathbb R_{x, y}^{6})$ .
Proof Observing $i(y\cdot D_x-\partial_xV(x)\cdot D_y)$ is skew-adjoint, then
The inequality hold due to
By (1.2) and (1.3) one has, for any $y, \eta\in \mathbb R^3$ and any $\alpha\in\mathbb Z_+^3$ ,
then
So we complete the lemma.
Lemma 3.3 Let $G\in S(1, |dy|^2+|d\eta|^2)$ and $B(y)$ be the matrix given in (1.6), we have $\forall~u\in C_0^\infty(\mathbb R^6)$ ,
Proof We notice that ${p(y)}^\alpha \in S({p(y)}^\alpha, |dy|^2+|d\eta|^2)$ , then
For the first term to (3.4),
where the third holds, since $G\in S(1, |dy|^2+|d\eta|^2)$ . As to the second term,
we get the third inequality from
Now, we will estimate the last term, similar to the above inequality, we get
Together the above estimate and Lemma 3.2 give Lemma 3.3.
Lemma 3.4 For all $u\in C_0^{\infty}(R^3)$ , we have
Proof In this proof, we let $u\in C_0^{\infty}(R^{2n})$ , the conclusion will follow if one could prove
From (1.7) we have $\left\langle y \right\rangle ^{1+\frac{1}{3}\gamma}|B(y)D_yu|\geq\left\langle y \right\rangle ^{1+\frac{5}{6}\gamma}|D_yu|+\left\langle y \right\rangle ^{1+\frac{5}{6}\gamma}|(y\wedge D_y)u|.$ As a preliminary step, let's first show that for any $\varepsilon>0$ there exists a constant $C_\varepsilon>0$ such that
In fact, the estimate
yields
Consequently, using (1.5), we compute
And thus
where the second inquality follows from
the third inquality holds due to interpolation inequality. The forth inquality holds because
and the last inequality follows from
As a result
and notice that $\gamma\geq0$ ,
Then we gain inequality (3.7).
Now we prove (3.6). Let's first write
the second inequality using (3.2). For the last term, we have
then the desired estimate (3.5) follows from the above inequalities and (3.7), completing the proof of Lemma 3.4.
Proof of Proposition 3.1 Let $\rho \in C^1\big(\mathbb{R}^{2n}\big)$ be a real-valued function given by
where $\chi\in C_0^\infty(\mathbb R;~[0, 1])$ such that $\chi=1$ in $[-1, 1]$ and supp $\chi \subset[-2, 2]$ . So we have
And it is easy to verify that $|\rho|\leq1$ .
Using the notation $Q=y\cdot D_x-\partial_xV(x)\cdot D_y$ ,
which along with yields ${\rm Re} \left( iQu, ~\rho u \right)_{L^2}\lesssim | \left( \mathcal{L}u, ~ u \right)_{L^2}|+| \left( \mathcal{L}u, ~ \rho u \right)_{L^2}|.$ Next, we want to give a lower bound for the term on the left side. Direct computation shows that
with $\mathcal A_j$ given by
We will proceed to treat the above three terms. First one has
from which it follows that
Here we used (3.8) in last inequality. As for the term $\mathcal A_2$ we make use of the relation
to compute
the first inequality using the fact that
As a result, we conclude
For the term $\mathcal A_3$ , using (1.8) gives
and thus
this along with (3.9), (3.10) and (3.11) shows that
Now for any $u\in C_0^\infty(\mathbb R^{2n})$ , we use the above estimate to the function $\left\langle \partial_xV(x) \right\rangle ^{1/3}u$ ; this gives
which, together with the fact that $\gamma\geq 0$ , implies
Moreover in view of (1.8), we have
Then the desired inequality (3.1) follows, completing the proof of Proposition 3.1.
In this section, we always consider $X=(x, \xi)\in\mathbb R^6$ as parameters, and study the operator acting on the velocity variable $y$ ,
where $Q_X=y\cdot \xi-\partial_xV(x)\cdot D_y$ and $ B(y)$ is the matrix given in (1.6).
Notations Throughout this section, we will use $||\cdot||_{L^2}$ and $\left( \cdot, ~\cdot \right)_{L^2}$ to denote respectively the norm and inner product in the space $L^2(\mathbb R_y^3)$ . Given a symbol $p$ , we use $p^{\rm Wick}$ and $p^{w}$ to denote the Wick and Weyl quantization of $p$ in $(y, \eta)$ .
The main result of this section is the following proposition.
Proposition 4.1 Let $\lambda$ be defined by
then the following estimate
holds for all $u\in \mathcal S (\mathbb R_y^3)$ , uniformly with respect to $X$ .
We would make use of the multiplier method introduced in [4], to show the above proposition through the following subsections.
Before the proof of Proposition 4.1, we list some lemmas.
Lemma 4.2 Let $\lambda$ be defined in (4.2), then
uniformly with respect to $X$ . Moreover if $\sigma\leq \frac{1}{3}$ then
with $r\in\left( 1, |dy|^2+|d\eta|^2 \right)$ uniformly with respect to $X$ .
Proof By direct verification, we see that for all $(y, \eta)\in~\mathbb R^{2n}$ and all $\alpha, \beta\in \mathbb{Z}_+^n$ , one has
which implies (4.4). Moreover note that for $\sigma\leq\frac{1}{3}$ ,
then we get (4.5) if $\sigma\leq \frac{1}{3}$ , and thus (4.6) in view of (2.4), completing the proof of Lemma 4.2.
Lemma 4.3 Let $\lambda$ be given in (4.2), then for all $u\in \mathcal S(\mathbb R^3)$ , one has
where $\Phi$ is defined by
Proof Similar to (3.2), we have, for any $u\in, \mathcal S(\mathbb R_y^{3})$ ,
Using the above inequality to $D_{y_j}u$ gives
which with the fact that $\gamma\geq0$ implies
So we only need to handle the last term in the above inequality. Direct verification shows
This gives
By Parseval's theorem, we may write, denoting by $\hat u$ the Fourier transform with respect to $y$ , $|\left( \xi_j u, ~D_{y_j} u \right)_{L^2}|=|\left( \xi_j \hat u, ~\eta_j \hat u \right)_{L^2 (\mathbb R^{6}_{\eta})}|, $ and hence
due to the inequality $|\xi_j\eta_j|\leq \varepsilon |\eta|^4+C_\varepsilon \left\langle \xi \right\rangle ^{4/3}.$ From (1.7) it follows that
the last inequality using Lemma 3.4.
Due to the arbitrariness of the number $\varepsilon $ , the above inequalities along with (4.10) and (4.11) gives the desired upper bound for the first term on the left side of (4.7).
It remains to treat the second term. In the following discussion, we use the notation
From (4.9), it follows that
In order to handle the last term in the above inequality, we write
Next we proceed to treat the above four terms. For the term $\mathcal N_1$ one has, with $\lambda$ defined in (4.2),
the last inequality holding because $ \left( \lambda^{-1/3} \right)^w A \left( \lambda^{-2/3} \right)^w \in {\rm Op} \left( S(1, ~|dy|^2 +|d\eta|^2) \right).$
On the other hand,
Observing (4.4), symbolic calculus give that
with $d_j$ , $1\leq j\leq 3$ , belonging to $S\left( \lambda^{2/3}, |dy|^2+|d\eta|^2 \right)$ uniformly with respect to $X$ . This shows
Combining the above inequalities, we have
Direct verification shows
with $a_{j, k}^\ell\in\left\{0, -1, +1\right\}$ , and thus
the last inequality using (3.2). It remains to treat $\mathcal N_5$ , and by (1.2) and (3.2), we have
Combining the above estimates, we conclude
This along with (4.12) and (4.13) yields the desired upper bound for $||\left\langle y \right\rangle ^{\gamma/2}|y\wedge D_y|^2||_{L^2}$ , letting $\varepsilon $ small enough. The proof of Lemma 4.3 is thus completed.
Lemma 4.4 Let $g\in S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ , and let $\lambda$ be defined in (4.2). Then for any $\varepsilon >0$ , there exists a constant $C_\varepsilon $ such that
where $\Phi$ is given in (4.8).
Proof As a preliminary step we firstly show that for any $\varepsilon >0$ , there exists a constant $C_\varepsilon $ such that
where $d$ is an arbitrary symbol belonging to $S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ . Observing (1.3) and (4.5), symbolic calculus (see for instance Theorem 2.3.8 in [11]) give that the symbols of the following commutators $\left[ \nu(y), ~\left( \lambda^{1/3} \right)^{w} \right], $ $\left[ \mu(y), ~\left( \lambda^{1/3} \right)^{w} \right], $ belong to $S\left( \Phi^{1/3}, |dy|^2+|d\eta|^2 \right)$ uniformly with respect to $X$ . As a result, using the notation
we have
The last inequality holding because
since $d\in S\left( 1, |dy|^2+|d\eta|^2 \right)$ uniformly with respect to $X$ . Moreover using (4.9) gives
Denote
Observing (4.5), symbolic calculus give that
with $f_j$ , $1\leq j\leq 7$ , belonging to $S\left( \Phi^{1/3}, |dy|^2+|d\eta|^2 \right)$ uniformly with respect to $\varepsilon $ and $X$ . It then follows that
Using similar arguments as the treatment of $\mathcal Z_1$ and $\mathcal Z_2$ , we conclude
This along with (4.16) gives
since
Moreover, we have
which can be deduced similarly as above, since by (1.3),
uniformly with respect to $X$ . Next we will treat the commutator $\left[ i Q_X, ~\left( \lambda^{1/3} \right)^{w} \right]$ , whose symbol is
In view of (4.4) and (4.2), one could verify that the above symbol belongs to
uniformly with respect to $X$ . As a result, observing $\lambda^{1/3}\in S(\lambda^{1/3}, ~|dy|^2+|d\eta|^2)$ uniformly with respect to $X$ , we have
uniformly with respect to $X$ , which implies
This along with (4.17) and (4.18) gives (4.15), since
Next we prove (4.14). The relation
gives, with $\tilde\varepsilon >0$ arbitrary,
We could apply (4.15) with $d=1+g$ to estimate the last term in the above inequality; this gives, with $\varepsilon >0$ arbitrary,
Let $\varepsilon $ small enough yields the desired estimate (4.14). The proof is thus completed.
In what follows, let $h_N$ , with $N$ a large integer, be a symbol defined by
where
with $\chi\in C_0^\infty(\mathbb R;~[0, 1])$ such that $\chi=1$ in $[-1, 1]$ and supp $\chi \subset[-2, 2]$ .
Lemma 4.5 Let $\lambda_N$ be given in (4.20). Then
uniformly with respect to $X$ . Moreover, if $\sigma\leq 1$ , then
Proof The proof is the same as Lemma 4.2.
Lemma 4.6 The symbol $h_N$ given in (4.19) belongs to $S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ .
Proof straightforward calculatation to get
combined with the following inequality $\left( |y\wedge\eta|^2+|y|^2+|\eta|^2 \right)\leq \lambda_N ^{2/3} ~~~ \text{in ${\rm supp}\psi_N$}$ give the desired lemma.
Lemma 4.7 Let $\lambda_N $ and $\psi_N$ be given in (4.20) and (4.21). Then for any $\sigma\in\mathbb R$ , the following two inequalities
hold uniformly with respect to $(x, \xi)$ .
Proof Using the inequality $ \left\langle \partial_xV\wedge\xi \right\rangle \leq N^{5/6}\lambda_N^{5/3} $ due to (4.20), we can caiculate that for any $\sigma\in\mathbb R$ one has
And thus (4.24) follows. In order to show (4.25), we write $|\left( \xi\cdot\partial_\eta+\partial_xV(x)\cdot\partial_y \right) \psi_N|=\left( \mathcal K_1+\mathcal K_2 \right)$ with
Using (4.24) shows $\mathcal K_2\lesssim N^3 \left( |y\wedge\eta|^{2}+|y|^2+|\eta|^2 \right).$ Moreover direct computation gives
the last inequality following from the fact that $\lambda_N^{2/3}\lesssim \left( |y\wedge\eta|^2+|{y}|^2+|\eta|^2 \right) N^2$ on the support of the function $\chi'\Big((|y\wedge\eta|^{2}+|y|^2+|\eta|^2 )N^2 \lambda_N ^{-2/3}\Big), $ then the above inequalities yield the desired inequality (4.25). The proof of Lemma is thus completed.
The rest of this section is occupied by
Proof of Proposition 4.1 Since the proof is quite long, we divide it into three steps.
Step Ⅰ Let $N$ be a large integer to be determined later and $H=h _N^{\rm Wick}$ be the Wick quantization of the symbol $h_N $ given in (4.19). To simplify the notation we will use $C_N$ to denote different suitable constants which depend only on $N$ . In the following discussion, let $u\in \mathcal S(\mathbb R^3_y)$ . By (2.4) and Lemma 4.6, we can find a symbol $\tilde h_N$ such that $H=\tilde h_N^{w}$ with $\tilde h_N\in S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ . Then using Lemma 3.3, one gives
This together with the relation
Next we will give a lower bound for the term on the left side. Observe the symbol of $Q_X$ is a first order polynomial in $y, \eta$ . Then $i Q_X =i\left( y\cdot\xi-\partial_xV(x)\cdot\eta \right)^{\rm Wick}, $ and hence
where $\left\{\cdot, ~\cdot\right\}$ is the Poisson bracket defined in (2.5). Direct calculus shows
the last inequality holding because $ \lambda_N^{2/3}\leq N^2\left( |y\wedge\eta|^2+|y|^2+|\eta|^2 \right) $ on the support of $1-\psi_N$ . Due to the positivity of the Wick quantization, the above inequalities, along with (4.26), (4.27) and the estimate
due to (4.9), yield
where $R_j$ are given by
Step Ⅱ In this step, we will treat the above terms $R_j$ , and show that there exists a symbol $q$ , belonging to $ S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ , such that
For this purpose, we define $q$ by
Then one can verify that $q\in S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $(x, \xi)$ . Thus by (3.4), we conclude
On the other hand, it is just a direct computation of the Poisson bracke to see that
Moreover, we have $R_{1, 2} \lesssim \left( |\partial_xV(x)\wedge\eta+y\wedge\xi|^2+|\partial_xV(x)|^2+|\xi|^2 \right)^{1/3}\lesssim \lambda_N^{2/3}, $ and
where the last inequality holds because
on the support of $1-\varphi$ . These inequalities, combining (4.33) and (4.32), yield
Consequently, observing that
we get the desired upper bound for the terms $R_1$ and $R_2$ . It remains to handle $R_3$ . By virtue of (4.24) and (4.25), we compute
The forth inequlity result from
As a result, the positivity of Wick quantization gives
Thus the desired estimate (4.30) follows.
Step Ⅲ Now, we proceed the proof of Proposition 4.1. From (4.29) and (4.30), it follows that there exists a symbol $p\in S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ , such that
which allows us to choose an integer $N_0$ large enough, such that
Consequently, observing that $\lambda^{2/3} \lesssim \lambda_{N_0}^{2/3}+|y|^2+|\eta|^2$ with $\lambda$ defined in (4.2), we get, combining (4.28),
Since $\left\langle \partial_xV(x) \right\rangle ^{2/3}+\left\langle \xi \right\rangle ^{2/3}\leq \lambda^{2/3}$ , the above inequality yields
Since $p\in S(1, |dy|^2+|d\eta|^2)$ uniformly with respect to $X$ , then applying the above inequality to the function $\left( \left\langle \partial_xV(x) \right\rangle ^{2/3}+\left\langle \xi \right\rangle ^{2/3} \right)^{1/2}u$ implies
Similarly, since $\left\langle \partial_xV(x)\wedge \xi \right\rangle ^{2/5} \leq \lambda^{2/3}$ , then by virtue of (4.34) we have, repeating the above arguments,
Now, we apply (4.34) to the function $\left( \lambda^{1/3} \right)^{w}u$ , to get
where the last inequality follows from (4.14). Furthermore, using (4.6) implies
the last inequality following from (4.35) and (4.36). Let the number $\varepsilon $ small enough yields $||\left( \lambda^{2/3} \right)^{w}u||_{L^2 } \lesssim ||\mathcal{L}_X u||_{L^2 } + ||u||_{L^2 }.$ This, along with (4.7) and (4.35), gives the desired estimate (4.3), completing the proof of Proposition 4.1.
In this section, we will show the hypoelliptic estimates in spatial and velocity variables for the original operator $\mathcal{L}$ .
Proposition 5.1 Let $V(x)$ be a $C^2$ -function satisfying assumption (1.8). Then for any $u\in C_0^\infty\big(\mathbb{R}^{2n}\big)$ , one has
Proof The proof of is quite similar as that of Proposition 4.1 in [2] and [3]. So we only give a sketch here and refer to [2] and [3] for more detailed discussions. With each fixed $x_\mu\in \mathbb R^3$ , we associate an operator
Let $P_{X_\mu}$ , with $X_\mu=(x_\mu, \xi)$ , be the operator defined in (4.1), i.e.,
Observe $\mathcal F_x \mathcal{L}_{x_\mu}= \mathcal{L}_{X_\mu}, $ where $\mathcal F_x$ stands for the partial Fourier transform in $x$ variable. Suppose $V$ satisfies condition (1.8). Then performing the Fourier transform with respect to $x$ , it follows from (4.3) that $\forall~u\in C_0^\infty\big(\mathbb{R}^{6}\big), $
Lemma 4.2 in [1] shows the metric $g$ defined by $g_x=\left\langle \partial_x V(x) \right\rangle ^{2/3}|dx|^2, ~~ x\in\mathbb{R}^3$ is slowly varying, i.e., we can find two constants $C_*, r_0>0$ such that if $g_x(x-y)\leq r_0^2$ , then
The main feature of a slowly varying metric is that it allows us to introduce some partitions of unity related to the metric (see for instance Lemma 18.4.4 of [8]). Precisely, we could find a constant $r>0$ and a sequence $x_\mu\in\mathbb{R}^n, \mu\geq1, $ such that the union of the balls
coves the whole space $\mathbb{R}^{n}.$ Moreover there exists a positive integer $N_r , $ depending only on $r, $ such that the intersection of more than $N_r $ balls is always empty. One can choose a family of nonnegative functions $\left\{\varphi_\mu\right\}_{\mu\geq 1}$ in $S(1, g)$ such that
Repeat the precess in [3], we see
Using the notation
we may write $\varphi_\mu \mathcal{L} u=\mathcal{L}_{x_\mu}~\varphi_\mu\, u+ R_\mu u, $ then
On the other hand, by Lemma 4.9 in [1], we have $\sum\limits_{\mu\geq1}|| R_\mu u||_{L^2}^2 \lesssim ||\mathcal{L} u||_{L^2}^2+||u||_{L^2}^2.$ The above two inequalities yield
Using (5.4) and (5.2), we have
As a result, combining these inequalities gives (5.1). The proof is then completed.