We consider, for , resolvent estimates for the semiclassical Schrödinger operator . Near infinity, the potential takes the form , where is a long range potential which is Lipschitz with respect to the radial variable, while for some . Near the origin, may behave like , provided . We find that, for any , there are such that we have a resolvent bound of the form for all . The h-dependence of the bound improves if decays at a faster rate toward infinity.
Let be the Laplacian on , . In this article, we study the semiclassical Schrödinger operator with real valued potential,
We use to denote polar coordinates on . For a function f defined on some subset of , we use the notation and denote the derivative with respect to the radial variable by .
We first describe the conditions we impose on the potential V. Let be such that near while near . We suppose that
has the bound
for some and some
On the other hand, we suppose may be decomposed as a sum of long- and short-range terms:
The long-range term must satisfy, for some and some
that
where denotes the characteristic function of . We also require that there is a function such that, for each , the function has distributional derivative equal to , and
where has the properties
A typical example of the function is for some .
As for the short-range term , we require
for some and . Depending on the value of δ, should satisfy
The properties (1.2) and (1.5) imply for some , . Therefore, by [19, Theorem 8], P is self-adjoint when equipped with domain the Sobolev space . Thus the resolvent is bounded for all . Our main result is the following limiting absorption resolvent estimate.
Let. Fixand. Suppose V satisfies properties (
1.2
) through (
1.11
). Definewhere.
If, there existandindependent of ε and h so thatIf, then for any, there existandindependent of ε and h so thatFinally, if, then for any, there existandindependent of ε and h so that
The proof of Theorem 1.1 in fact establishes a more complicated but slightly improved version of (1.14). For any , there exist and independent of ε and h so that
where .
The condition is needed for technical reasons in the proof of (1.15). However, it is clear that once (1.15) holds for some , it holds for all too (with the same constants C and ).
Theorem 1.1 improves upon recent work on resolvent estimates in low regularity in several ways. When , the bound (1.13) was previously proved in [14] if , , and . Second, when , it was established in [29] that, if , , and for some , then
Thus, the novelties of Theorem 1.1 are that it gives resolvent bounds for more types of decay conditions on and , improves those bounds in several cases, allows V to be singular as , and includes the dimension two case.
Furthermore, Theorem 1.1 warrants comparison with the resolvent bounds obtained in [31,32] for short-range, radially symmetric potentials V:
Thus, another way to interpret how Theorem 1.1 extends the previous literature is that it shows arbitrary short-range potentials have resolvent bounds similar to those for short-range radial potentials, though additional losses remain.
Bounds on are known to hold under various geometric, regularity, and decay assumptions. Burq [3,4] showed for V smooth and decaying sufficiently fast near infinity, and also for more general perturbations of the Laplacian. Cardoso and Vodev [5] extended Burq’s estimate to infinite volume Riemannian manifolds which may contain cusps. This exponential behavior is sharp in general, see [10] for exponential resolvent lower bounds. On , , still holds if V has long-range decay and Lipschitz regularity with respect to the radial variable [8,13,20,23,30]. Potentials with singularities near zero are treated in [13,20], and in particular [20] requires , for
and . In one dimension, if V is a finite Borel measure [17].
In contrast, if , , has purely terms, it is an open problem to determine whether the bounds (1.13), (1.14), and (1.15) have optimal h-dependence. Further works on resolvent estimates with little regularity assumed are [9,12,16,21,24,26–28].
To prove Theorem 1.1, we establish a global Carleman estimate (5.1). This Carleman estimate is the byproduct of patching together what we call the away-from-origin estimate (5.6) and the near-origin estimate (5.7).
The away-from-origin estimate is an application of the so called energy method, a well established tool for proving semiclassical Carleman estimates. In particular, we combine and update the approaches from [14, Section 3] and [20, Section 3], to construct the weight and phase , which are key inputs to the energy method.
Near the origin, should vanish like , to absorb the singular behavior of both V and, in dimension two, the so called effective potential (the latter arising after we separate variables in Section 2). In our situation, is only near zero. In the proof of Proposition 4.1 below, this necessitates , which is a stronger requirement than what is needed if has some radial regularity (see [20, Section 3]). This is the source of the discrepancy between (1.4) and (1.16).
Away from the origin, roughly speaking, should increase and have , to furnish the weights appearing in (1.12). Meanwhile, the main task of is control without becoming too large, so as to keep bounded. Since may decay slowly toward infinity, this is a delicate balancing act, and the compromise we strike is that have comparably slow decay for and suitable , see (3.12). Our choice of M, see (3.7), is inspired by [29, Section 2] and more refined compared to [14, Section 3]. This is why we can handle decay slower than that treated in [14].
The near-origin estimate was proved by Obovu [20, Lemma 2.2] using the Mellin transform, building on an earlier study of radial potentials [11]. It makes up for the loss in the away-from-origin estimate stemming from the vanishing of as . We emphasize that this vanishing of is essential in dimension two, even if is not singular, because in that case the effective potential has an unfavorable sign.
Resolvent bounds like (1.13), (1.14), and (1.15) have application to local energy decay for the wave equation
where Ω is a compact (possibly empty) obstacle with smooth boundary, and the initial data are compactly supported. A general logarithmic decay rate was first proved by Burq [3,4] for c smooth. Similar decay was subsequently established for and bounded from above and below and identically one outside of a compact set [22, Theorem 2]. See also [1,2,6,15,18]. Since Theorem 1.1 allows the potential to be singular as , we expect [22, Theorem 2] extends to c which tends to 0 at a point. However, for such a c, the low frequency character of the solution to (1.17) still needs to be accounted for (see, e.g., [22, Section 4]). This question will be taken up elsewhere.
It’s worth mentioning that, in dimension , the hypotheses of Theorem 1.1 hold for potentials V which are “Coulomb-like” near , i.e., obeying as . However, the assumption (1.2) does not capture such behavior in dimension two, because in that case is not in near the origin. For Coulomb-like V in dimension two, one can use a quadratic form to show that is self-adjoint with respect to [7, Proposition 1.1]. However, it seems difficult to use the method of this paper to prove resolvent estimates for . This is because our Carleman estimate holds only for functions in . While it is well known that is dense in for any , it is not evident from the standard result on essential self-adjointness for singular potentials [25, Theorem 2] that a similar class of smooth functions is dense in , where . This is a technical but nevertheless interesting issue that warrants further study.
Preliminary calculations and overview of proof of Theorem 1.1
In this section, we set the stage for proving Theorem 1.1 by means of the energy method, which has proven to be a dependable tool for establishing resolvent estimates in low regularity (see, e.g., [5,8,14,20]). Throughout this section, we take P as in (1.1), and assume the potential V obeys (1.2) through (1.11).
We work in polar coordinates, beginning from the well known identity
where
and denotes the negative Laplace-Beltrami operator on . Let φ be a soon-to-be-constructed phase function on , which is locally absolutely continuous, and obeys and . Using φ, we form the conjugated operator
For , define a spherical energy functional,
where and denote the norm and inner product on , respectively. For a weight that is piecewise , the distribution on is given by
where we have put
We shall construct w so that and . Then using (2.4) and for all , we find
For , put , , yielding
In Section 6, we show how Theorem 1.1 follows from a certain global Carleman estimate, see Lemma 5.1. An essential ingredient for this Carleman estimate is to specify φ and w as precisely as possible, in order that the second line of (2.7) has a good lower bound. More precisely, putting
we shall see that it suffices for w and φ to satisfy, for suitable ,
To facilitate the proof of (2.9), we proceed, as in [13,14,20], to analyze A and B in terms of the auxiliary functions
In particular, from (2.8) and (2.10),
So, to show (2.9), it is enough to bound the bracketed expression in (2.11) from below by . The next section is devoted to constructing w and φ, and their corresponding and Φ, that will bring about (2.9).
Determination of the weight and phase
In this section, we develop the functions w and φ, and their associated and Φ, as in (2.10). They play an essential role in the proof of the lower bound (2.9) for (Proposition 4.1), and in the proof of the Carleman estimate (Lemma 5.1). We should keep in mind that A and B (see (2.8)) depend not only on w and φ, but also on a potential V that obeys (1.2) to (1.11).
First, we fix
Using (1.7) and (1.8), fix independent of h large enough so that
Next, we introduce several quantities depending on the semiclassical parameter h and on δ as in (1.10). These quantities also involve parameters , that are independent of h and will be specified in the proof of Proposition 4.1:
In this and later sections, we always assume h is restricted to , where is small enough so that
In particular, from , and , (3.7), (3.8), (3.9),
Our weight w and phase φ are:
where
The parameters τ and κ are independent of h and will be fixed in the proof of Proposition 4.1. Note that the denominator of is at least since and , where y is given by (1.6).
Recalling that and Φ are defined by (2.10), we use (3.11) and (3.12) to calculate
To conclude this section, we collect several basic properties of w, and an elementary Lemma about , which are important to the proofs of the lower bound (2.9) and the Carleman estimate.
There exists C independent of h so that for all,
To see (3.20), note that from (3.11) w is clearly increasing, so we need only compute . By (3.5), (3.8) and (3.15), for some independent of ,
For (3.21), we use (3.11) to compute for :
for some constant independent of , where when we have used that
Finally, (3.22) follows from (3.20) and
□
We note first that thanks to (3.16), (3.17), and (1.11). The estimate (3.23) follows by combining
with
□
Proof of the main estimate
Suppose V satisfies (
1.2
) through (
1.11
). Fix,,, andLet w and φ be as constructed in Section
3
.
There existandas in (
3.7
),as in (
3.14
),as in (
3.16
),, and, all independent h, so thatand
We prove Proposition 4.1 over the course of Sections 4.1, 4.2, and 4.3. Throughout the proof, C denotes a positive constant whose value may change from line to line, but is always independent of T, t, τ, κ, and h. Initially, we take small enough so that (3.9) holds. At several steps of the proof, we further decrease if necessary.
Using these, , and that and in a neighborhood of (see (1.3) and (1.5)), we revisit (2.11) and find
In the second estimate, we used that the minimum is less than , but in the third estimate, we used that it is less than . Therefore
Since (see (1.4)), and since (4.1) implies , we may choose large enough, independent of h, so that (4.2) holds for .
Case:
When ,
We first derive some bounds on (see (3.12)), and for this we use Lemma 3.2. By (3.23),
Next, we bound the exponent depending on the value of δ. If or 1, then both k and are independent of h (see (3.6) and (3.16), respectively), thus we simply have . On the other hand, when , both k and depend on h. But in this case thanks to (3.9), and, by (3.16), (3.17) and ,
Thus we conclude
The estimate (4.5) informs our choice of κ. If or 1, fix . If , fix small enough so that the factor in (4.5) is bounded from above by , where
So with κ now fixed, we have
As in the previous case, we estimate each of the terms on the right side of (2.11), keeping in mind that now . By , (3.19), (3.16), the lower bound in (4.7), and ,
Continuing on, we use , (3.19), the upper bound in (4.7), , , and to find
To estimate the next term, we use , for , , , and
to see
To finish the estimate we used (1.11), (3.6) and (3.17). In particular, when or 1, and ; when , , , and .
To estimate the final term we use , , and (3.3), yielding
Putting the above bounds into (2.11) and recalling yields
Modify τ to be the maximum of and its value assigned previously. Restricting h further so that , we arrive at (4.2) when .
When ,
Combining the two identities in the first line of (4.9), and substituting the expression for (see (3.15)), shows
Recall from (2.6) that we need to have . Since we have previously arranged for all (see (3.10)), and because (see (1.9)), we may take smaller, if needed, so and imply .
From the second line of (4.9),
From for and (4.7), we also find
We now make additional calculations involving that are crucial below. This is where we make use of the parameters , that were introduced in the definition of M, see (3.7). First, consider when . By our standing assumption (3.9), we have and . Using the definition of k (see (3.6)), it is straightforward to verify that too. Thus, from , , (see (3.7)), and (see (3.10)),
We will fix the parameter T for this case later.
Second, consider when . Then and we fix at once. Furthermore, (see (3.7)) and (see (3.10)). Then for small enough and , . Using also ,
Once more, our goal is to control the terms on the right side of (2.11), but this time for . First, by (see (4.9)), (see (4.10), , and the upper bound in (4.11),
Note that in the last step we used for while for . Using now the first line of (4.12) and the first line of (4.13),
Next, by , , , , the upper bound in (4.11),
Since for all (see (3.10)), by further decreasing as needed we attain for and . On the other hand we attain for and . So, overall,
Continuing on, we decrease if necessary, so if . Complementing this with , , , , , the lower bound in (4.11), and ,
Recalling and for , while and for , we substitute,
Here, we also used that, when , (see (3.9)), and when , . Combining this with the previous estimate, the second line of (4.12), and the second line of (4.13),
The final term we need to estimate is,
where we used that, for , , (see (3.3)), and
From the above, and taking smaller so that , we conclude,
If , fix , and further decrease as needed, in particular so that , to arrive at (4.2) for . If , pick t large enough so that , and then further decrease so that , to attain (4.2) for .
Thus, by Sections 4.1 and 4.2, we have demonstrated (4.2).
Bounding the phase
Our remaining goal is to show (4.3). Recall (4.7) and (4.11):
We also have, from , for , and for ,
Using these, we estimate ,
Recall that we found,
where we used that we have fixed when and when . Combining this with (3.6):
and , we see that
In the case , we have already fixed independent of h. Therefore, for some independent of h,
Noting (see (4.6)), we have arrived at (4.3). □
Carleman estimate
Our goal in this section is to prove Lemma 5.1, which is a Carleman estimate from which Theorem 1.1 follows.
Suppose the assumptions of Proposition
4.1
hold. There existand, both independent of h and ε, so thatfor all,,, and.
There are three steps to the proof of Lemma 5.1. First, by way of Proposition 4.1, we establish a Carleman estimate which is similar to (5.1) but has a loss at the origin, because the weight w vanishes quadratically as (see (3.11)). We call this the away-from-origin estimate. Second, we use Obovu’s result [20, Lemma 2.2], which is based on Mellin transform techniques, to obtain an estimate for small r which does not have loss as . In fact, the pertinent weight in Obovu’s estimate is unbounded as . We call this the near-origin estimate. The third and final step is to glue together the near- and away-from-origin estimates.
We give the proof of Lemma 5.1 over the course of Sections 5.1, 5.2, and 5.3. The notation denotes the integral over with respect to the measure . Throughout, and are constants, both independent of h and ε, whose values may change from line to line.
Away-from-orgin estimate
We begin from (2.7). Applying (4.2), we bound the right side of (2.7) from below. For some ,
Next, we integrate both sides of (5.2). We integrate and use , and , hence . Using also (3.22) yields
The remaining task is to absorb the term involving on the right side of (5.3) into the left side. To this end, let with near , and near . We have
To get the second line, we used and for , see (3.11). The first term in the second line of (5.4) is easily absorbed into the left side of (5.3). As for the second term, integrating by parts,
and
These two identities, together with the facts that , , is bounded on , on , and on for and , imply
For h sufficiently small, the second line of (5.5) is readily absorbed into the right side of (5.3). Therefore, (5.3), (5.4), and (5.5) imply
Fix. There existand, all independent of ε and h, so that for all,,, and,where
Combining the near- and away-from-origin estimates
For , set . We have
where we used (3.21) and
Furthermore,
where, as in Section 5.1, . To get (5.12), we used (1.2) and (5.10). To get (5.13), we used (5.10), (3.12), and (3.14), hence
Consider now the second line of (5.9). We bound the first term appearing there using (5.7) and (5.11) through (5.13) ( for h small enough, see (5.8)). We bound the second and third terms using (5.6). Since negative powers of α are bounded from above by for h small, we conclude, for , , and ,
where we have used
Employing (5.6) once more, to bound the last line of (5.14), we arrive at (5.1) as desired. □
Resolvent estimates
In this section, we deduce Theorem 1.1 from the Carleman estimate (5.1). This same argument has been presented before, see, e.g., [8,13,14,20]. But we include it here for the sake of completeness. The constants and may change between lines but stay independent of E, ε, and h.
By the spectral theorem for self-adjoint operators, the bounds (1.13), (1.14), and (1.15) clearly hold for . Therefore, to prove Theorem 1.1, it suffices to consider .
Since increasing s in (1.12) decreases the operator norm, to establish a certain estimate for (1.12) for fixed independent h, it suffices to show the same estimate for h small enough and an h-dependent s of the form . For the rest of the proof, we assume s has this form.
By Lemma 5.1,
for all , , , and , and where . Moreover, for any ,
Setting , and using (6.2) to estimate from above in (6.1), we absorb the term that now appears on the right of (6.1) into the left side. Multiplying through by , and applying (4.3), we find, for , , , and ,
The final task is to use (6.3) to show, for , , , and ,
from which Theorem 1.1 follows. To establish (6.4), we prove a simple Sobolev space estimate and then apply a density argument that relies on (6.3).
The operator
is bounded . So, for such that ,
for some constant depending on , ε and h.
Given , the function because
with being bounded since .
Now, choose a sequence such that in . Define . Then, as ,
Also, applying (6.5),
We then achieve (6.4) by replacing v by in (6.3) and sending . □
Footnotes
Acknowledgements
It is a pleasure to thank Kiril Datchev and Jeffrey Galkowski for helpful discussions, as well as the anonymous referee for helpful comments and corrections. The author gratefully acknowledges support from ARC DP180100589, NSF DMS 2204322, and from a 2023 Fulbright Future Scholarship funded by the Kinghorn Foundation and hosted by University of Melbourne. The author affirms that there is no conflict of interest.
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