Weighted Sobolev spaces and rough elliptic estimates

Written by GPT-6.1 Sol (OpenAI) and GPT-6 Astra (OpenAI). Self-checked by the writing AI. Original exposition: CC0.

Working question: Does the order of a spatial weight and a derivative matter? Multiplication by ⟨x⟩t\langle x\rangle^t and the Fourier multiplier ⟨D⟩s\langle D\rangle^s generally do not commute. Even for integer derivatives the product rule produces lower-order terms. The norm-equivalence theorem controls these terms for all real exponents and then applies the resulting scale to the actual rough elliptic graph.

A Sobolev norm measures derivatives; a spatial weight measures behavior at infinity. Scattering problems need both at once. The position weight and the Fourier multiplier usually do not commute, so a definition must specify their order and prove that exchanging them gives an equivalent norm. After doing this for every real pair of exponents, we show that an elliptic graph estimate survives multiplication by a polynomial weight even when the operator has rough coefficients.

Read The Sobolev domain of an elliptic operator for the unweighted graph estimate and its precise coefficient class, and Admissible differential perturbations for the local multiplication estimates. For the smooth symbol calculus we use the complete programme proof Finite composition and adjoints with spatial weights. It supplies the symbol estimates, distribution identities and uniform finite remainders for the exact metric below. Fourier inversion, Plancherel, Schwartz density and the needed measure interchanges are proved in A finite-derivative bound for left quantization. The particular calculus interfaces are identified in Section 2. See also Lerner [L].

Write Dj=−i∂jD_j=-i\partial_j, ⟨x⟩=(1+∣x∣2)1/2\langle x\rangle=(1+|x|^2)^{1/2}, and

Mtu=⟨x⟩tu,Jsu=⟨D⟩su,s,t∈R.(1) M_tu=\langle x\rangle^t u,\qquad J_su=\langle D\rangle^s u,\qquad s,t\in\mathbb R. \tag{1}

The Fourier transform has kernel e−ix⋅ξe^{-ix\cdot\xi}. Thus JsJ_s is multiplication by ⟨ξ⟩s\langle\xi\rangle^s on the Fourier side, and HsH^s has norm ∥Jsu∥2\|J_su\|_2.

1. Measuring derivatives and decay

Definition 1.1. For arbitrary real s,ts,t, let

Hs,t(Rn)={u∈S′(Rn):MtJsu∈L2},∥u∥s,t=∥MtJsu∥2.(2) H^{s,t}(\mathbb R^n) =\{u\in\mathcal S'(\mathbb R^n):M_tJ_su\in L^2\}, \qquad \|u\|_{s,t}=\|M_tJ_su\|_2. \tag{2}

Here ss measures differentiability and tt measures spatial decay. Positive tt demands more decay; negative tt permits more growth. The case t=0t=0 is HsH^s, and the case s=0s=0 is weighted L2L^2.

Both MtM_t and JsJ_s are continuous automorphisms of S\mathcal S and S′\mathcal S'. For multiplication this follows from

∣∂γ⟨x⟩t∣≤Ct,γ⟨x⟩t−∣γ∣.(3) |\partial^\gamma\langle x\rangle^t| \le C_{t,\gamma}\langle x\rangle^{t-|\gamma|}. \tag{3}

To prove (3) for every real exponent, repeated differentiation produces a finite sum of terms cxν(1+∣x∣2)t/2−ℓc x^\nu(1+|x|^2)^{t/2-\ell} with 2ℓ−∣ν∣=∣γ∣2\ell-|\nu|=|\gamma|. A derivative on the monomial reduces ∣ν∣|\nu| by one; a derivative on the power increases ℓ\ell by one and ∣ν∣|\nu| by one. Thus this identity holds inductively, and ∣xν∣≤⟨x⟩∣ν∣|x^\nu|\le\langle x\rangle^{|\nu|} proves (3).

The product rule controls every Schwartz seminorm; the same argument with −t-t gives the inverse. On the Fourier side it proves the assertion for JsJ_s. The distribution actions follow by transposition, or by Fourier transformation and multiplication. In particular,

(MtJs)−1=J−sM−t.(4) (M_tJ_s)^{-1}=J_{-s}M_{-t}. \tag{4}

This order is essential.

Proposition 1.2. The space Hs,tH^{s,t}, with the norm in (2), is a Hilbert space continuously embedded in S′\mathcal S'. Schwartz functions are dense in it.

Proof. The map T=MtJsT=M_tJ_s sends the displayed space bijectively onto L2L^2, with inverse (4), and is an isometry for its defining norm. Pull back the L2L^2 inner product. Completeness follows: if TujTu_j converges to vv in L2L^2, then uju_j converges in the norm to T−1vT^{-1}v. The embedding L2⊂S′L^2\subset\mathcal S' is continuous by Cauchy–Schwarz against a Schwartz test, and T−1T^{-1} is continuous on S′\mathcal S', giving the asserted embedding.

For density, approximate TuTu in L2L^2 by Schwartz functions vjv_j. The functions T−1vjT^{-1}v_j are Schwartz and converge to uu in (2). No sign restriction on ss or tt entered this argument. □\square

For a smooth power tail u(x)=⟨x⟩−au(x)=\langle x\rangle^{-a},

u∈H0,t⟺a>t+n2.(5) u\in H^{0,t} \quad\Longleftrightarrow\quad a>t+\frac n2. \tag{5}

Indeed its squared weighted radial integrand is comparable at infinity to rn−1+2(t−a)r^{n-1+2(t-a)}. Equality gives a logarithmically divergent integral. In particular a nondecaying function can lie in a sufficiently negatively weighted space. Problem 2 compares this threshold with integer Sobolev orders.

2. The metric and the exact calculus interfaces

For 0<δ≤10<\delta\le1, use the phase-space metric

Gδ,(x,ξ)(y,η)=⟨x⟩−2δ∣y∣2+⟨ξ⟩−2∣η∣2.(6) G_{\delta,(x,\xi)}(y,\eta) =\langle x\rangle^{-2\delta}|y|^2 +\langle\xi\rangle^{-2}|\eta|^2. \tag{6}

For a positive weight ww, the scalar class S(w,Gδ)S(w,G_\delta) consists of smooth symbols with

∣∂xβ∂ξαa(x,ξ)∣≤Cαβw(x,ξ)⟨x⟩−δ∣β∣⟨ξ⟩−∣α∣.(7) |\partial_x^\beta\partial_\xi^\alpha a(x,\xi)| \le C_{\alpha\beta}w(x,\xi) \langle x\rangle^{-\delta|\beta|} \langle\xi\rangle^{-|\alpha|}. \tag{7}

This coordinate description agrees with the directional metric seminorms: test coordinate directions for one implication, and expand multilinear derivatives for the other. The constants at each derivative order involve only finitely many coordinate derivatives.

We check the metric conditions rather than infer them from (7). On phase space take σ((x,ξ),(y,η))=ξ⋅y−x⋅η\sigma((x,\xi),(y,\eta))=\xi\cdot y-x\cdot\eta. Quadratic duality gives

Gδ,(x,ξ)σ(y,η)=⟨ξ⟩2∣y∣2+⟨x⟩2δ∣η∣2,hδ(x,ξ)=⟨x⟩−δ⟨ξ⟩−1≤1.(8) \begin{aligned} G_{\delta,(x,\xi)}^\sigma(y,\eta) &=\langle\xi\rangle^2|y|^2 +\langle x\rangle^{2\delta}|\eta|^2,\\ h_\delta(x,\xi)&=\langle x\rangle^{-\delta}\langle\xi\rangle^{-1}\le1. \end{aligned} \tag{8}

Indeed weighted Cauchy–Schwarz bounds ∣η⋅v−y⋅ν∣2/Gδ,(x,ξ)(v,ν)|\eta\cdot v-y\cdot\nu|^2/G_{\delta,(x,\xi)}(v,\nu) by the first expression in (8). For a nonzero (y,η)(y,\eta), equality holds at v=⟨x⟩2δηv=\langle x\rangle^{2\delta}\eta, ν=−⟨ξ⟩2y\nu=-\langle\xi\rangle^2y; the zero vector gives zero. This proves the symplectic dual formula directly.

Here hδ2=sup⁡Gδ/Gδσh_\delta^2=\sup G_\delta/G_\delta^\sigma. Both coordinate coefficient ratios equal ⟨x⟩−2δ⟨ξ⟩−2\langle x\rangle^{-2\delta}\langle\xi\rangle^{-2}, giving the second expression in (8). The metric has no mixed position–frequency terms, so it also satisfies the reflection condition used for changes of quantization.

Lemma 2.1. The metric GδG_\delta is slowly varying and symplectically temperate. Every weight

wτ,μ(x,ξ)=⟨x⟩τ⟨ξ⟩μ,τ,μ∈R,(9) w_{\tau,\mu}(x,\xi)=\langle x\rangle^\tau\langle\xi\rangle^\mu, \qquad \tau,\mu\in\mathbb R, \tag{9}

is locally comparable and symplectically temperate for this metric.

Proof. Suppose Gδ,X(Y−X)≤r2G_{\delta,X}(Y-X)\le r^2, where X=(x,ξ)X=(x,\xi), Y=(y,η)Y=(y,\eta) and r<1/2r<1/2. Then

∣y−x∣≤r⟨x⟩δ≤r⟨x⟩,∣η−ξ∣≤r⟨ξ⟩.(10) |y-x|\le r\langle x\rangle^\delta\le r\langle x\rangle,\qquad |\eta-\xi|\le r\langle\xi\rangle. \tag{10}

The Japanese bracket is one-Lipschitz. Each bracket at YY, divided by the corresponding bracket at XX, therefore lies between 1−r1-r and 1+r1+r. Raising these ratios to the fixed powers in (6) and (9) proves the local comparisons.

For the global condition put

QY(X−Y)=Gδ,Yσ(X−Y).(11) Q_Y(X-Y)=G_{\delta,Y}^\sigma(X-Y). \tag{11}

Since both coefficients in (8) are at least one, QY(X−Y)≥∣X−Y∣2Q_Y(X-Y)\ge |X-Y|^2. In each direction,

⟨x⟩⟨y⟩,⟨y⟩⟨x⟩,⟨ξ⟩⟨η⟩,⟨η⟩⟨ξ⟩≤1+∣X−Y∣≤C(1+QY(X−Y))1/2.(12) \frac{\langle x\rangle}{\langle y\rangle}, \frac{\langle y\rangle}{\langle x\rangle}, \frac{\langle\xi\rangle}{\langle\eta\rangle}, \frac{\langle\eta\rangle}{\langle\xi\rangle} \le 1+|X-Y|\le C(1+Q_Y(X-Y))^{1/2}. \tag{12}

Compare the two coefficients of Gδ,XσG_{\delta,X}^\sigma with those of Gδ,YσG_{\delta,Y}^\sigma. Formula (12) bounds both ratios by a fixed power of 1+QY(X−Y)1+Q_Y(X-Y). This is the required dual-form temperateness inequality. The same formula gives wτ,μ(Y)/wτ,μ(X)≤C(1+QY(X−Y))Nw_{\tau,\mu}(Y)/w_{\tau,\mu}(X)\le C(1+Q_Y(X-Y))^N for a finite NN, including negative τ,μ\tau,\mu. □\square

The programme reading Finite composition and adjoints with spatial weights proves the following interfaces for exactly this metric and all its locally comparable, symplectically temperate weights. It uses our Fourier normalization throughout.

  1. Section 5 proves the continuous actions on S\mathcal S and S′\mathcal S'. Theorem 3.1 proves the exact quantization-change automorphism and inverse, so left and Weyl symbols give equivalent classes.
  2. Theorem 4.1 and Section 5 prove the finite-seminorm left product in S(w1w2,Gδ)S(w_1w_2,G_\delta), its finite remainder in S(w1w2hδN,Gδ)S(w_1w_2h_\delta^N,G_\delta), and its equality to operator composition on both spaces. Lemma 2.1 supplies the complete oscillatory estimates in all four near/far regions.
  3. Section 6 applies the proved finite-derivative operator bound to S(1,Gδ)S(1,G_\delta) and its quantization transforms. This gives the required L2L^2 bounds with finite-seminorm control.

Each of these bounds uses only finitely many symbol seminorms. Lerner [L], Lemma 2.3.12 and Theorems 2.3.18–2.3.19, gives the broader free-source formulas.

The constants depend on the fixed metric and weight comparison constants and the required finite seminorms. Thus bounded symbol families with common structural constants give uniform operator bounds. This uniformity will be needed for the truncated weights in Section 5. These interfaces concern smooth symbols; we will apply them to the weight operators, while treating rough coefficients by the separate multiplication estimate.

3. Exchanging the factors and mapping between spaces

Theorem 3.1. For every s,t∈Rs,t\in\mathbb R,

cs,t∥MtJsu∥2≤∥JsMtu∥2≤Cs,t∥MtJsu∥2.(13) c_{s,t}\|M_tJ_su\|_2 \le \|J_sM_tu\|_2 \le C_{s,t}\|M_tJ_su\|_2. \tag{13}

Each finite-norm condition implies the other, for u∈S′u\in\mathcal S'. Moreover, if a left symbol belongs to S(wτ,μ,Gδ)S(w_{\tau,\mu},G_\delta), then

a(x,D):Hs,t⟶Hs−μ,t−τcontinuously.(14) a(x,D):H^{s,t}\longrightarrow H^{s-\mu,t-\tau} \quad\text{continuously}. \tag{14}

All four exponents are arbitrary real numbers. The operator norm is bounded by finitely many symbol seminorms, with constants fixed by the exponents, metric and weight structure.

Proof. By (3), the symbols of MtM_t and JsJ_s belong to S(⟨x⟩t,Gδ)S(\langle x\rangle^t,G_\delta) and S(⟨ξ⟩s,Gδ)S(\langle\xi\rangle^s,G_\delta). The composite operators

A=JsMtJ−sM−t,B=MtJsM−tJ−s(15) A=J_sM_tJ_{-s}M_{-t},\qquad B=M_tJ_sM_{-t}J_{-s} \tag{15}

have symbols of weight one. The three interfaces therefore make them bounded on L2L^2. Their algebraic identities on S′\mathcal S' are

JsMtu=A(MtJsu),MtJsu=B(JsMtu).(16) \begin{aligned} J_sM_tu&=A(M_tJ_su),\\ M_tJ_su&=B(J_sM_tu). \end{aligned} \tag{16}

They prove both inequalities and both finite-norm implications. The bounded extensions agree with the distributional operators on L2L^2: approximate in L2L^2 by Schwartz inputs and use their continuous embeddings and distributional action.

For (14) conjugate by the defining isometries of the source and target:

Ca=Mt−τJs−μ a(x,D) J−sM−t.(17) C_a=M_{t-\tau}J_{s-\mu}\,a(x,D)\,J_{-s}M_{-t}. \tag{17}

Its product weight is

⟨x⟩t−τ⟨ξ⟩s−μ⟨x⟩τ⟨ξ⟩μ⟨ξ⟩−s⟨x⟩−t=1.(18) \langle x\rangle^{t-\tau}\langle\xi\rangle^{s-\mu} \langle x\rangle^\tau\langle\xi\rangle^\mu \langle\xi\rangle^{-s}\langle x\rangle^{-t}=1. \tag{18}

Consequently CaC_a is bounded on L2L^2 with the asserted finite-seminorm control. Apply it to MtJsuM_tJ_su, and use (4), to obtain ∥a(x,D)u∥s−μ,t−τ≤C∥u∥s,t\|a(x,D)u\|_{s-\mu,t-\tau}\le C\|u\|_{s,t}. Density, or the distributional identity in (17), gives the assertion on the whole space. □\square

For example the left symbol ⟨x⟩−ρ⟨ξ⟩μ\langle x\rangle^{-\rho}\langle\xi\rangle^\mu quantizes exactly as M−ρJμM_{-\rho}J_\mu, and maps

Hs,t⟶Hs−μ,t+ρ.(19) H^{s,t}\longrightarrow H^{s-\mu,t+\rho}. \tag{19}

Its decaying coefficient improves the permitted spatial weight by ρ\rho. This conclusion uses operator composition rather than a claim that the position and Fourier factors commute.

For nonnegative integer kk, the definition also has a familiar derivative form.

Corollary 3.2. For u∈S′u\in\mathcal S',

∥u∥k,t≍∑∣α∣≤k∥⟨x⟩tDαu∥2.(20) \|u\|_{k,t}\asymp \sum_{|\alpha|\le k}\|\langle x\rangle^tD^\alpha u\|_2. \tag{20}

In particular either side is finite exactly when the other is.

Proof. Set v=Mtuv=M_tu. The ordinary integer Sobolev norm is equivalent to ∑∣α∣≤k∥Dαv∥2\sum_{|\alpha|\le k}\|D^\alpha v\|_2, by Plancherel and comparison of ⟨ξ⟩2k\langle\xi\rangle^{2k} with the finite sum of ∣ξα∣2|\xi^\alpha|^2. Theorem 3.1 compares this norm with ∥u∥k,t\|u\|_{k,t}. In the distributional product rule every term of Dα(Mtu)D^\alpha(M_tu) is a bounded smooth multiple of MtDβuM_tD^\beta u, ∣β∣≤∣α∣|\beta|\le|\alpha|, by (3). Conversely, expand MtDα(M−tv)M_tD^\alpha(M_{-t}v); all the ratios MtDγ⟨x⟩−tM_tD^\gamma\langle x\rangle^{-t} are bounded, so each resulting term is controlled by a derivative of vv. These finite expansions prove the two bounds, including the finite-norm implications. □\square

Corollary 3.3 (Fourier exchange of decay and regularity). For every real s,ts,t, the unitary Fourier transform gives an isomorphism

F:Hs,t⟶Ht,s. \mathcal F:H^{s,t}\longrightarrow H^{t,s}.

Proof. On Schwartz inputs, Fourier inversion and the even bracket multipliers give F−1MsF=Js\mathcal F^{-1}M_s\mathcal F=J_s and F−1JtF=Mt\mathcal F^{-1}J_t\mathcal F=M_t. Consequently

∥Fu∥t,s=∥JsMtu∥2≍∥MtJsu∥2. \|\mathcal Fu\|_{t,s}=\|J_sM_tu\|_2 \asymp\|M_tJ_su\|_2.

Theorem 3.1 supplies the equivalence for every real pair, and the same argument for the inverse Fourier transform gives the reverse map. Density extends both maps and identifies them with the distributional Fourier transform. This proves the Fourier-exchange statement of [HJS], Proposition 3.10, with the factor order in our definition kept explicit. □\square

4. The rough elliptic estimate

We retain the full scalar coefficient class from the preceding domain theorem. Let n,m≥1n,m\ge1 be integers, P0(D)P_0(D) a real constant-coefficient elliptic operator of order mm, and

P=P0+∑∣α∣≤maα(x)Dα.(21) P=P_0+\sum_{|\alpha|\le m}a_\alpha(x)D^\alpha. \tag{21}

The highest-order aαa_\alpha are continuous and tend to zero at infinity. For k=m−∣α∣>0k=m-|\alpha|>0, the lower coefficient belongs to LlocpαL^{p_\alpha}_{\mathrm{loc}}, where

pα={n/k,n>2k,a fixed finite number greater than 2,n=2k,2,n<2k,∥aα∥Lpα(B(y,1))⟶0(∣y∣→∞).(22) p_\alpha= \begin{cases} n/k,&n>2k,\\ \text{a fixed finite number greater than }2,&n=2k,\\ 2,&n<2k, \end{cases} \qquad \|a_\alpha\|_{L^{p_\alpha}(B(y,1))}\longrightarrow0 \quad (|y|\to\infty). \tag{22}

Assume that the perturbation is symmetric on compact smooth tests and that the total continuous principal symbol is elliptic. Local membership is explicit; the tail limit by itself would not supply it. The preceding domain theorem makes PP self-adjoint with domain HmH^m; its graph estimate proves

∥v∥Hm≤C0(∥Pv∥2+∥v∥2),v∈Hm.(23) \|v\|_{H^m}\le C_0(\|Pv\|_2+\|v\|_2),\qquad v\in H^m. \tag{23}

Theorem 4.1. For every t∈Rt\in\mathbb R, if u∈Hmu\in H^m and the right side below is finite, then u∈Hm,tu\in H^{m,t} and

∥u∥m,t≤Ct(∥Pu∥0,t+∥u∥0,t).(24) \|u\|_{m,t}\le C_t\bigl(\|Pu\|_{0,t}+\|u\|_{0,t}\bigr). \tag{24}

The constant depends on the fixed operator and weight exponent. No derivatives of the rough coefficients and no prescribed rate of their decay are required.

This is an estimate on the known unweighted domain. It transfers a spatial weight from uu and PuPu to the highest derivatives. In particular it does not assert that every distributional solution already belongs to HmH^m. We prove it using bounded weights whose estimates stay uniform as their truncation is removed.

5. Uniform bounds for the regularized weight

For 0<ε≤10<\varepsilon\le1, define

Fε(x)=⟨x⟩(1+ε∣x∣2)1/2,wε(x)=Fε(x)t.(25) F_\varepsilon(x)= \frac{\langle x\rangle}{(1+\varepsilon|x|^2)^{1/2}}, \qquad w_\varepsilon(x)=F_\varepsilon(x)^t. \tag{25}

For each fixed ε\varepsilon, 1≤Fε≤ε−1/21\le F_\varepsilon\le\varepsilon^{-1/2}. Thus wεw_\varepsilon and its reciprocal are bounded smooth functions with bounded derivatives, though their zeroth-order bounds can depend on ε\varepsilon. Also wε(x)→⟨x⟩tw_\varepsilon(x)\to\langle x\rangle^t pointwise as ε↓0\varepsilon\downarrow0.

Lemma 5.1. For every multi-index γ\gamma,

∣Dγwε∣≤Ct,γwε⟨x⟩−∣γ∣,∣Dγwε−1∣≤Ct,γwε−1⟨x⟩−∣γ∣.(26) \begin{aligned} |D^\gamma w_\varepsilon|&\le C_{t,\gamma} w_\varepsilon\langle x\rangle^{-|\gamma|},\\ |D^\gamma w_\varepsilon^{-1}|&\le C_{t,\gamma} w_\varepsilon^{-1}\langle x\rangle^{-|\gamma|}. \end{aligned} \tag{26}

uniformly for 0<ε≤10<\varepsilon\le1. The weights wε±1w_\varepsilon^{\pm1} have common local comparison and temperateness constants for G1G_1.

Proof. Put bε=(1+ε∣x∣2)1/2b_\varepsilon=(1+\varepsilon|x|^2)^{1/2}. For ∣γ∣≥1|\gamma|\ge1, differentiation of log⁡⟨x⟩\log\langle x\rangle, followed by scaling x↦εxx\mapsto\sqrt\varepsilon x, gives

∣∂γlog⁡bε(x)∣≤Cγ(ε1+ε∣x∣2)∣γ∣/2≤Cγ⟨x⟩−∣γ∣.(27) |\partial^\gamma\log b_\varepsilon(x)| \le C_\gamma\left(\frac{\varepsilon}{1+\varepsilon|x|^2}\right)^{|\gamma|/2} \le C_\gamma\langle x\rangle^{-|\gamma|}. \tag{27}

For completeness the unscaled logarithmic estimate follows inductively by differentiating 12log⁡(1+∣x∣2)\tfrac12\log(1+|x|^2): its positive-order derivatives are finite sums of polynomials of degree at most twice the denominator power minus the derivative order, divided by powers of 1+∣x∣21+|x|^2. Each term has the claimed decay. The last inequality in (27) uses ε(1+∣x∣2)≤1+ε∣x∣2\varepsilon(1+|x|^2)\le1+\varepsilon|x|^2. The same bound holds for positive derivatives of log⁡wε=t(log⁡⟨x⟩−log⁡bε)\log w_\varepsilon=t(\log\langle x\rangle-\log b_\varepsilon). Repeatedly differentiate its exponential. Each resulting product of logarithmic derivatives has total derivative order ∣γ∣|\gamma|; division by wεw_\varepsilon leaves a bound C⟨x⟩−∣γ∣C\langle x\rangle^{-|\gamma|}. Apply the same argument to −log⁡wε-\log w_\varepsilon for the reciprocal.

The function bεb_\varepsilon is ε\sqrt\varepsilon-Lipschitz, and ε⟨x⟩≤bε(x)\sqrt\varepsilon\langle x\rangle\le b_\varepsilon(x). If ∣y−x∣≤r⟨x⟩|y-x|\le r\langle x\rangle, r<1/2r<1/2, the ratios of both ⟨y⟩/⟨x⟩\langle y\rangle/\langle x\rangle and bε(y)/bε(x)b_\varepsilon(y)/b_\varepsilon(x) lie between 1−r1-r and 1+r1+r. This proves uniform local comparison. Globally each of these ratios, and its reciprocal, is at most 1+∣x−y∣1+|x-y|. Hence

wε(y)wε(x),wε(x)wε(y)≤(1+∣x−y∣)2∣t∣.(28) \frac{w_\varepsilon(y)}{w_\varepsilon(x)}, \frac{w_\varepsilon(x)}{w_\varepsilon(y)} \le (1+|x-y|)^{2|t|}. \tag{28}

The dual distance for G1G_1 dominates ∣x−y∣2|x-y|^2, proving the uniform global condition. □\square

The symbols wεw_\varepsilon and wε−1w_\varepsilon^{-1}, independent of frequency, consequently form uniformly bounded families relative to their respective variable weights for G1G_1. In the factor-exchange proof (15), replace Mt,M−tM_t,M_{-t} by multiplication by these two functions. Their product weights still cancel to one, and all structural and normalized derivative constants remain uniform. Thus for each fixed ss,

∥wεJsu∥2≍∥Js(wεu)∥2,(29) \|w_\varepsilon J_su\|_2 \asymp \|J_s(w_\varepsilon u)\|_2, \tag{29}

with constants independent of ε\varepsilon. The large possible supremum of wεw_\varepsilon, or of its reciprocal, is not used in this bound.

6. Commutators without differentiating coefficients

Lemma 6.1. On HmH^m,

∥[P,wε]wε−1v∥2≤Ct∥v∥Hm−1,(30) \|[P,w_\varepsilon]w_\varepsilon^{-1}v\|_2 \le C_t\|v\|_{H^{m-1}}, \tag{30}

where the expression on the left extends continuously to Hm−1H^{m-1} and CtC_t is independent of ε\varepsilon.

Proof. Include the constant coefficients of P0P_0 among coefficients cαc_\alpha of PP. Since a scalar coefficient commutes with the weight, the product rule gives

[cαDα,wε]wε−1v=∑0<γ≤α(αγ)cα(Dγwε)Dα−γ(wε−1v).(31) \begin{aligned} &[c_\alpha D^\alpha,w_\varepsilon]w_\varepsilon^{-1}v\\ &\quad=\sum_{0<\gamma\le\alpha} \binom{\alpha}{\gamma}c_\alpha(D^\gamma w_\varepsilon) D^{\alpha-\gamma}(w_\varepsilon^{-1}v). \end{aligned} \tag{31}

Expand the last derivative. Every term has the form

Cαγη cαbγη,εDβv,bγη,ε=(Dγwε)(Dηwε−1),β=α−γ−η.(32) \begin{gathered} C_{\alpha\gamma\eta}\,c_\alpha b_{\gamma\eta,\varepsilon}D^\beta v,\\ b_{\gamma\eta,\varepsilon} =(D^\gamma w_\varepsilon)(D^\eta w_\varepsilon^{-1}),\\ \beta=\alpha-\gamma-\eta. \end{gathered} \tag{32}

By (26) its smooth ratio is uniformly bounded, in fact by C⟨x⟩−∣γ∣−∣η∣C\langle x\rangle^{-|\gamma|-|\eta|}. Neither expansion differentiates cαc_\alpha.

For a lower rough coefficient, with original gap k=m−∣α∣>0k=m-|\alpha|>0, the gap for DβvD^\beta v under the Hm−1H^{m-1} norm is

k′=(m−1)−∣β∣=k−1+∣γ∣+∣η∣≥k.(33) k'=(m-1)-|\beta|=k-1+|\gamma|+|\eta|\ge k. \tag{33}

The original LpαL^{p_\alpha} assumption suffices at this larger gap. To check every endpoint, the multiplier exponent for gap k′k' is n/k′>2n/k'>2 when n>2k′n>2k', any fixed finite exponent greater than 2 when n=2k′n=2k', and 2 when n<2k′n<2k'. In the first case n/k′≤pαn/k'\le p_\alpha; in the second choose an exponent no larger than pαp_\alpha, which is greater than 2 because k≤k′=n/2k\le k'=n/2; in the third use 2≤pα2\le p_\alpha. Finite-volume inclusion on unit balls supplies each smaller local exponent. Multiplication by the bounded ratio in (32) preserves these bounds.

Local membership and the tail hypothesis in (22) give a finite uniform unit-ball norm: far centers are bounded by the tail limit, and balls with centers in a fixed compact set lie in one larger compact set. The global coefficient multiplier estimate in Admissible differential perturbations, Proposition 2.1, now bounds every such term Hm−1→L2H^{m-1}\to L^2. Highest-order coefficients are bounded and ∣β∣≤m−1|\beta|\le m-1, so their terms are bounded directly by ∥v∥Hm−1\|v\|_{H^{m-1}}. The same direct argument handles all constant coefficients of P0P_0.

If m=1m=1, only terms with ∣α∣=1|\alpha|=1 contribute: the zeroth-order coefficients commute with the weight, and the remaining terms are bounded multipliers on L2=H0L^2=H^0. Thus this case does not require a positive-order multiplier theorem with order zero.

There are finitely many terms, all with uniform constants, proving (30). Initially the identities hold on compact smooth inputs. For fixed ε\varepsilon, multiplication by wε±1w_\varepsilon^{\pm1} is continuous on HmH^m, P:Hm→L2P:H^m\to L^2 is continuous, and compact smooth functions are dense in HmH^m. Passage to the limit proves the identity there. The term estimates also give its stated extension. □\square

Proof of Theorem 4.1. Set v=wεuv=w_\varepsilon u. It belongs to HmH^m for every fixed ε\varepsilon, and

Pv=wεPu+[P,wε]wε−1v.(34) Pv=w_\varepsilon Pu+[P,w_\varepsilon]w_\varepsilon^{-1}v. \tag{34}

Apply (23) and Lemma 6.1 to obtain

∥v∥Hm≤C0∥wεPu∥2+C1∥v∥Hm−1+C0∥v∥2,(35) \|v\|_{H^m}\le C_0\|w_\varepsilon Pu\|_2 +C_1\|v\|_{H^{m-1}}+C_0\|v\|_2, \tag{35}

with C1C_1 independent of ε\varepsilon. For any η>0\eta>0, splitting Fourier space at a sufficiently large fixed radius gives

∥v∥Hm−1≤η∥v∥Hm+Cη∥v∥2.(36) \|v\|_{H^{m-1}}\le\eta\|v\|_{H^m}+C_\eta\|v\|_2. \tag{36}

On the high-frequency part the ratio ⟨ξ⟩m−1/⟨ξ⟩m\langle\xi\rangle^{m-1}/\langle\xi\rangle^m is as small as needed; on the remaining ball ⟨ξ⟩m−1\langle\xi\rangle^{m-1} is bounded. This also proves (36) for m=1m=1. Choose η\eta so that C1η≤1/2C_1\eta\le1/2 and absorb. Then (29), with s=ms=m, yields

∥wεJmu∥2≤Ct(∥wεPu∥2+∥wεu∥2).(37) \|w_\varepsilon J_mu\|_2 \le C_t\bigl(\|w_\varepsilon Pu\|_2+\|w_\varepsilon u\|_2\bigr). \tag{37}

All constants here precede the limit in ε\varepsilon.

If t≥0t\ge0, wε≤⟨x⟩tw_\varepsilon\le\langle x\rangle^t, so the finite weighted right side gives integrable dominating squares. If t<0t<0, Fε≥1F_\varepsilon\ge1 gives wε≤1w_\varepsilon\le1, and u,Pu∈L2u,Pu\in L^2 provide dominating squares. In both cases dominated convergence makes the right side of (37) tend to the right side of (24). Since Jmu∈L2J_mu\in L^2, pointwise convergence of the weights and Fatou's inequality give

∥⟨x⟩tJmu∥2≤lim inf⁡ε↓0∥wεJmu∥2.(38) \|\langle x\rangle^tJ_mu\|_2 \le\liminf_{\varepsilon\downarrow0}\|w_\varepsilon J_mu\|_2. \tag{38}

This proves membership and (24). □\square

Combined with (20), the theorem controls every weighted derivative through order mm. Only the smooth auxiliary weights were differentiated. The coefficient class stays exactly the one needed for the unweighted domain theorem.

Use the conclusion

Compare the two orders of the weight and multiplier before applying a mapping theorem. Check that the rough graph estimate uses a known input regularity rather than assuming the conclusion being proved.

7. Graded exercises with complete solutions

Exercise 1 — Basic: equivalent norms can differ. Take s=t=2s=t=2. Compute the commutator of J2=1−ΔJ_2=1-\Delta and M2=1+∣x∣2M_2=1+|x|^2. Show on a Schwartz function that factor-order equivalence does not mean equality of operators.

Solution 1. Apply the ordinary Laplacian product rule:

[J2,M2]u=−4x⋅∇u−2nu.(39) [J_2,M_2]u=-4x\cdot\nabla u-2nu. \tag{39}

For u=e−∣x∣2u=e^{-|x|^2}, ∇u=−2xu\nabla u=-2xu, so the right side is (8∣x∣2−2n)e−∣x∣2(8|x|^2-2n)e^{-|x|^2}, which is not zero. Theorem 3.1 compares the two norms by bounded conjugated operators. It does not replace the product rule by commutation. The equality in (39) also makes explicit that the commutator has fewer derivatives than J2J_2.

Exercise 2 — Intermediate: a power tail at every integer order. For real a,ta,t and integer k≥0k\ge0, determine exactly when u=⟨x⟩−au=\langle x\rangle^{-a} belongs to Hk,tH^{k,t}. Include the equality case.

Solution 2. For ∣α∣≤k|\alpha|\le k, (3) gives ∣Dαu∣≤Cα⟨x⟩−a−∣α∣|D^\alpha u|\le C_\alpha\langle x\rangle^{-a-|\alpha|}. If a>t+n/2a>t+n/2, all these weighted derivatives are square integrable by radial integration, hence (20) gives u∈Hk,tu\in H^{k,t}. Conversely, (20) requires its zeroth derivative to belong to weighted L2L^2, whose exact condition is (5). At a=t+n/2a=t+n/2 the radial square integral behaves as ∫1∞r−1 dr\int_1^\infty r^{-1}\,dr, so it diverges. Thus the threshold is the same for every nonnegative integer kk. This reflects the extra decay of derivatives of this particular smooth tail; it is not a statement about arbitrary oscillating functions.

Exercise 3 — Intermediate: constants before a limit. In one dimension compute ∂xlog⁡wε\partial_x\log w_\varepsilon. Prove that its bound is uniform in ε\varepsilon, explain why the reciprocal has the same normalized derivative estimates, and decide which domination applies for positive and negative tt.

Solution 3. Direct differentiation of (25) gives

∂xlog⁡wε=t(x1+x2−εx1+εx2)=t(1−ε)x(1+x2)(1+εx2).(40) \partial_x\log w_\varepsilon =t\left(\frac{x}{1+x^2}-\frac{\varepsilon x}{1+\varepsilon x^2}\right) =\frac{t(1-\varepsilon)x}{(1+x^2)(1+\varepsilon x^2)}. \tag{40}

Its absolute value is at most ∣t∣⟨x⟩−1|t|\langle x\rangle^{-1}. Higher logarithmic derivatives have the uniform bound (27), for both terms in the difference. Differentiating an exponential expresses wε−1∂xjwεw_\varepsilon^{-1}\partial_x^j w_\varepsilon as a finite sum of products of these derivatives, with total order jj. Replacing tt by −t-t proves the reciprocal assertion.

Since 1≤Fε≤⟨x⟩1\le F_\varepsilon\le\langle x\rangle, positive tt gives wε≤⟨x⟩tw_\varepsilon\le\langle x\rangle^t, while negative tt gives wε≤1w_\varepsilon\le1. The former uses the assumed weighted norms of u,Puu,Pu for domination; the latter uses their already known unweighted L2L^2 norms. The possibly large supremum of wε−1w_\varepsilon^{-1} for negative tt is irrelevant to the normalized estimates and factor exchange.

Exercise 4 — Advanced: a rough coefficient loses no derivatives. In dimension four let a∈Lloc4a\in L^4_{\mathrm{loc}} have finite uniform unit-ball L4L^4 norm. It is a possible coefficient of D12D_1^2 in an order-three operator. Expand [aD12,wε]wε−1v[aD_1^2,w_\varepsilon]w_\varepsilon^{-1}v, and prove that it is bounded from H2H^2 to L2L^2 uniformly in ε\varepsilon, without any derivative of aa.

Solution 4. The expansion is

2a(D1wε)wε−1D1v+a((D12wε)wε−1+2(D1wε)(D1wε−1))v.(41) 2a(D_1w_\varepsilon)w_\varepsilon^{-1}D_1v +a\left((D_1^2w_\varepsilon)w_\varepsilon^{-1} +2(D_1w_\varepsilon)(D_1w_\varepsilon^{-1})\right)v. \tag{41}

The ratios are uniformly bounded by (26). The first term uses one derivative of vv, with remaining gap one under the H2H^2 norm. In dimension four the required coefficient exponent is 4/1=44/1=4, exactly the given one. For the zeroth-derivative term the remaining gap is two, the critical case n=2k′n=2k'; a finite exponent greater than 2 is allowed, so choose 4 again. The uniform local multiplication estimate therefore controls each term by a constant times ∥v∥H2\|v\|_{H^2}. Equivalently its local Hölder step pairs a∈L4a\in L^4 with the respective local L4L^4 functions D1vD_1v and vv, and its partition argument sums the estimates. No coefficient derivative appears: aa multiplies the product-rule expansion on the left. The larger gap in the second term only improves the available embedding.

Exercise 5 — Advanced: a spectral parameter and the indispensable lower norm. Under Theorem 4.1 suppose u∈Hmu\in H^m and (P−z)u=f(P-z)u=f, with f,u∈H0,tf,u\in H^{0,t}. Derive a weighted estimate for uu, uniform for zz in a fixed bounded set. Show that a term controlling uu cannot generally be deleted, already for the unweighted Laplacian.

Solution 5. The equation gives Pu=f+zuPu=f+zu, so (24) implies

∥u∥m,t≤Ct(∥f∥0,t+(1+∣z∣)∥u∥0,t).(42) \|u\|_{m,t} \le C_t\bigl(\|f\|_{0,t}+(1+|z|)\|u\|_{0,t}\bigr). \tag{42}

If ∣z∣≤R|z|\le R, the constant Ct(1+R)C_t(1+R) is uniform. This argument applies to real or complex zz; it does not assert an inverse or bound ∥u∥0,t\|u\|_{0,t} by ff.

For necessity of the lower norm, take P=−ΔP=-\Delta, t=0t=0, a nonzero ϕ∈Cc∞\phi\in C_c^\infty, and uR(x)=R−n/2ϕ(x/R)u_R(x)=R^{-n/2}\phi(x/R). Change of variables gives

∥uR∥2=∥ϕ∥2,∥PuR∥2=R−2∥Δϕ∥2,∥uR∥H2≥∥ϕ∥2.(43) \|u_R\|_2=\|\phi\|_2,\qquad \|Pu_R\|_2=R^{-2}\|\Delta\phi\|_2,\qquad \|u_R\|_{H^2}\ge\|\phi\|_2. \tag{43}

Let R→∞R\to\infty. A bound ∥u∥H2≤C∥Pu∥2\|u\|_{H^2}\le C\|Pu\|_2 would contradict these identities. The graph estimate retains its L2L^2 term because it controls frequencies near zero as well as the elliptic high-frequency part.

8. Reading and further directions

[L] Nicolas Lerner, Metrics on the Phase Space and Non-Selfadjoint Pseudo-Differential Operators, chapter on phase-space metrics, explains the metric calculus and the role of uncertainty and temperateness. Its quantization conventions should be compared with the D=−i∂D=-i\partial convention here. The linked course prerequisites give the precise interfaces used in this proof.

[A] Shmuel Agmon, Spectral properties of Schrödinger operators and scattering theory, 1975, Appendix A, Lemma A.3, equations (A.16)–(A.19), gives the constant-coefficient weighted-commutator proof. Sections 5–6 supply the rough-coefficient extension without differentiating those coefficients.

[K] Shige Toshi Kuroda, Scattering theory for differential operators, II, 1973, §2.4, uses a positive constant-coefficient form reference and a weighted derivative factor. Its bounded, strongly elliptic form coefficients are a different class from (21)–(22); the rough graph proof here supplies that distinction.

[AT] Shmuel Agmon, notes by Karl Gustafson, reworked by Michael Taylor, Limiting Absorption Principle for Long Range Potentials, Theorem 2.A, states the smooth weighted mapping rule without giving its proof. Theorem 3.1 above proves the factor exchange and mapping rule on every real scale using the complete programme calculus proof; Sections 5–6 then treat the additional rough coefficients.

[HJS] Andrew Hassell, Qiuye Jia and Ethan Sussman, Lecture notes on non-elliptic Fredholm theory, arXiv:2604.18956v1, Propositions 3.10–3.11, gives Fourier exchange and all-real mapping in the smooth scattering calculus. Corollary 3.3 integrates the former, while our metric proof and rough commutator argument handle the additional coefficient class.

The next question is how much differentiability can be recovered from a distributional solution away from its energy surface. The weighted mapping theorem supplies the norm estimates for a smooth inverse symbol. To allow an arbitrary initial spatial weight in the error term, a parametrix must have a remainder rapidly decreasing in both position and frequency. The present lesson proves the weighted scale and rough graph estimate; construction of that inverse and the estimates near the energy surface require further work.