Misplaced Pages

Singular integral operators of convolution type

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
(Redirected from Beurling transform) Mathematical concept

In mathematics, singular integral operators of convolution type are the singular integral operators that arise on R and T through convolution by distributions; equivalently they are the singular integral operators that commute with translations. The classical examples in harmonic analysis are the harmonic conjugation operator on the circle, the Hilbert transform on the circle and the real line, the Beurling transform in the complex plane and the Riesz transforms in Euclidean space. The continuity of these operators on L is evident because the Fourier transform converts them into multiplication operators. Continuity on L spaces was first established by Marcel Riesz. The classical techniques include the use of Poisson integrals, interpolation theory and the Hardy–Littlewood maximal function. For more general operators, fundamental new techniques, introduced by Alberto Calderón and Antoni Zygmund in 1952, were developed by a number of authors to give general criteria for continuity on L spaces. This article explains the theory for the classical operators and sketches the subsequent general theory.

L theory

Hilbert transform on the circle

See also: Harmonic conjugate

The theory for L functions is particularly simple on the circle. If fL(T), then it has a Fourier series expansion f ( θ ) = n Z a n e i n θ . {\displaystyle f(\theta )=\sum _{n\in \mathbf {Z} }a_{n}e^{in\theta }.}

Hardy space H(T) consists of the functions for which the negative coefficients vanish, an = 0 for n < 0. These are precisely the square-integrable functions that arise as boundary values of holomorphic functions in the open unit disk. Indeed, f is the boundary value of the function

F ( z ) = n 0 a n z n , {\displaystyle F(z)=\sum _{n\geq 0}a_{n}z^{n},}

in the sense that the functions

f r ( θ ) = F ( r e i θ ) , {\displaystyle f_{r}(\theta )=F(re^{i\theta }),}

defined by the restriction of F to the concentric circles |z| = r, satisfy

f r f 2 0. {\displaystyle \|f_{r}-f\|_{2}\rightarrow 0.}

The orthogonal projection P of L(T) onto H(T) is called the Szegő projection. It is a bounded operator on L(T) with operator norm 1. By Cauchy's theorem

F ( z ) = 1 2 π i | ζ | = 1 f ( ζ ) ζ z d ζ = 1 2 π π π f ( θ ) 1 e i θ z d θ . {\displaystyle F(z)={1 \over 2\pi i}\int _{|\zeta |=1}{\frac {f(\zeta )}{\zeta -z}}\,d\zeta ={1 \over 2\pi }\int _{-\pi }^{\pi }{f(\theta ) \over 1-e^{-i\theta }z}\,d\theta .}

Thus

F ( r e i φ ) = 1 2 π π π f ( φ θ ) 1 r e i θ d θ . {\displaystyle F(re^{i\varphi })={1 \over 2\pi }\int _{-\pi }^{\pi }{f(\varphi -\theta ) \over 1-re^{i\theta }}\,d\theta .}

When r = 1, the integrand on the right-hand side has a singularity at θ = 0. The truncated Hilbert transform is defined by

H ε f ( φ ) = i π ε | θ | π f ( φ θ ) 1 e i θ d θ = 1 π | ζ e i φ | δ f ( ζ ) ζ e i φ d ζ , {\displaystyle H_{\varepsilon }f(\varphi )={i \over \pi }\int _{\varepsilon \leq |\theta |\leq \pi }{f(\varphi -\theta ) \over 1-e^{i\theta }}\,d\theta ={1 \over \pi }\int _{|\zeta -e^{i\varphi }|\geq \delta }{f(\zeta ) \over \zeta -e^{i\varphi }}\,d\zeta ,}

where δ = |1 – e|. Since it is defined as convolution with a bounded function, it is a bounded operator on L(T). Now

H ε 1 = i π ε π 2 ( 1 e i θ ) 1 d θ = i π ε π 1 d θ = i i ε π . {\displaystyle H_{\varepsilon }{1}={i \over \pi }\int _{\varepsilon }^{\pi }2\Re (1-e^{i\theta })^{-1}\,d\theta ={i \over \pi }\int _{\varepsilon }^{\pi }1\,d\theta =i-{i\varepsilon \over \pi }.}

If f is a polynomial in z then

H ε f ( z ) i ( 1 ε ) π f ( z ) = 1 π i | ζ z | δ f ( ζ ) f ( z ) ζ z d ζ . {\displaystyle H_{\varepsilon }f(z)-{i(1-\varepsilon ) \over \pi }f(z)={1 \over \pi i}\int _{|\zeta -z|\geq \delta }{f(\zeta )-f(z) \over \zeta -z}\,d\zeta .}

By Cauchy's theorem the right-hand side tends to 0 uniformly as ε, and hence δ, tends to 0. So

H ε f i f {\displaystyle H_{\varepsilon }f\rightarrow if}

uniformly for polynomials. On the other hand, if u(z) = z it is immediate that

H ε f ¯ = u 1 H ε ( u f ¯ ) . {\displaystyle {\overline {H_{\varepsilon }f}}=-u^{-1}H_{\varepsilon }(u{\overline {f}}).}

Thus if f is a polynomial in z without constant term

H ε f i f {\displaystyle H_{\varepsilon }f\rightarrow -if} uniformly.

Define the Hilbert transform on the circle by H = i ( 2 P I ) . {\displaystyle H=i(2P-I).}

Thus if f is a trigonometric polynomial

H ε f H f {\displaystyle H_{\varepsilon }f\rightarrow Hf} uniformly.

It follows that if f is any L function

H ε f H f {\displaystyle H_{\varepsilon }f\rightarrow Hf} in the L norm.

This is an immediate consequence of the result for trigonometric polynomials once it is established that the operators Hε are uniformly bounded in operator norm. But on

( 1 e i θ ) 1 = [ ( 1 e i θ ) 1 i θ 1 ] + i θ 1 . {\displaystyle (1-e^{i\theta })^{-1}=+i\theta ^{-1}.}

The first term is bounded on the whole of , so it suffices to show that the convolution operators Sε defined by

S ε f ( φ ) = ε | θ | π f ( φ θ ) θ 1 d θ {\displaystyle S_{\varepsilon }f(\varphi )=\int _{\varepsilon \leq |\theta |\leq \pi }f(\varphi -\theta )\theta ^{-1}\,d\theta }

are uniformly bounded. With respect to the orthonormal basis e convolution operators are diagonal and their operator norms are given by taking the supremum of the moduli of the Fourier coefficients. Direct computation shows that these all have the form

1 π | a b sin t t d t | {\displaystyle {\frac {1}{\pi }}\left|\int _{a}^{b}{\sin t \over t}\,dt\right|}

with 0 < a < b. These integrals are well known to be uniformly bounded.

It also follows that, for a continuous function f on the circle, Hεf converges uniformly to Hf, so in particular pointwise. The pointwise limit is a Cauchy principal value, written

H f = P . V . 1 π f ( ζ ) ζ e i φ d ζ . {\displaystyle Hf=\mathrm {P.V.} \,{1 \over \pi }\int {f(\zeta ) \over \zeta -e^{i\varphi }}\,d\zeta .}

If f is just in L then Hεf converges to Hf pointwise almost everywhere. In fact define the Poisson operators on L functions by

T r ( a n e i n θ ) = r | n | a n e i n θ , {\displaystyle T_{r}\left(\sum a_{n}e^{in\theta }\right)=\sum r^{|n|}a_{n}e^{in\theta },}

for r < 1. Since these operators are diagonal, it is easy to see that Trf tends to f in L as r increases to 1. Moreover, as Lebesgue proved, Trf also tends pointwise to f at each Lebesgue point of f. On the other hand, it is also known that TrHfH1 − r f tends to zero at each Lebesgue point of f. Hence H1 – r f tends pointwise to f on the common Lebesgue points of f and Hf and therefore almost everywhere.

Results of this kind on pointwise convergence are proved more generally below for L functions using the Poisson operators and the Hardy–Littlewood maximal function of f.

The Hilbert transform has a natural compatibility with orientation-preserving diffeomorphisms of the circle. Thus if H is a diffeomorphism of the circle with

H ( e i θ ) = e i h ( θ ) , h ( θ + 2 π ) = h ( θ ) + 2 π , {\displaystyle H(e^{i\theta })=e^{ih(\theta )},\,\,\,h(\theta +2\pi )=h(\theta )+2\pi ,}

then the operators

H ε h f ( e i φ ) = 1 π | e i h ( θ ) e i h ( φ ) | ε f ( e i θ ) e i θ e i φ e i θ d θ , {\displaystyle H_{\varepsilon }^{h}f(e^{i\varphi })={\frac {1}{\pi }}\int _{|e^{ih(\theta )}-e^{ih(\varphi )}|\geq \varepsilon }{\frac {f(e^{i\theta })}{e^{i\theta }-e^{i\varphi }}}e^{i\theta }\,d\theta ,}

are uniformly bounded and tend in the strong operator topology to H. Moreover, if Vf(z) = f(H(z)), then VHVH is an operator with smooth kernel, so a Hilbert–Schmidt operator.

In fact if G is the inverse of H with corresponding function g(θ), then

( V H ε h V 1 H ε ) f ( e i φ ) = 1 π | e i θ e i φ | ε [ g ( θ ) e i g ( θ ) e i g ( θ ) e i g ( φ ) e i θ e i θ e i φ ] f ( e i θ ) d θ . {\displaystyle (VH_{\varepsilon }^{h}V^{-1}-H_{\varepsilon })f(e^{i\varphi })={1 \over \pi }\int _{|e^{i\theta }-e^{i\varphi }|\geq \varepsilon }\left\,f(e^{i\theta })\,d\theta .}

Since the kernel on the right hand side is smooth on T × T, it follows that the operators on the right hand side are uniformly bounded and hence so too are the operators Hε. To see that they tend strongly to H, it suffices to check this on trigonometric polynomials. In that case

H ε h f ( ζ ) = 1 π i | H ( z ) H ( ζ ) | ε f ( z ) z ζ d z = 1 π i | H ( z ) H ( ζ ) | ε f ( z ) f ( ζ ) z ζ d z + f ( ζ ) π i | H ( z ) H ( ζ ) | ε d z z ζ . {\displaystyle H_{\varepsilon }^{h}f(\zeta )={1 \over \pi i}\int _{|H(z)-H(\zeta )|\geq \varepsilon }{\frac {f(z)}{z-\zeta }}dz={1 \over \pi i}\int _{|H(z)-H(\zeta )|\geq \varepsilon }{f(z)-f(\zeta ) \over z-\zeta }\,dz+{\frac {f(\zeta )}{\pi i}}\int _{|H(z)-H(\zeta )|\geq \varepsilon }{dz \over z-\zeta }.}

In the first integral the integrand is a trigonometric polynomial in z and ζ and so the integral is a trigonometric polynomial in ζ. It tends in L to the trigonometric polynomial 1 π i f ( z ) f ( ζ ) z ζ d z . {\displaystyle {1 \over \pi i}\int {f(z)-f(\zeta ) \over z-\zeta }\,dz.}

The integral in the second term can be calculated by the principle of the argument. It tends in L to the constant function 1, so that

lim ε 0 H ε h f ( ζ ) = f ( ζ ) + 1 π i f ( z ) f ( ζ ) z ζ d z , {\displaystyle \lim _{\varepsilon \to 0}H_{\varepsilon }^{h}f(\zeta )=f(\zeta )+{1 \over \pi i}\int {f(z)-f(\zeta ) \over z-\zeta }\,dz,}

where the limit is in L. On the other hand, the right hand side is independent of the diffeomorphism. Since for the identity diffeomorphism, the left hand side equals Hf, it too equals Hf (this can also be checked directly if f is a trigonometric polynomial). Finally, letting ε → 0,

( V H V 1 H ) f ( e i φ ) = 1 π [ g ( θ ) e i g ( θ ) e i g ( θ ) e i g ( φ ) e i θ e i θ e i φ ] f ( e i θ ) d θ . {\displaystyle (VHV^{-1}-H)f(e^{i\varphi })={\frac {1}{\pi }}\int \left\,f(e^{i\theta })\,d\theta .}

The direct method of evaluating Fourier coefficients to prove the uniform boundedness of the operator H does not generalize directly to L spaces with 1 < p < ∞. Instead a direct comparison of Hf with the Poisson integral of the Hilbert transform is used classically to prove this. If f has Fourier series

f ( e i θ ) = n Z a n e i n θ , {\displaystyle f(e^{i\theta })=\sum _{n\in \mathbf {Z} }a_{n}e^{in\theta },}

its Poisson integral is defined by

P r f ( e i θ ) = n Z a n r | n | e i n θ = 1 2 π 0 2 π ( 1 r 2 ) f ( e i θ ) 1 2 r cos θ + r 2 d θ = K r f ( e i θ ) , {\displaystyle P_{r}f(e^{i\theta })=\sum _{n\in \mathbf {Z} }a_{n}r^{|n|}e^{in\theta }={1 \over 2\pi }\int _{0}^{2\pi }{(1-r^{2})f(e^{i\theta }) \over 1-2r\cos \theta +r^{2}}\,d\theta =K_{r}\star f(e^{i\theta }),}

where the Poisson kernel Kr is given by K r ( e i θ ) = n Z r | n | e i n θ = 1 r 2 1 2 r cos θ + r 2 . {\displaystyle K_{r}(e^{i\theta })=\sum _{n\in \mathbf {Z} }r^{|n|}e^{in\theta }={1-r^{2} \over 1-2r\cos \theta +r^{2}}.}

In f is in L(T) then the operators Pr satisfy P r f f p 0. {\displaystyle \|P_{r}f-f\|_{p}\rightarrow 0.}

In fact the Kr are positive so K r 1 = 1 2 π 0 2 π K r ( e i θ ) d θ = 1. {\displaystyle \|K_{r}\|_{1}={1 \over 2\pi }\int _{0}^{2\pi }K_{r}(e^{i\theta })\,d\theta =1.}

Thus the operators Pr have operator norm bounded by 1 on L. The convergence statement above follows by continuity from the result for trigonometric polynomials, where it is an immediate consequence of the formula for the Fourier coefficients of Kr.

The uniform boundedness of the operator norm of Hε follows because HPrH1−r is given as convolution by the function ψr, where ψ r ( e i θ ) = 1 + 1 r 1 + r cot ( θ 2 ) K r ( e i θ ) 1 + 1 r 1 + r cot ( 1 r 2 ) K r ( e i θ ) {\displaystyle {\begin{aligned}\psi _{r}(e^{i\theta })&=1+{\frac {1-r}{1+r}}\cot \left({\tfrac {\theta }{2}}\right)K_{r}(e^{i\theta })\\&\leq 1+{\frac {1-r}{1+r}}\cot \left({\tfrac {1-r}{2}}\right)K_{r}(e^{i\theta })\end{aligned}}} for 1 − r ≤ |θ| ≤ π, and, for |θ| < 1 − r, ψ r ( e i θ ) = 1 + 2 r sin θ 1 2 r cos θ + r 2 . {\displaystyle \psi _{r}(e^{i\theta })=1+{2r\sin \theta \over 1-2r\cos \theta +r^{2}}.}

These estimates show that the L norms ∫ |ψr| are uniformly bounded. Since H is a bounded operator, it follows that the operators Hε are uniformly bounded in operator norm on L(T). The same argument can be used on L(T) once it is known that the Hilbert transform H is bounded in operator norm on L(T).

Hilbert transform on the real line

See also: Hilbert transform

As in the case of the circle, the theory for L functions is particularly easy to develop. In fact, as observed by Rosenblum and Devinatz, the two Hilbert transforms can be related using the Cayley transform.

The Hilbert transform HR on L(R) is defined by H R f ^ = ( i χ [ 0 , ) i χ ( , 0 ] ) f ^ , {\displaystyle {\widehat {H_{\mathbf {R} }f}}=\left(i\chi _{}\right){\widehat {f}},} where the Fourier transform is given by f ^ ( t ) = 1 2 π f ( x ) e i t x d x . {\displaystyle {\widehat {f}}(t)={1 \over {\sqrt {2\pi }}}\int _{-\infty }^{\infty }f(x)e^{-itx}\,dx.}

Define the Hardy space H(R) to be the closed subspace of L(R) consisting of functions for which the Fourier transform vanishes on the negative part of the real axis. Its orthogonal complement is given by functions for which the Fourier transform vanishes on the positive part of the real axis. It is the complex conjugate of H(R). If PR is the orthogonal projection onto H(R), then

H R = i ( 2 P R I ) . {\displaystyle H_{\mathbf {R} }=i(2P_{\mathbf {R} }-I).}

The Cayley transform C ( x ) = x i x + i {\displaystyle C(x)={x-i \over x+i}} carries the extended real line onto the circle, sending the point at ∞ to 1, and the upper halfplane onto the unit disk.

Define the unitary operator from L(T) onto L(R) by U f ( x ) = π 1 / 2 ( x + i ) 1 f ( C ( x ) ) . {\displaystyle Uf(x)=\pi ^{-1/2}(x+i)^{-1}f(C(x)).}

This operator carries the Hardy space of the circle H(T) onto H(R). In fact for |w| < 1, the linear span of the functions f w ( z ) = 1 1 w z {\displaystyle f_{w}(z)={\frac {1}{1-wz}}} is dense in H(T). Moreover, U f w ( x ) = 1 π 1 ( 1 w ) ( x z ¯ ) {\displaystyle Uf_{w}(x)={\frac {1}{\sqrt {\pi }}}{\frac {1}{(1-w)(x-{\overline {z}})}}} where z = C 1 ( w ¯ ) . {\displaystyle z=C^{-1}({\overline {w}}).}

On the other hand, for zH, the linear span of the functions g z ( t ) = e i t z χ [ 0 , ) ( t ) {\displaystyle g_{z}(t)=e^{itz}\chi _{[0,\infty )}(t)} is dense in L((0,∞)). By the Fourier inversion formula, they are the Fourier transforms of h z ( x ) = g z ^ ( x ) = i 2 π ( x + z ) 1 , {\displaystyle h_{z}(x)={\widehat {g_{z}}}(-x)={i \over {\sqrt {2\pi }}}(x+z)^{-1},} so the linear span of these functions is dense in H(R). Since U carries the fw's onto multiples of the hz's, it follows that U carries H(T) onto H(R). Thus U H T U = H R . {\displaystyle UH_{\mathbf {T} }U^{*}=H_{\mathbf {R} }.}

In Nikolski (1986), part of the L theory on the real line and the upper halfplane is developed by transferring the results from the circle and the unit disk. The natural replacements for concentric circles in the disk are lines parallel to the real axis in H. Under the Cayley transform, these correspond to circles in the disk that are tangent to the unit circle at the point one. The behaviour of functions in H(T) on these circles is part of the theory of Carleson measures. However, the theory of singular integrals can be developed more easily by working directly on R.

H(R) consists exactly of L functions f that arise of boundary values of holomorphic functions on H in the following sense: f is in H provided that there is a holomorphic function F(z) on H such that the functions fy(x) = f(x + iy) for y > 0 are in L and fy tends to f in L as y → 0. In this case F is necessarily unique and given by Cauchy's integral formula:

F ( z ) = 1 2 π i f ( s ) s z d s . {\displaystyle F(z)={1 \over 2\pi i}\int _{-\infty }^{\infty }{f(s) \over s-z}\,ds.}

In fact, identifying H with L(0,∞) via the Fourier transform, for y > 0 multiplication by e on L(0,∞) induces a contraction semigroup Vy on H. Hence for f in L

1 2 π i f ( s ) s z d s = 1 2 π f ( s ) g z ^ ( s ) d s = 1 2 π f ^ ( s ) g z ( s ) d s = V y P f ( x ) . {\displaystyle {1 \over 2\pi i}\int _{-\infty }^{\infty }{f(s) \over s-z}\,ds={1 \over {\sqrt {2\pi }}}\int _{-\infty }^{\infty }f(s){\widehat {g_{z}}}(s)\,ds={1 \over {\sqrt {2\pi }}}\int _{-\infty }^{\infty }{\widehat {f}}(s)g_{z}(s)\,ds=V_{y}Pf(x).}

If f is in H, F(z) is holomorphic for Im z > 0, since the family of L functions gz depends holomorphically on z. Moreover, fy = Vyf tends to f in H since this is true for the Fourier transforms. Conversely if such an F exists, by Cauchy's integral theorem and the above identity applied to fy

f y + t = V t P f y {\displaystyle f_{y+t}=V_{t}Pf_{y}}

for t > 0. Letting t tend to 0, it follows that Pfy = fy, so that fy lies in H. But then so too does the limit f. Since V t f y = f y + t = V y f t , {\displaystyle V_{t}f_{y}=f_{y+t}=V_{y}f_{t},} uniqueness of F follows from f t = lim y 0 f y + t = lim y 0 V t f y = V t f . {\displaystyle f_{t}=\lim _{y\to 0}f_{y+t}=\lim _{y\to 0}V_{t}f_{y}=V_{t}f.}

For f in L, the truncated Hilbert transforms are defined by H ε , R f ( x ) = 1 π ε | y x | R f ( y ) x y d y = 1 π ε | y | R f ( x y ) y d y H ε f ( x ) = 1 π | y x | ε f ( y ) x y d y = 1 π | y | ε f ( x y ) y d y . {\displaystyle {\begin{aligned}H_{\varepsilon ,R}f(x)&={1 \over \pi }\int _{\varepsilon \leq |y-x|\leq R}{f(y) \over x-y}\,dy={1 \over \pi }\int _{\varepsilon \leq |y|\leq R}{f(x-y) \over y}\,dy\\H_{\varepsilon }f(x)&={1 \over \pi }\int _{|y-x|\geq \varepsilon }{f(y) \over x-y}\,dy={1 \over \pi }\int _{|y|\geq \varepsilon }{f(x-y) \over y}\,dy.\end{aligned}}}

The operators Hε,R are convolutions by bounded functions of compact support, so their operator norms are given by the uniform norm of their Fourier transforms. As before the absolute values have the form

1 2 π | a b 2 sin t t d t | . {\displaystyle {1 \over {\sqrt {2\pi }}}\left|\int _{a}^{b}{2\sin t \over t}\,dt\right|.}

with 0 < a < b, so the operators Hε,R are uniformly bounded in operator norm. Since Hε,Rf tends to Hεf in L for f with compact support, and hence for arbitrary f, the operators Hε are also uniformly bounded in operator norm.

To prove that Hε f tends to Hf as ε tends to zero, it suffices to check this on a dense set of functions. On the other hand,

H ε f ¯ = H ε ( f ¯ ) , {\displaystyle {\overline {H_{\varepsilon }f}}=-H_{\varepsilon }({\overline {f}}),}

so it suffices to prove that Hεf tends to if for a dense set of functions in H(R), for example the Fourier transforms of smooth functions g with compact support in (0,∞). But the Fourier transform f extends to an entire function F on C, which is bounded on Im(z) ≥ 0. The same is true of the derivatives of g. Up to a scalar these correspond to multiplying F(z) by powers of z. Thus F satisfies a Paley-Wiener estimate for Im(z) ≥ 0:

| F ( m ) ( z ) | K N , m ( 1 + | z | ) N {\displaystyle |F^{(m)}(z)|\leq K_{N,m}(1+|z|)^{-N}}

for any m, N ≥ 0. In particular, the integral defining Hεf(x) can be computed by taking a standard semicircle contour centered on x. It consists of a large semicircle with radius R and a small circle radius ε with the two portions of the real axis between them. By Cauchy's theorem, the integral round the contour is zero. The integral round the large contour tends to zero by the Paley-Wiener estimate. The integral on the real axis is the limit sought. It is therefore given as minus the limit on the small semicircular contour. But this is the limit of

1 π Γ F ( z ) z x d z . {\displaystyle {1 \over \pi }\int _{\Gamma }{F(z) \over z-x}\,dz.}

Where Γ is the small semicircular contour, oriented anticlockwise. By the usual techniques of contour integration, this limit equals if(x). In this case, it is easy to check that the convergence is dominated in L since

H ε f ( x ) = 1 π | y x | ε f ( y ) f ( x ) y x d y = 1 π | y x | ε 0 1 f ( x + t ( y x ) ) d t d y {\displaystyle H_{\varepsilon }f(x)={\frac {1}{\pi }}\int _{|y-x|\geq \varepsilon }{\frac {f(y)-f(x)}{y-x}}\,dy={\frac {1}{\pi }}\int _{|y-x|\geq \varepsilon }\int _{0}^{1}f^{\prime }(x+t(y-x))\,dt\,dy}

so that convergence is dominated by G ( x ) = 1 2 π 0 1 | f ( x + t y ) | d y {\displaystyle G(x)={\frac {1}{2\pi }}\int _{0}^{1}\int _{-\infty }^{\infty }|f^{\prime }(x+ty)|\,dy} which is in L by the Paley-Wiener estimate.

It follows that for f on L(R) H ε f H f . {\displaystyle H_{\varepsilon }f\rightarrow Hf.}

This can also be deduced directly because, after passing to Fourier transforms, Hε and H become multiplication operators by uniformly bounded functions. The multipliers for Hε tend pointwise almost everywhere to the multiplier for H, so the statement above follows from the dominated convergence theorem applied to the Fourier transforms.

As for the Hilbert transform on the circle, Hεf tends to Hf pointwise almost everywhere if f is an L function. In fact, define the Poisson operators on L functions by

T y f ( x ) = P y ( x t ) f ( t ) d t , {\displaystyle T_{y}f(x)=\int _{-\infty }^{\infty }P_{y}(x-t)f(t)\,dt,}

where the Poisson kernel is given by

P y ( x ) = y π ( x 2 + y 2 ) . {\displaystyle P_{y}(x)={\frac {y}{\pi (x^{2}+y^{2})}}.}

for y > 0. Its Fourier transform is P y ^ ( t ) = e y | t | , {\displaystyle {\widehat {P_{y}}}(t)=e^{-y|t|},}

from which it is easy to see that Tyf tends to f in L as y increases to 0. Moreover, as Lebesgue proved, Tyf also tends pointwise to f at each Lebesgue point of f. On the other hand, it is also known that TyHfHyf tends to zero at each Lebesgue point of f. Hence Hεf tends pointwise to f on the common Lebesgue points of f and Hf and therefore almost everywhere. The absolute values of the functions Tyff and TyHfHyf can be bounded pointwise by multiples of the maximal function of f.

As for the Hilbert transform on the circle, the uniform boundedness of the operator norms of Hε follows from that of the Tε if H is known to be bounded, since HTεHε is the convolution operator by the function

g ε ( x ) = { x π ( x 2 + ε 2 ) | x | ε x π ( x 2 + ε 2 ) 1 π x | x | > ε {\displaystyle g_{\varepsilon }(x)={\begin{cases}{\frac {x}{\pi (x^{2}+\varepsilon ^{2})}}&|x|\leq \varepsilon \\{\frac {x}{\pi (x^{2}+\varepsilon ^{2})}}-{\frac {1}{\pi x}}&|x|>\varepsilon \end{cases}}}

The L norms of these functions are uniformly bounded.

Riesz transforms in the complex plane

Main article: Riesz transform

The complex Riesz transforms R and R* in the complex plane are the unitary operators on L(C) defined as multiplication by z/|z| and its conjugate on the Fourier transform of an L function f:

R f ^ ( z ) = z ¯ | z | f ^ ( z ) , R f ^ ( z ) = z | z | f ^ ( z ) . {\displaystyle {\widehat {Rf}}(z)={{\overline {z}} \over |z|}{\widehat {f}}(z),\,\,\,{\widehat {R^{*}f}}(z)={z \over |z|}{\widehat {f}}(z).}

Identifying C with R, R and R* are given by

R = i R 1 + R 2 , R = i R 1 R 2 , {\displaystyle R=-iR_{1}+R_{2},\,\,\,R^{*}=-iR_{1}-R_{2},}

where R1 and R2 are the Riesz transforms on R defined below.

On L(C), the operator R and its integer powers are unitary. They can also be expressed as singular integral operators:

R k f ( w ) = lim ε 0 | z w | ε M k ( w z ) f ( z ) d x d y , {\displaystyle {R^{k}f(w)=\lim _{\varepsilon \to 0}\int _{|z-w|\geq \varepsilon }M_{k}(w-z)f(z)\,dx\,dy,}}

where M k ( z ) = k 2 π i k z k | z | k + 2 ( k 1 ) , M k ( z ) = M k ( z ) ¯ . {\displaystyle M_{k}(z)={k \over 2\pi i^{k}}{z^{k} \over |z|^{k+2}}\,\,\,\,(k\geq 1),\,\,\,\,M_{-k}(z)={\overline {M_{k}(z)}}.}

Defining the truncated higher Riesz transforms as R ε ( k ) f ( w ) = | z w | ε M k ( w z ) f ( z ) d x d y , {\displaystyle {R_{\varepsilon }^{(k)}f(w)=\int _{|z-w|\geq \varepsilon }M_{k}(w-z)f(z)\,dx\,dy,}} these operators can be shown to be uniformly bounded in operator norm. For odd powers this can be deduced by the method of rotation of Calderón and Zygmund, described below. If the operators are known to be bounded in operator norm it can also be deduced using the Poisson operators.

The Poisson operators Ts on R are defined for s > 0 by

T s f ( x ) = 1 2 π R 2 s f ( x ) ( | x t | 2 + s 2 ) 3 / 2 d t . {\displaystyle {T_{s}f(x)={1 \over 2\pi }\int _{\mathbf {R} ^{2}}{sf(x) \over (|x-t|^{2}+s^{2})^{3/2}}\,dt.}}

They are given by convolution with the functions

P s ( x ) = s 2 π ( | x | 2 + s 2 ) 3 / 2 . {\displaystyle {P_{s}(x)={s \over 2\pi (|x|^{2}+s^{2})^{3/2}}.}}

Ps is the Fourier transform of the function e, so under the Fourier transform they correspond to multiplication by these functions and form a contraction semigroup on L(R). Since Py is positive and integrable with integral 1, the operators Ts also define a contraction semigroup on each L space with 1 < p < ∞.

The higher Riesz transforms of the Poisson kernel can be computed:

R k P s ( z ) = k 2 π i k z k ( | z | 2 + s 2 ) k / 2 + 1 {\displaystyle {R^{k}P_{s}(z)={k \over 2\pi i^{k}}{z^{k} \over (|z|^{2}+s^{2})^{k/2+1}}}}

for k ≥ 1 and the complex conjugate for − k. Indeed, the right hand side is a harmonic function F(x,y,s) of three variable and for such functions

T s 1 F ( x , y , s 2 ) = F ( x , y , s 1 + s 2 ) . {\displaystyle {T_{s_{1}}F(x,y,s_{2})=F(x,y,s_{1}+s_{2}).}}

As before the operators

T ε R k R ε ( k ) {\displaystyle {T_{\varepsilon }R^{k}-R_{\varepsilon }^{(k)}}}

are given by convolution with integrable functions and have uniformly bounded operator norms. Since the Riesz transforms are unitary on L(C), the uniform boundedness of the truncated Riesz transforms implies that they converge in the strong operator topology to the corresponding Riesz transforms.

The uniform boundedness of the difference between the transform and the truncated transform can also be seen for odd k using the Calderón-Zygmund method of rotation. The group T acts by rotation on functions on C via U θ f ( z ) = f ( e i θ z ) . {\displaystyle {U_{\theta }f(z)=f(e^{i\theta }z).}}

This defines a unitary representation on L(C) and the unitary operators Rθ commute with the Fourier transform. If A is a bounded operator on L(R) then it defines a bounded operator A on L(C) simply by making A act on the first coordinate. With the identification L(R) = L(R) ⊗ L(R), A = AI. If φ is a continuous function on the circle then a new operator can be defined by B = 1 2 π 0 2 π φ ( θ ) U θ A ( 1 ) U θ d θ . {\displaystyle {B={1 \over 2\pi }\int _{0}^{2\pi }\varphi (\theta )U_{\theta }A^{(1)}U_{\theta }^{*}\,d\theta .}}

This definition is understood in the sense that ( B f , g ) = 1 2 π 0 2 π φ ( θ ) ( U θ A ( 1 ) U θ f , g ) d θ {\displaystyle {(Bf,g)={1 \over 2\pi }\int _{0}^{2\pi }\varphi (\theta )(U_{\theta }A^{(1)}U_{\theta }^{*}f,g)\,d\theta }}

for any f, g in L(C). It follows that B 1 2 π 0 2 π | φ ( θ ) | A d θ . {\displaystyle {\|B\|\leq {1 \over 2\pi }\int _{0}^{2\pi }|\varphi (\theta )|\cdot \|A\|\,d\theta .}}

Taking A to be the Hilbert transform H on L(R) or its truncation Hε, it follows that R = 1 2 π 0 2 π e i θ U θ H ( 1 ) U θ d θ , R ε = 1 2 π 0 2 π e i θ U θ H ε ( 1 ) U θ d θ . {\displaystyle {\begin{aligned}R&={1 \over 2\pi }\int _{0}^{2\pi }e^{-i\theta }U_{\theta }H^{(1)}U_{\theta }^{*}\,d\theta ,\\R_{\varepsilon }&={1 \over 2\pi }\int _{0}^{2\pi }e^{-i\theta }U_{\theta }H_{\varepsilon }^{(1)}U_{\theta }^{*}\,d\theta .\end{aligned}}}

Taking adjoints gives a similar formula for R* and its truncation. This gives a second way to verify estimates of the norms of R, R* and their truncations. It has the advantage of being applicable also for L spaces.

The Poisson operators can also be used to show that the truncated higher Riesz transforms of a function tend to the higher Riesz transform at the common Lebesgue points of the function and its transform. Indeed, (RTεRε)f → 0 at each Lebesgue point of f; while (RRTε)f → 0 at each Lebesgue point of Rf.

Beurling transform in the complex plane

See also: Beltrami equation

Since

z ¯ z = ( z ¯ | z | ) 2 , {\displaystyle {{\overline {z}} \over z}=\left({{\overline {z}} \over |z|}\right)^{2},}

the Beurling transform T on L is the unitary operator equal to R. This relation has been used classically in Vekua (1962) and Ahlfors (1966) to establish the continuity properties of T on L spaces. The results on the Riesz transform and its powers show that T is the limit in the strong operator topology of the truncated operators T ε f ( w ) = 1 π | z w | ε f ( z ) ( w z ) 2 d x d y . {\displaystyle T_{\varepsilon }f(w)=-{\frac {1}{\pi }}\iint _{|z-w|\geq \varepsilon }{\frac {f(z)}{(w-z)^{2}}}dxdy.}

Accordingly, Tf can be written as a Cauchy principal value integral:

T f ( w ) = 1 π P . V . f ( z ) ( w z ) 2 d x d y = 1 π lim ε 0 | z w | ε f ( z ) ( w z ) 2 d x d y . {\displaystyle Tf(w)=-{\frac {1}{\pi }}P.V.\iint {\frac {f(z)}{(w-z)^{2}}}dxdy=-{\frac {1}{\pi }}\lim _{\varepsilon \to 0}\iint _{|z-w|\geq \varepsilon }{\frac {f(z)}{(w-z)^{2}}}dx\,dy.}

From the description of T and T* on Fourier transforms, it follows that if f is smooth of compact support

T ( z f ) = z T ( f ) , T ( z ¯ f ) = z ¯ T ( f ) . {\displaystyle {\begin{aligned}T(\partial _{z}f)&=\partial _{z}T(f),\\T(\partial _{\overline {z}}f)&=\partial _{\overline {z}}T(f).\end{aligned}}}

Like the Hilbert transform in one dimension, the Beurling transform has a compatibility with conformal changes of coordinate. Let Ω be a bounded region in C with smooth boundary ∂Ω and let φ be a univalent holomorphic map of the unit disk D onto Ω extending to a smooth diffeomorphism of the circle onto ∂Ω. If χΩ is the characteristic function of Ω, the operator can χΩΩ defines an operator T(Ω) on L(Ω). Through the conformal map φ, it induces an operator, also denoted T(Ω), on L(D) which can be compared with T(D). The same is true of the truncations Tε(Ω) and Tε(D).

Let Uε be the disk |zw| < ε and V the region |φ(z) − φ(w)| < ε. On L(D) T ε ( Ω ) f ( w ) = 1 π D V ε [ φ ( w ) φ ( z ) ( φ ( z ) φ ( w ) ) 2 f ( z ) ] d x d y , T ε ( D ) f ( w ) = 1 π D U ε f ( z ) ( z w ) 2 d x d y , {\displaystyle {\begin{aligned}T_{\varepsilon }(\Omega )f(w)&=-{\frac {1}{\pi }}\iint _{D\backslash V_{\varepsilon }}\leftdx\,dy,\\T_{\varepsilon }(D)f(w)&=-{1 \over \pi }\iint _{D\backslash U_{\varepsilon }}{f(z) \over (z-w)^{2}}\,dx\,dy,\end{aligned}}}

and the operator norms of these truncated operators are uniformly bounded. On the other hand, if

T ε ( D ) f ( w ) = 1 π D V ε f ( z ) ( z w ) 2 d x d y , {\displaystyle T_{\varepsilon }^{\prime }(D)f(w)=-{1 \over \pi }\iint _{D\backslash V_{\varepsilon }}{\frac {f(z)}{(z-w)^{2}}}dx\,dy,}

then the difference between this operator and Tε(Ω) is a truncated operator with smooth kernel K(w,z):

K ( w , z ) = 1 π [ φ ( w ) φ ( z ) ( φ ( z ) φ ( w ) ) 2 1 ( z w ) 2 ] . {\displaystyle K(w,z)=-{1 \over \pi }\left.}

So the operators T′ε(D) must also have uniformly bounded operator norms. To see that their difference tends to 0 in the strong operator topology, it is enough to check this for f smooth of compact support in D. By Green's theorem

( T ε ( D ) T ε ( D ) ) f ( w ) = 1 π U ε z f ( z ) z w d x d y 1 π V ε z f ( z ) z w d x d y + 1 2 π i U ε f ( z ) z w d z ¯ 1 2 π i V ε f ( z ) z w d z ¯ . {\displaystyle \left(T_{\varepsilon }(D)-T_{\varepsilon }^{\prime }(D)\right)f(w)={\frac {1}{\pi }}\iint _{U_{\varepsilon }}{\partial _{z}f(z) \over z-w}dx\,dy-{1 \over \pi }\iint _{V_{\varepsilon }}{\partial _{z}f(z) \over z-w}dx\,dy+{1 \over 2\pi i}\int _{\partial U_{\varepsilon }}{\frac {f(z)}{z-w}}d{\overline {z}}-{\frac {1}{2\pi i}}\int _{\partial V_{\varepsilon }}{f(z) \over z-w}\,d{\overline {z}}.}

All four terms on the right hand side tend to 0. Hence the difference T(Ω) − T(D) is the Hilbert–Schmidt operator with kernel K.

For pointwise convergence there is simple argument due to Mateu & Verdera (2006) showing that the truncated integrals converge to Tf precisely at its Lebesgue points, that is almost everywhere. In fact T has the following symmetry property for f, gL(C)

( T f ) g = 1 π lim | z w | ε f ( w ) g ( z ) ( w z ) 2 = f ( T g ) . {\displaystyle \iint (Tf)g=-{1 \over \pi }\lim \int _{|z-w|\geq \varepsilon }{\frac {f(w)g(z)}{(w-z)^{2}}}=\iint f(Tg).}

On the other hand, if χ is the characteristic function of the disk D(z,ε) with centre z and radius ε, then

T χ ( w ) = ε 2 1 χ ( w ) ( w z ) 2 . {\displaystyle T\chi (w)=-\varepsilon ^{2}{\frac {1-\chi (w)}{(w-z)^{2}}}.}

Hence T ε ( f ) ( z ) = 1 π ε 2 f ( T χ ) = 1 π ε 2 ( T f ) χ = A v D ( z , ε ) T f . {\displaystyle T_{\varepsilon }(f)(z)={1 \over \pi \varepsilon ^{2}}\iint f(T\chi )={1 \over \pi \varepsilon ^{2}}\iint (Tf)\chi =\mathbf {Av} _{D(z,\varepsilon )}\,Tf.}

By the Lebesgue differentiation theorem, the right-hand side converges to Tf at the Lebesgue points of Tf.

Riesz transforms in higher dimensions

Main article: Riesz transform

For f in the Schwartz space of R, the jth Riesz transform is defined by

R j f ( x ) = c n lim ε 0 | y | ε f ( x y ) y j | y | n + 1 d y = c n n 1 j f ( x y ) 1 | y | n 1 d y , {\displaystyle R_{j}f(x)=c_{n}\lim _{\varepsilon \to 0}\int _{|y|\geq \varepsilon }f(x-y){y_{j} \over |y|^{n+1}}dy={\frac {c_{n}}{n-1}}\int \partial _{j}f(x-y){1 \over |y|^{n-1}}dy,}

where c n = Γ ( n + 1 2 ) π n + 1 2 . {\displaystyle c_{n}=\Gamma \left({\tfrac {n+1}{2}}\right)\pi ^{-{\frac {n+1}{2}}}.}

Under the Fourier transform:

R j f ^ ( t ) = i t j | t | f ^ ( t ) . {\displaystyle {\widehat {R_{j}f}}(t)={it_{j} \over |t|}{\widehat {f}}(t).}

Thus Rj corresponds to the operator ∂jΔ, where Δ = −∂1 − ⋯ −∂n denotes the Laplacian on R. By definition Rj is a bounded and skew-adjoint operator for the L norm and

R 1 2 + + R n 2 = I . {\displaystyle R_{1}^{2}+\cdots +R_{n}^{2}=-I.}

The corresponding truncated operators R j , ε f ( x ) = c n | y | ε f ( x y ) y j | y | n + 1 d y {\displaystyle R_{j,\varepsilon }f(x)=c_{n}\int _{|y|\geq \varepsilon }f(x-y){y_{j} \over |y|^{n+1}}dy} are uniformly bounded in the operator norm. This can either be proved directly or can be established by the Calderón−Zygmund method of rotations for the group SO(n). This expresses the operators Rj and their truncations in terms of the Hilbert transforms in one dimension and its truncations. In fact if G = SO(n) with normalised Haar measure and H is the Hilbert transform in the first coordinate, then

R j = G φ ( g ) g H ( 1 ) g 1 d g , R j , ε = G φ ( g ) g H ε ( 1 ) g 1 d g , R j , ε , R = G φ ( g ) g H ε , R ( 1 ) g 1 d g . {\displaystyle {\begin{aligned}R_{j}&=\int _{G}\varphi (g)gH^{(1)}g^{-1}\,dg,\\R_{j,\varepsilon }&=\int _{G}\varphi (g)gH_{\varepsilon }^{(1)}g^{-1}\,dg,\\R_{j,\varepsilon ,R}&=\int _{G}\varphi (g)gH_{\varepsilon ,R}^{(1)}g^{-1}\,dg.\end{aligned}}}

where φ(g) is the (1,j) matrix coefficient of g.

In particular for fL, RjfRjf in L. Moreover, Rjf tends to Rj almost everywhere. This can be proved exactly as for the Hilbert transform by using the Poisson operators defined on L(R) when R is regarded as the boundary of a halfspace in R. Alternatively it can be proved directly from the result for the Hilbert transform on R using the expression of Rj as an integral over G.

The Poisson operators Ty on R are defined for y > 0 by

T y f ( x ) = c n R n y f ( x ) ( | x t | 2 + y 2 ) n + 1 2 d t . {\displaystyle T_{y}f(x)=c_{n}\int _{\mathbf {R} ^{n}}{\frac {yf(x)}{\left(|x-t|^{2}+y^{2}\right)^{\frac {n+1}{2}}}}dt.}

They are given by convolution with the functions P y ( x ) = c n y ( | x | 2 + y 2 ) n + 1 2 . {\displaystyle P_{y}(x)=c_{n}{\frac {y}{\left(|x|^{2}+y^{2}\right)^{\frac {n+1}{2}}}}.}

Py is the Fourier transform of the function e, so under the Fourier transform they correspond to multiplication by these functions and form a contraction semigroup on L(R). Since Py is positive and integrable with integral 1, the operators Ty also define a contraction semigroup on each L space with 1 < p < ∞.

The Riesz transforms of the Poisson kernel can be computed

R j P ε ( x ) = c n x j ( | x | 2 + ε 2 ) n + 1 2 . {\displaystyle R_{j}P_{\varepsilon }(x)=c_{n}{\frac {x_{j}}{\left(|x|^{2}+\varepsilon ^{2}\right)^{\frac {n+1}{2}}}}.}

The operator RjTε is given by convolution with this function. It can be checked directly that the operators RjTεRj,ε are given by convolution with functions uniformly bounded in L norm. The operator norm of the difference is therefore uniformly bounded. We have (RjTεRj,ε)f → 0 at each Lebesgue point of f; while (RjRjTε)f → 0 at each Lebesgue point of Rjf. So Rj,εfRjf on the common Lebesgue points of f and Rjf.

L theory

Elementary proofs of M. Riesz theorem

The theorem of Marcel Riesz asserts that singular integral operators that are continuous for the L norm are also continuous in the L norm for 1 < p < ∞ and that the operator norms vary continuously with p.

Bochner's proof for Hilbert transform on the circle

Once it is established that the operator norms of the Hilbert transform on L(T) are bounded for even integers, it follows from the Riesz–Thorin interpolation theorem and duality that they are bounded for all p with 1 < p < ∞ and that the norms vary continuously with p. Moreover, the arguments with the Poisson integral can be applied to show that the truncated Hilbert transforms Hε are uniformly bounded in operator norm and converge in the strong operator topology to H.

It is enough to prove the bound for real trigonometric polynomials without constant term:

f ( e i θ ) = m = 1 N a m e i m θ + a m e i m θ , a m = a m ¯ . {\displaystyle f\left(e^{i\theta }\right)=\sum _{m=1}^{N}a_{m}e^{im\theta }+a_{-m}e^{-im\theta },\qquad a_{-m}={\overline {a_{m}}}.}

Since f + iHf is a polynomial in e without constant term

1 2 π 0 2 π ( f + i H f ) 2 n d θ = 0. {\displaystyle {\frac {1}{2\pi }}\int _{0}^{2\pi }(f+iHf)^{2n}\,d\theta =0.}

Hence, taking the real part and using Hölder's inequality:

H f 2 n 2 n k = 0 n 1 ( 2 n 2 k ) | ( ( H f ) 2 k , f 2 n 2 k ) | k = 0 n 1 ( 2 n 2 k ) H f 2 n 2 k f 2 n 2 n 2 k . {\displaystyle \|Hf\|_{2n}^{2n}\leq \sum _{k=0}^{n-1}{2n \choose 2k}\left|\left((Hf)^{2k},f^{2n-2k}\right)\right|\leq \sum _{k=0}^{n-1}{2n \choose 2k}\|Hf\|_{2n}^{2k}\cdot \|f\|_{2n}^{2n-2k}.}

So the M. Riesz theorem follows by induction for p an even integer and hence for all p with 1 < p < ∞.

Cotlar's proof for Hilbert transform on the line

Once it is established that the operator norms of the Hilbert transform on L(R) are bounded when p is a power of 2, it follows from the Riesz–Thorin interpolation theorem and duality that they are bounded for all p with 1 < p < ∞ and that the norms vary continuously with p. Moreover, the arguments with the Poisson integral can be applied to show that the truncated Hilbert transforms Hε are uniformly bounded in operator norm and converge in the strong operator topology to H.

It is enough to prove the bound when f is a Schwartz function. In that case the following identity of Cotlar holds:

( H f ) 2 = f 2 + 2 H ( f H ( f ) ) . {\displaystyle (Hf)^{2}=f^{2}+2H(fH(f)).}

In fact, write f = f+ + f according to the ±i eigenspaces of H. Since f ± iHf extend to holomorphic functions in the upper and lower half plane, so too do their squares. Hence

f 2 ( H f ) 2 = ( f + + f ) 2 + ( f + f ) 2 = 2 ( f + 2 + f 2 ) = 2 i H ( f + 2 f 2 ) = 2 H ( f ( H f ) ) . {\displaystyle f^{2}-(Hf)^{2}=\left(f_{+}+f_{-}\right)^{2}+\left(f_{+}-f_{-}\right)^{2}=2\left(f_{+}^{2}+f_{-}^{2}\right)=-2iH\left(f_{+}^{2}-f_{-}^{2}\right)=-2H(f(Hf)).}

(Cotlar's identity can also be verified directly by taking Fourier transforms.)

Hence, assuming the M. Riesz theorem for p = 2,

H f 2 n + 1 2 = ( H f ) 2 2 n f 2 2 n + 2 H ( f H ( f ) ) 2 n f 2 n + 1 2 + 2 H 2 n f 2 n + 1 H f 2 n + 1 . {\displaystyle \|Hf\|_{2^{n+1}}^{2}=\left\|(Hf)^{2}\right\|_{2^{n}}\leq \left\|f^{2}\right\|_{2^{n}}+2\|H(fH(f))\|_{2^{n}}\leq \|f\|_{2^{n+1}}^{2}+2\|H\|_{2^{n}}\|f\|_{2^{n+1}}\|Hf\|_{2^{n+1}}.}

Since

R 2 > 1 + 2 H 2 n R {\displaystyle R^{2}>1+2\|H\|_{2^{n}}R}

for R sufficiently large, the M. Riesz theorem must also hold for p = 2.

Exactly the same method works for the Hilbert transform on the circle. The same identity of Cotlar is easily verified on trigonometric polynomials f by writing them as the sum of the terms with non-negative and negative exponents, i.e. the ±i eigenfunctions of H. The L bounds can therefore be established when p is a power of 2 and follow in general by interpolation and duality.

Calderón–Zygmund method of rotation

The method of rotation for Riesz transforms and their truncations applies equally well on L spaces for 1 < p < ∞. Thus these operators can be expressed in terms of the Hilbert transform on R and its truncations. The integration of the functions Φ from the group T or SO(n) into the space of operators on L is taken in the weak sense:

( G Φ ( x ) d x f , g ) = G ( Φ ( x ) f , g ) d x {\displaystyle \left(\int _{G}\Phi (x)\,dx\,f,g\right)=\int _{G}(\Phi (x)f,g)\,dx}

where f lies in L and g lies in the dual space L with ⁠1/p⁠ + ⁠1/q⁠. It follows that Riesz transforms are bounded on L and that the differences with their truncations are also uniformly bounded. The continuity of the L norms of a fixed Riesz transform is a consequence of the Riesz–Thorin interpolation theorem.

Pointwise convergence

See also: Fatou's theorem

The proofs of pointwise convergence for Hilbert and Riesz transforms rely on the Lebesgue differentiation theorem, which can be proved using the Hardy-Littlewood maximal function. The techniques for the simplest and best-known case, namely the Hilbert transform on the circle, are a prototype for all the other transforms. This case is explained in detail here.

Let f be in L(T) for p > 1. The Lebesgue differentiation theorem states that

A ( ε ) = 1 2 ε x ε x + ε | f ( t ) f ( x ) | d t 0 {\displaystyle {A(\varepsilon )={1 \over 2\varepsilon }\int _{x-\varepsilon }^{x+\varepsilon }|f(t)-f(x)|\,dt\to 0}}

for almost all x in T. The points at which this holds are called the Lebesgue points of f. Using this theorem it follows that if f is an integrable function on the circle, the Poisson integral Trf tends pointwise to f at each Lebesgue point of f. In fact, for x fixed, A(ε) is a continuous function on [0,π]. Continuity at 0 follows because x is a Lebesgue point and elsewhere because, if h is an integrable function, the integral of |h| on intervals of decreasing length tends to 0 by Hölder's inequality.

Letting r = 1 − ε, the difference can be estimated by two integrals:

2 π | T r f ( x ) f ( x ) | = 0 2 π | ( f ( x y ) f ( x ) ) P r ( y ) | d y | y | ε + | y | ε . {\displaystyle 2\pi |T_{r}f(x)-f(x)|=\int _{0}^{2\pi }|(f(x-y)-f(x))P_{r}(y)|\,dy\leq \int _{|y|\leq \varepsilon }+\int _{|y|\geq \varepsilon }.}

The Poisson kernel has two important properties for ε small

sup y [ ε , ε ] | P 1 ε ( y ) | ε 1 . sup y ( ε , ε ) | P 1 ε ( y ) | 0. {\displaystyle {\begin{aligned}\sup _{y\in }|P_{1-\varepsilon }(y)|&\leq \varepsilon ^{-1}.\\\sup _{y\notin (-\varepsilon ,\varepsilon )}|P_{1-\varepsilon }(y)|&\to 0.\end{aligned}}}

The first integral is bounded by A(ε) by the first inequality so tends to zero as ε goes to 0; the second integral tends to 0 by the second inequality.

The same reasoning can be used to show that T1 − εHfHεf tends to zero at each Lebesgue point of f. In fact the operator T1 − εHf has kernel Qr + i, where the conjugate Poisson kernel Qr is defined by Q r ( θ ) = 2 r sin θ 1 2 r cos θ + r 2 . {\displaystyle {Q_{r}(\theta )={2r\sin \theta \over 1-2r\cos \theta +r^{2}}.}}

Hence 2 π | T 1 ε H f ( x ) H ε f ( x ) | | y | ε | f ( x y ) f ( x ) | | Q r ( y ) | d y + | y | ε | f ( x y ) f ( x ) | | Q 1 ( y ) Q r ( y ) | d y . {\displaystyle {2\pi |T_{1-\varepsilon }Hf(x)-H_{\varepsilon }f(x)|\leq \int _{|y|\leq \varepsilon }|f(x-y)-f(x)|\cdot |Q_{r}(y)|\,dy+\int _{|y|\geq \varepsilon }|f(x-y)-f(x)|\cdot |Q_{1}(y)-Q_{r}(y)|\,dy.}}

The conjugate Poisson kernel has two important properties for ε small sup y [ ε , ε ] | Q 1 ε ( y ) | ε 1 . sup y ( ε , ε ) | Q 1 ( y ) Q 1 ε ( y ) | 0. {\displaystyle {\begin{aligned}\sup _{y\in }|Q_{1-\varepsilon }(y)|&\leq \varepsilon ^{-1}.\\\sup _{y\notin (-\varepsilon ,\varepsilon )}|Q_{1}(y)-Q_{1-\varepsilon }(y)|&\to 0.\end{aligned}}}

Exactly the same reasoning as before shows that the two integrals tend to 0 as ε → 0.

Combining these two limit formulas it follows that Hεf tends pointwise to Hf on the common Lebesgue points of f and Hf and therefore almost everywhere.

Maximal functions

See also: Hardy–Littlewood maximal function

Much of the L theory has been developed using maximal functions and maximal transforms. This approach has the advantage that it also extends to L spaces in an appropriate "weak" sense and gives refined estimates in L spaces for p > 1. These finer estimates form an important part of the techniques involved in Lennart Carleson's solution in 1966 of Lusin's conjecture that the Fourier series of L functions converge almost everywhere. In the more rudimentary forms of this approach, the L theory is given less precedence: instead there is more emphasis on the L theory, in particular its measure-theoretic and probabilistic aspects; results for other L spaces are deduced by a form of interpolation between L and L spaces. The approach is described in numerous textbooks, including the classics Zygmund (1977) and Katznelson (1968). Katznelson's account is followed here for the particular case of the Hilbert transform of functions in L(T), the case not covered by the development above. F. Riesz's proof of convexity, originally established by Hardy, is established directly without resorting to Riesz−Thorin interpolation.

If f is an L function on the circle its maximal function is defined by

f ( t ) = sup 0 < h π 1 2 h t h t + h | f ( s ) | d s . {\displaystyle {f^{*}(t)=\sup _{0<h\leq \pi }{1 \over 2h}\int _{t-h}^{t+h}|f(s)|\,ds.}}

f* is finite almost everywhere and is of weak L type. In fact for λ > 0 if

E f ( λ ) = { x : | f ( x ) | > λ } , f λ = χ E ( λ ) f , {\displaystyle {E_{f}(\lambda )=\{x:\,|f(x)|>\lambda \},\,\,f_{\lambda }=\chi _{E(\lambda )}f,}}

then

m ( E f ( λ ) ) 8 λ E f ( λ ) | f | 8 f 1 λ , {\displaystyle m(E_{f^{*}}(\lambda ))\leq {8 \over \lambda }\int _{E_{f}(\lambda )}|f|\leq {8\|f\|_{1} \over \lambda },}

where m denotes Lebesgue measure.

The Hardy−Littlewood inequality above leads to a proof that almost every point x of T is a Lebesgue point of an integrable function f, so that

lim h 0 x h x + h | f ( t ) f ( x ) | d t 2 h 0. {\displaystyle \lim _{h\to 0}{\frac {\int _{x-h}^{x+h}|f(t)-f(x)|\,dt}{2h}}\to 0.}

In fact, let

ω ( f ) ( x ) = lim sup h 0 x h x + h | f ( t ) f ( x ) | d t 2 h f ( x ) + | f ( x ) | . {\displaystyle \omega (f)(x)=\limsup _{h\to 0}{\frac {\int _{x-h}^{x+h}|f(t)-f(x)|\,dt}{2h}}\leq f^{*}(x)+|f(x)|.}

If g is continuous, then the ω(g) =0, so that ω(fg) = ω(f). On the other hand, f can be approximated arbitrarily closely in L by continuous g. Then, using Chebychev's inequality,

m { x : ω ( f ) ( x ) > λ } = m { x : ω ( f g ) ( x ) > λ } m { x : ( f g ) ( x ) > λ } + m { x : | f ( x ) g ( x ) | > λ } C λ 1 f g 1 . {\displaystyle m\{x:\,\omega (f)(x)>\lambda \}=m\{x:\,\omega (f-g)(x)>\lambda \}\leq m\{x:\,(f-g)^{*}(x)>\lambda \}+m\{x:\,|f(x)-g(x)|>\lambda \}\leq C\lambda ^{-1}\|f-g\|_{1}.}

The right-hand side can be made arbitrarily small, so that ω(f) = 0 almost everywhere.

The Poisson integrals of an L function f satisfy

| T r f | f . {\displaystyle {|T_{r}f|\leq f^{*}.}}

It follows that Tr f tends to f pointwise almost everywhere. In fact let

Ω ( f ) = lim sup r 1 | T r f f | . {\displaystyle {\Omega (f)=\limsup _{r\to 1}|T_{r}f-f|.}}

If g is continuous, then the difference tends to zero everywhere, so Ω(fg) = Ω(f). On the other hand, f can be approximated arbitrarily closely in L by continuous g. Then, using Chebychev's inequality,

m { x : Ω ( f ) ( x ) > λ } = m { x : Ω ( f g ) ( x ) > λ } m { x : ( f g ) ( x ) > λ } + m { x : | f ( x ) g ( x ) | > λ } C λ 1 f g 1 . {\displaystyle m\{x:\,\Omega (f)(x)>\lambda \}=m\{x:\,\Omega (f-g)(x)>\lambda \}\leq m\{x:\,(f-g)^{*}(x)>\lambda \}+m\{x:\,|f(x)-g(x)|>\lambda \}\leq C\lambda ^{-1}\|f-g\|_{1}.}

The right-hand side can be made arbitrarily small, so that Ω(f) = 0 almost everywhere. A more refined argument shows that convergence occurs at each Lebesgue point of f.

If f is integrable the conjugate Poisson integrals are defined and given by convolution by the kernel Qr. This defines Hf inside |z| < 1. To show that Hf has a radial limit for almost all angles, consider

F ( z ) = exp ( f ( z ) i H f ( z ) ) , {\displaystyle {F(z)=\exp(-f(z)-iHf(z)),}}

where f(z) denotes the extension of f by Poisson integral. F is holomorphic in the unit disk with |F(z)| ≤ 1. The restriction of F to a countable family of concentric circles gives a sequence of functions in L(T) which has a weak g limit in L(T) with Poisson integral F. By the L results, g is the radial limit for almost all angles of F. It follows that Hf(z) has a radial limit almost everywhere. This is taken as the definition of Hf on T, so that TrH f tends pointwise to H almost everywhere. The function Hf is of weak L type.

The inequality used above to prove pointwise convergence for L function with 1 < p < ∞ make sense for L functions by invoking the maximal function. The inequality becomes

| H ε f T 1 ε H f | 4 f . {\displaystyle {|H_{\varepsilon }f-T_{1-\varepsilon }Hf|\leq 4f^{*}.}}

Let

ω ( f ) = lim sup ε 0 | H ε f T 1 ε H f | . {\displaystyle {\omega (f)=\limsup _{\varepsilon \to 0}|H_{\varepsilon }f-T_{1-\varepsilon }Hf|.}}

If g is smooth, then the difference tends to zero everywhere, so ω(fg) = ω(f). On the other hand, f can be approximated arbitrarily closely in L by smooth g. Then

m { x : ω ( f ) ( x ) > λ } = m { x : ω ( f g ) ( x ) > λ } m { x : 4 ( f g ) ( x ) > λ } C λ 1 f g 1 . {\displaystyle m\{x:\,\omega (f)(x)>\lambda \}=m\{x:\,\omega (f-g)(x)>\lambda \}\leq m\{x:\,4(f-g)^{*}(x)>\lambda \}\leq C\lambda ^{-1}\|f-g\|_{1}.}

The right hand side can be made arbitrarily small, so that ω(f) = 0 almost everywhere. Thus the difference for f tends to zero almost everywhere. A more refined argument can be given to show that, as in case of L, the difference tends to zero at all Lebesgue points of f. In combination with the result for the conjugate Poisson integral, it follows that, if f is in L(T), then Hεf converges to Hf almost everywhere, a theorem originally proved by Privalov in 1919.

General theory

Calderón & Zygmund (1952) introduced general techniques for studying singular integral operators of convolution type. In Fourier transform the operators are given by multiplication operators. These will yield bounded operators on L if the corresponding multiplier function is bounded. To prove boundedness on L spaces, Calderón and Zygmund introduced a method of decomposing L functions, generalising the rising sun lemma of F. Riesz. This method showed that the operator defined a continuous operator from L to the space of functions of weak L. The Marcinkiewicz interpolation theorem and duality then implies that the singular integral operator is bounded on all L for 1 < p < ∞. A simple version of this theory is described below for operators on R. As de Leeuw (1965) showed, results on R can be deduced from corresponding results for T by restricting the multiplier to the integers, or equivalently periodizing the kernel of the operator. Corresponding results for the circle were originally established by Marcinkiewicz in 1939. These results generalize to R and T. They provide an alternative method for showing that the Riesz transforms, the higher Riesz transforms and in particular the Beurling transform define bounded operators on L spaces.

Calderón-Zygmund decomposition

See also: Rising sun lemma and Calderón–Zygmund lemma

Let f be a non-negative integrable or continuous function on . Let I = (a,b). For any open subinterval J of , let fJ denote the average of |f| over J. Let α be a positive constant greater than fI. Divide I into two equal intervals (omitting the midpoint). One of these intervals must satisfy fJ < α since their sum is 2fI so less than 2α. Otherwise the interval will satisfy α ≤ fJ < 2α. Discard such intervals and repeat the halving process with the remaining interval, discarding intervals using the same criterion. This can be continued indefinitely. The discarded intervals are disjoint and their union is an open set Ω. For points x in the complement, they lie in a nested set of intervals with lengths decreasing to 0 and on each of which the average of f is bounded by α. If f is continuous these averages tend to |f(x)|. If f is only integrable this is only true almost everywhere, for it is true at the Lebesgue points of f by the Lebesgue differentiation theorem. Thus f satisfies |f(x)| ≤ α almost everywhere on Ω, the complement of Ω. Let Jn be the set of discarded intervals and define the "good" function g by

g ( x ) = χ J n ( f ) ( x J n ) , g ( x ) = f ( x ) ( x Ω c ) . {\displaystyle {g(x)=\chi _{J_{n}}(f)\,\,\,(x\in J_{n}),\,\,\,\,\,g(x)=f(x)\,\,\,(x\in \Omega ^{c}).}}

By construction |g(x)| ≤ 2α almost everywhere and g 1 f 1 . {\displaystyle {\|g\|_{1}\leq \|f\|_{1}.}}

Combining these two inequalities gives g p p ( 2 α ) p 1 f 1 . {\displaystyle {\|g\|_{p}^{p}\leq (2\alpha )^{p-1}\|f\|_{1}.}}

Define the "bad" function b by b = fg. Thus b is 0 off Ω and equal to f minus its average on Jn. So the average of b on Jn is zero and b 1 2 f 1 . {\displaystyle {\|b\|_{1}\leq 2\|f\|_{1}.}}

Moreover, since |b| ≥ α on Ω m ( Ω ) α 1 f 1 . {\displaystyle {m(\Omega )\leq \alpha ^{-1}\|f\|_{1}.}}

The decomposition f ( x ) = g ( x ) + b ( x ) {\displaystyle \displaystyle {f(x)=g(x)+b(x)}}

is called the Calderón–Zygmund decomposition.

Multiplier theorem

See also: Multiplier (Fourier analysis) and Marcinkiewicz interpolation theorem

Let K(x) be a kernel defined on R\{0} such that

W ( f ) = lim ε 0 | x | ε K ( x ) f ( x ) d x {\displaystyle W(f)=\lim _{\varepsilon \to 0}\int _{|x|\geq \varepsilon }K(x)f(x)\,dx}

exists as a tempered distribution for f a Schwartz function. Suppose that the Fourier transform of T is bounded, so that convolution by W defines a bounded operator T on L(R). Then if K satisfies Hörmander's condition

A = sup y 0 | x | 2 | y | | K ( x y ) K ( x ) | d x < , {\displaystyle A=\sup _{y\neq 0}\int _{|x|\geq 2|y|}|K(x-y)-K(x)|\,dx<\infty ,}

then T defines a bounded operator on L for 1 < p < ∞ and a continuous operator from L into functions of weak type L.

In fact by the Marcinkiewicz interpolation argument and duality, it suffices to check that if f is smooth of compact support then

m { x : | T f ( x ) | 2 λ } ( 2 A + 4 T ) λ 1 f 1 . {\displaystyle m\{x:\,|Tf(x)|\geq 2\lambda \}\leq (2A+4\|T\|)\cdot \lambda ^{-1}\|f\|_{1}.}

Take a Calderón−Zygmund decomposition of f as above f ( x ) = g ( x ) + b ( x ) {\displaystyle f(x)=g(x)+b(x)} with intervals Jn and with α = λμ, where μ > 0. Then

m { x : | T f ( x ) | 2 λ } m { x : | T g ( x ) | λ } + m { x : | T b ( x ) | λ } . {\displaystyle m\{x:\,|Tf(x)|\geq 2\lambda \}\leq m\{x:\,|Tg(x)|\geq \lambda \}+m\{x:\,|Tb(x)|\geq \lambda \}.}

The term for g can be estimated using Chebychev's inequality:

m { x : | T g ( x ) | 2 λ } λ 2 T g 2 2 λ 2 T 2 g 2 2 2 λ 1 μ T 2 f 1 . {\displaystyle m\{x:\,|Tg(x)|\geq 2\lambda \}\leq \lambda ^{-2}\|Tg\|_{2}^{2}\leq \lambda ^{-2}\|T\|^{2}\|g\|_{2}^{2}\leq 2\lambda ^{-1}\mu \|T\|^{2}\|f\|_{1}.}

If J* is defined to be the interval with the same centre as J but twice the length, the term for b can be broken up into two parts:

m { x : | T b ( x ) | λ } m { x : x J n , | T b ( x ) | λ } + m ( J n ) . {\displaystyle m\{x:\,|Tb(x)|\geq \lambda \}\leq m\{x:\,x\notin \cup J_{n}^{*},\,\,\,|Tb(x)|\geq \lambda \}+m(\cup J_{n}^{*}).}

The second term is easy to estimate:

m ( J n ) m ( J n ) = 2 m ( J n ) 2 λ 1 μ 1 f 1 . {\displaystyle m(\cup J_{n}^{*})\leq \sum m(J_{n}^{*})=2\sum m(J_{n})\leq 2\lambda ^{-1}\mu ^{-1}\|f\|_{1}.}

To estimate the first term note that

b = b n , b n = ( f A v J n ( f ) ) χ J n . {\displaystyle b=\sum b_{n},\qquad b_{n}=(f-\mathbf {Av} _{J_{n}}(f))\chi _{J_{n}}.}

Thus by Chebychev's inequality:

m { x : x J m , | T b ( x ) | λ } λ 1 ( J m ) c | T b ( x ) | d x λ 1 n ( J n ) c | T b n ( x ) | d x . {\displaystyle m\{x:\,x\notin \cup J_{m}^{*},\,\,\,|Tb(x)|\geq \lambda \}\leq \lambda ^{-1}\int _{(\cup J_{m}^{*})^{c}}|Tb(x)|\,dx\leq \lambda ^{-1}\sum _{n}\int _{(J_{n}^{*})^{c}}|Tb_{n}(x)|\,dx.}

By construction the integral of bn over Jn is zero. Thus, if yn is the midpoint of Jn, then by Hörmander's condition:

( J n ) c | T b n ( x ) | d x = ( J n ) c | J n ( K ( x y ) K ( x y n ) ) b n ( y ) d y | d x J n | b n ( y ) | ( J n ) c | K ( x y ) K ( x y n ) | d x d y A b n 1 . {\displaystyle \int _{(J_{n}^{*})^{c}}|Tb_{n}(x)|\,dx=\int _{(J_{n}^{*})^{c}}\left|\int _{J_{n}}(K(x-y)-K(x-y_{n}))b_{n}(y)\,dy\right|\,dx\leq \int _{J_{n}}|b_{n}(y)|\int _{(J_{n}^{*})^{c}}|K(x-y)-K(x-y_{n})|\,dxdy\leq A\|b_{n}\|_{1}.}

Hence m { x : x J m , | T b ( x ) | λ } λ 1 A b 1 2 A λ 1 f 1 . {\displaystyle m\left\{x:\,x\notin \cup J_{m}^{*},|Tb(x)|\geq \lambda \right\}\leq \lambda ^{-1}A\|b\|_{1}\leq 2A\lambda ^{-1}\|f\|_{1}.}

Combining the three estimates gives

m { x : | T f ( x ) | λ } ( 2 μ T 2 + 2 μ 1 + 2 A ) λ 1 f 1 . {\displaystyle m\{x:\,|Tf(x)|\geq \lambda \}\leq \left(2\mu \|T\|^{2}+2\mu ^{-1}+2A\right)\lambda ^{-1}\|f\|_{1}.}

The constant is minimized by taking μ = T 1 . {\displaystyle \mu =\|T\|^{-1}.}

The Markinciewicz interpolation argument extends the bounds to any L with 1 < p < 2 as follows. Given a > 0, write

f = f a + f a , {\displaystyle f=f_{a}+f^{a},}

where fa = f if |f| < a and 0 otherwise and f = f if |f| ≥ a and 0 otherwise. Then by Chebychev's inequality and the weak type L inequality above

m { x : | T f ( x ) | > a } m { x : | T f a ( x ) | > a 2 } + m { x : | T f a ( x ) | > a 2 } 4 a 2 T 2 f a 2 2 + C a 1 f a 1 . {\displaystyle m\{x:\,|Tf(x)|>a\}\leq m\left\{x:\,|Tf_{a}(x)|>{\tfrac {a}{2}}\right\}+m\left\{x:\,|Tf^{a}(x)|>{\tfrac {a}{2}}\right\}\leq 4a^{-2}\|T\|^{2}\|f_{a}\|_{2}^{2}+Ca^{-1}\|f^{a}\|_{1}.}

Hence

T f p p = p 0 a p 1 m { x : | T f ( x ) | > a } d a p 0 a p 1 ( 4 a 2 T 2 f a 2 2 + C a 1 f a 1 ) d a = 4 T 2 | f ( x ) | < a | f ( x ) | 2 a p 3 d x d a + 2 C | f ( x ) | a | f ( x ) | a p 2 d x d a ( 4 T 2 ( 2 p ) 1 + C ( p 1 ) 1 ) | f | p = C p f p p . {\displaystyle {\begin{aligned}\|Tf\|_{p}^{p}&=p\int _{0}^{\infty }a^{p-1}m\{x:\,|Tf(x)|>a\}\,da\\&\leq p\int _{0}^{\infty }a^{p-1}\left(4a^{-2}\|T\|^{2}\|f_{a}\|_{2}^{2}+Ca^{-1}\|f^{a}\|_{1}\right)da\\&=4\|T\|^{2}\iint _{|f(x)|<a}|f(x)|^{2}a^{p-3}\,dx\,da+2C\iint _{|f(x)|\geq a}|f(x)|a^{p-2}\,dx\,da\\&\leq \left(4\|T\|^{2}(2-p)^{-1}+C(p-1)^{-1}\right)\int |f|^{p}\\&=C_{p}\|f\|_{p}^{p}.\end{aligned}}}

By duality

T f q C p f q . {\displaystyle \|Tf\|_{q}\leq C_{p}\|f\|_{q}.}

Continuity of the norms can be shown by a more refined argument or follows from the Riesz–Thorin interpolation theorem.

Notes

  1. Torchinsky 2004, pp. 65–66
  2. Bell 1992, pp. 14–15
  3. Krantz 1999
  4. Torchinsky 1986 harvnb error: no target: CITEREFTorchinsky1986 (help)
  5. Stein & Rami 2005, pp. 112–114 harvnb error: no target: CITEREFSteinRami2005 (help)
  6. See:
  7. Garnett 2007, p. 102
  8. See:
  9. Stein & Shakarchi 2005, pp. 213–221
  10. Hörmander 1990
  11. Titchmarsh, 1939 & 102–105 harvnb error: no target: CITEREFTitchmarsh1939102–105 (help)
  12. See:
  13. Stein & Shakarchi 2005, pp. 112–114
  14. Stein & Weiss 1971
  15. Astala, Ivaniecz & Martin 2009, pp. 101–102 harvnb error: no target: CITEREFAstalaIvanieczMartin2009 (help)
  16. Grafakos 2005 harvnb error: no target: CITEREFGrafakos2005 (help)
  17. Stein & Weiss 1971
  18. Stein & Weiss 1971, p. 51
  19. Grafakos 2008
  20. Stein & Weiss 1971, pp. 222–223
  21. Stein & Weiss 1971
  22. Astala, Iwaniecz & Martin 2009, pp. 93–95 harvnb error: no target: CITEREFAstalaIwanieczMartin2009 (help)
  23. Astala, Iwaniecz & Martin 2009, pp. 97–98 harvnb error: no target: CITEREFAstalaIwanieczMartin2009 (help)
  24. Grafokos 2008, pp. 272–274 harvnb error: no target: CITEREFGrafokos2008 (help)
  25. Grafakos 2008
  26. Stein & Weiss 1971, pp. 222–223, 236–237
  27. Stein & Weiss 1971
  28. Grafakos 2005, p. 215−216 harvnb error: no target: CITEREFGrafakos2005 (help)
  29. Grafakos 2005, p. 255−257 harvnb error: no target: CITEREFGrafakos2005 (help)
  30. Gohberg & Krupnik 1992, pp. 19–20
  31. See:
  32. Torchinsky 2005, pp. 41–42 harvnb error: no target: CITEREFTorchinsky2005 (help)
  33. Katznelson 1968, pp. 10–21
  34. Stein, Shakarchi & 112-114 harvnb error: no target: CITEREFSteinShakarchi112-114 (help)
  35. Garnett 2007, pp. 102–103
  36. Krantz 1999
  37. Torchinsky 1986 harvnb error: no target: CITEREFTorchinsky1986 (help)
  38. Stein & Shakarchi 2005, pp. 112–114
  39. Arias de Reyna 2002
  40. Duren 1970, pp. 8–10, 14
  41. See also:
  42. Krantz 1999, p. 71
  43. Katznelson 1968, pp. 74–75
  44. Katznelson 1968, p. 76
  45. Katznelson 1968, p. 64
  46. Katznelson 1968, p. 66
  47. Katznelson 2004, pp. 78–79 harvnb error: no target: CITEREFKatznelson2004 (help)
  48. See:
  49. Torchinsky 2005, pp. 74–76, 84–85 harvnb error: no target: CITEREFTorchinsky2005 (help)
  50. Grafakos 2008, pp. 290–293
  51. Hörmander 1990, p. 245
  52. Torchinsky 2005, pp. 87–91 harvnb error: no target: CITEREFTorchinsky2005 (help)

References

Categories: