Littlewood–Paley theory uses a decomposition of a function
f into a sum of functions
fρ with localized frequencies. There are several ways to construct such a decomposition; a typical method is as follows. If
f(x) is a function on
R, and
ρ is a measurable set (in the frequency space) with
characteristic function \chi_\rho(\xi), then
fρ is defined via its
Fourier transform :\hat f_\rho := \chi_\rho\hat f. Informally,
fρ is the piece of
f whose frequencies lie in
ρ. If Δ is a collection of measurable sets which (up to measure 0) are disjoint and have union on the real line, then a well behaved function
f can be written as a sum of functions
fρ for
ρ ∈ Δ. When Δ consists of the sets of the form : \rho = [-2^{k+1},-2^k] \cup [2^k,2^{k+1}]. for
k an
integer, this gives a so-called "dyadic decomposition" of
f : Σ
ρ fρ. There are many variations of this construction; for example, the characteristic function of a set used in the definition of
fρ can be replaced by a smoother function. A key estimate of Littlewood–Paley theory is the Littlewood–Paley theorem, which bounds the size of the functions
fρ in terms of the size of
f. There are many versions of this theorem corresponding to the different ways of decomposing
f. A typical estimate is to bound the
Lp norm of (Σ
ρ |
fρ|2)1/2 by a multiple of the
Lp norm of
f. In higher dimensions it is possible to generalize this construction by replacing intervals with rectangles with sides parallel to the coordinate axes. Unfortunately these are rather special sets, which limits the applications to higher dimensions. ==The Littlewood–Paley
g function==