For , the Landweber full inverse filter obeys
Indeed, with , the telescoping geometric series and give . Thus noise of norm at most produces iterate error at most . If , replace 2 by 1 to obtain . Together with exact-data strong convergence, a stopping choice and proves convergent regularization of an inverse problem.
The unital continuous functional calculus has image , the norm closure of star polynomials including constants. The smallest closed star subalgebra need not contain the ambient identity: for it is zero. In a nonunital algebra, apply the unital calculus in the C-star unitization and retain functions vanishing at zero to recover inside the original algebra.
Unit vector Created 2026-09-24 Updated 2026-10-14
A unit vector is a vector of norm one in a normed vector space. For a nonzero vector , vector normalization produces one by dividing by . In a real Euclidean space, this keeps the direction and removes the magnitude. The zero vector cannot be normalized because its norm is zero.
For with Euclidean norm , the corresponding unit vector is
The Euclidean vector can therefore be reconstructed as : size and direction are distinct pieces of information. The standard basis vectors are familiar unit vectors, but a unit vector need not point along a coordinate axis.
Figure 1.
Normalization keeps direction and places the endpoint on the unit circle
. The original Euclidean vector has magnitude . Its vector normalization lies on the unit circle. The enlarged right panel also shows its negative, which has the same Euclidean norm and the opposite direction. Details.
Upwind finite difference scheme Created 2026-10-06 Updated 2026-10-14
For constant-speed advection with , the explicit upwind scheme uses , . For the neighbour must be on the other side. When , the update is a convex combination and is contractive in the maximum norm on a periodic grid, or with appropriate controlled inflow data.
On a periodic grid, von Neumann stability analysis gives and , proving the same exact contraction range in the discrete L2 norm. Boundary estimates are still required on a finite interval; stable scalar eigenvalues of a triangular boundary update alone need not give a mesh-uniform bound.
Vector Created 2026-09-24 Updated 2026-10-14
A vector is an element of a vector space. Its defining operations are vector addition and scalar multiplication. An arrow in a Euclidean space is one example; a polynomial or a function can also be a vector when the chosen vector space uses the corresponding addition and scalar multiplication.
For instance, the polynomials and belong to the real vector space of polynomials of degree at most two. Their vector addition gives , and scalar multiplication gives . In the monomial basis these are the coordinate vectors , , and respectively. The vectors are the polynomials; these tuples are their representations in a chosen basis.
A general vector space does not itself prescribe lengths or angles. A norm supplies a size, while an inner product also supplies angle information and orthogonality. The familiar arrow geometry below belongs to Euclidean vectors, where this extra structure is available.
Vector measure 2026-10-07
A finite-dimensional vector measure has scalar measures as components and a total variation norm of a measure defined using their joint vector norm. Finite variation controls every pairing with a bounded continuous vector test. Derivatives in the bounded-variation space are examples.
Vector normalization is not a linear map. With and ,
Consequently, adding individually normalized directions does not generally give the direction of the original vector sum. Compute the intended vector sum first, then normalize it if it is nonzero. Cancellation is a further boundary case: has no normalized direction even though both nonzero summands do. A numerical algorithm must check that case before dividing by the norm.
Von Neumann algebra 2026-10-14
A unital star-subalgebra of the bounded operators on a Hilbert space that is closed in the weak operator topology, equivalently in the strong operator topology. The Von Neumann double commutant theorem makes these conditions equivalent to equality with the double commutant of an operator algebra. It is norm closed and hence a C-star algebra.
Localized wavelets of support diameter and norm , with enough vanishing moments, satisfy
Subtract a Taylor polynomial annihilated by the wavelet, apply the Hölder-Taylor remainder bound on its support of a function, and multiply by its norm. The same argument applies to localized boundary wavelets with the same cancellation; finitely many coarse scaling functions are handled separately.
If for a bounded operator on a separable Banach space, and is a nonempty weak-star closed convex subset of the dual unit ball with , then has a fixed point in . The Cesàro averages of the orbit remain in , and minus the identity sends those averages to vectors of norm at most . Weak-star compactness supplies a cluster point, and the adjoint action is weak-star continuous. The corresponding assertion with only weak closedness is false for the right shift on the probability simplex in , the dual of .
Weak-type operator 2026-10-14
An operator has weak type , with finite , if the displayed bound holds for every input and every , with one constant independent of both. It controls the distribution of its output rather than requiring its strong norm to be finite.
A symmetric positive-definite matrix defines an inner product on real coordinate vectors by
For diagonal , positive diagonal entries weight the squared coordinate errors. This is the finite-coordinate version of a weighted inner product; the positive-definite matrix example appears in Francis Narcowich, Inner Products and Norms, standard inner products, example 8.
For , the squared norm of is . A first-coordinate error of one costs as much as a second-coordinate error of two. The unit sphere is the ellipse , and orthogonality means . Thus “closest” and “perpendicular” depend on the chosen inner product. The orthogonal projection residual example shows how this changes a best approximation.
For with integral one, the Cauchy-Schwarz inequality makes the mass functional bounded on the weighted Hilbert space. The vector has norm one, so the velocity-reset projection is the orthogonal projection onto its span. Consequently is bounded and self-adjoint. This Hilbert geometry differs from the norm-one positive reset projection on phase-space .
Let and . The displayed norm makes the holomorphic functions with finite norm a Banach space. Finiteness forces : for fixed , the weight grows like near zero. A Cauchy sequence in this norm converges uniformly on every compact subset of , including at . Its limit is holomorphic by locally uniform convergence of holomorphic functions, and the pointwise norm bounds show convergence in the original norm. The shrinking domain compensates for loss of an -derivative in a Cauchy-Kovalevskaya theorem argument.
Weighted Neumann heat kernel with constant drift Created 2026-10-05 Updated 2026-10-06
On , the differential operator with homogeneous Neumann boundary conditions is self-adjoint in the weighted inner product with weight . Its eigenfunctions and nonnegative decay rates are
Their squared norms are and . The Sturm-Liouville eigenfunction expansion gives
This kernel acts against the measure , not Lebesgue measure alone. It is symmetric in ; the transition density against Lebesgue measure is .
Wiener algebra 2026-10-06
The Wiener algebra consists of periodic functions with absolutely summable Fourier coefficients, with norm . Multiplication corresponds to discrete convolution of coefficients, so the norm is submultiplicative. Consequently also belongs to the algebra when does. Every such Fourier series is uniformly convergent and defines a continuous function.