Let be the distinct interior roots of where its sign changes, and put . If , orthogonality gives . But has constant sign on , apart from its isolated zeros, because every sign change has been canceled. It is not identically zero, and the positive weight makes its integral nonzero, a contradiction. Thus . Degree forces exactly distinct simple roots, all inside .
For distinct nodes, let . Lagrange interpolation polynomial gives for every polynomial of degree at most . Integrating this identity proves exactness with .
For the Gaussian quadrature nodes, divide any as , with . The integral of vanishes by orthogonality, and its nodal values vanish because . The remaining polynomial is integrated exactly by the preceding interpolation result. Hence
Its weights are positive: exactness applied to gives .
Define the error functional . It annihilates polynomials of degree at most . For , the Peano kernel theorem gives
where a formal Peano kernel with the normalization made explicit is
No evaluation of is needed. The supplied inner product presupposes an integrable positive weight on the finite interval, so the integral and point-evaluation error functional is bounded on continuous functions.
For constant-density incompressible inviscid flow with conservative body force, Euler equations for an inviscid fluid give . Using , take the curl to obtain . Since both divergences vanish, the vector identity expands this to
Without incompressibility or the constant-density/barotropic hypothesis, extra compression or baroclinic terms are present; the printed equation uses these flow assumptions.
Let , with . Axisymmetric mass conservation is . If is independent of , then is affine in . The impermeable moving-plate conditions force , and integrating the radial equation gives . Regularity at the axis excludes . The meridional part of the axisymmetric inviscid flow between moving parallel plates is therefore
For no swirl, completes the field. Continuity alone does not determine azimuthal motion; this must be specified separately. More generally, prescribe a smooth regular initial profile independent of . The azimuthal part of Euler equations for an inviscid fluid is
so conservation of along radial particle paths gives , where . Together with the meridional components above, this gives a family of complete fields, with a suitable pressure determined by the radial and vertical equations. The field is therefore not unique without rotational data.
With the stated solid-body rotation, and . The vorticity equation gives , hence
For a fluid particle, , so is constant and is constant. This is conservation of angular momentum about the axis: radial spreading when the plates approach decreases the angular velocity. The meridional and rotating fields satisfy the inviscid equations with an appropriate pressure; no tangential no-slip condition is imposed on inviscid plates.
Interpret the three conditions at zero as an initial-value problem on , with interior source . A causal Green function satisfies and vanishes for . Since the leading coefficient of the third derivative is one, the jump conditions for a third-order Green function require and continuous and to jump by one. For , the homogeneous roots are . Solving , yields
For it vanishes near zero, so all three initial boundary conditions hold. The matching conditions ensure that supplies precisely a Dirac delta, without unwanted delta derivatives.
The homogeneous solution carrying the nonzero initial data is . The Green-function representation therefore gives
For the integral vanishes. For , set and integrate to obtain . Thus
The bracket and its first two derivatives vanish at , so match continuously there; its third derivative jumps by the stated forcing. The value assigned to is immaterial. The source at the initial endpoint would need a separate endpoint-delta convention, which is not used in this integral.
Fix . The Cauchy integral formula and the uniformly convergent geometric series on give
Defining
the remainder after degree has modulus at most , which tends to zero uniformly on each smaller disk. Differentiating the integral formula at zero identifies , independently of . Since is an entire function, can be chosen larger than any given , proving the global Taylor series.
For the requested radius , the same coefficient integral gives the Cauchy estimate
To characterize equality in the Cauchy coefficient estimate, parametrize its circle:
If , the identity theorem gives . Otherwise equality in the modulus bound requires the continuous integrand to have both constant modulus and constant complex argument. To see this directly, rotate its average to the positive real axis: its real part is bounded above by , and equality of its average with forces that real part to equal everywhere. Thus on the circle. The identity theorem extends that equality to the plane. Conversely every such monomial attains the bound. Therefore
including the zero function and, when , arbitrary constant functions.
A contraction mapping satisfies for all , with one fixed . The contraction mapping theorem states that such a map on a nonempty complete metric space has a unique fixed point and that every sequence of iterates converges to it.
Choose and put . Iteration gives , so for ,
Thus the iterates form a Cauchy sequence and converge by completeness to . The Lipschitz bound gives continuity of , hence . Two fixed points satisfy , forcing equality of the points. Passing also gives the usual geometric error estimate. For , convergence occurs after one application.
If is a contraction mapping, let be its unique fixed point. The commutation identity gives , so uniqueness implies . Any fixed point of is a fixed point of , giving uniqueness, without even assuming continuous. On the complete discrete metric space , the map , has constant second iterate but is not a contraction: .
For the specified function, on because it starts at zero and has derivative . Therefore maps the complete half-line into itself. Its derivative satisfies
The mean value theorem therefore makes it a contraction of constant at most . Hence
Associate to the symmetric bilinear form . If is identically zero, every basis is diagonal. Otherwise choose with . Every has the decomposition
whose second term lies in . Thus , with no cross term in . Induction on dimension gives a diagonal basis. Rescaling its nonzero entries reduces the form to
with additional zero coordinates. Define the rank of a quadratic form and its signature . Rank is intrinsic, since it is the rank of , equivalently . Also is the greatest dimension of a subspace on which the restriction of is a positive-definite quadratic form: any such subspace intersects the negative-plus-zero coordinate space only at zero, so its dimension is at most , while the positive coordinate space attains . The corresponding negative statement identifies . This proves the basis independence of and , the Sylvester's law of inertia conclusion.
For a totally isotropic subspace on which vanishes, polarization identity also makes vanish on . Quotient by the radical of a bilinear form. In the resulting nondegenerate form, projection of an isotropic subspace to either the positive or negative coordinate space is injective, so its dimension is at most . Consequently . The radical of a bilinear form together with the vectors , , attains this bound. The maximum dimension of a totally isotropic subspace is therefore
The criterion for membership in a diagonal basis follows similarly: a nonzero vector can belong to a diagonal basis if it has nonzero quadratic value, by the same orthogonal splitting, or if it lies in the radical of a bilinear form, by choosing a radical basis containing it. An isotropic vector in a diagonal basis must be orthogonal to every basis vector, and hence must lie in that radical. For the specified form, its radical is the -axis, giving exactly
The zero vector never belongs to a basis.

Pinned article: Introduction to the OurBigBook Project

Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
We have two killer features:
  1. topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculus
    Articles of different users are sorted by upvote within each article page. This feature is a bit like:
    • a Wikipedia where each user can have their own version of each article
    • a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
    This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.
    Figure 1.
    Screenshot of the "Derivative" topic page
    . View it live at: ourbigbook.com/go/topic/derivative
  2. local editing: you can store all your personal knowledge base content locally in a plaintext markup format that can be edited locally and published either:
    This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
    Figure 5. . You can also edit articles on the Web editor without installing anything locally.
    Video 3.
    Edit locally and publish demo
    . Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension.
  3. https://raw.githubusercontent.com/ourbigbook/ourbigbook-media/master/feature/x/hilbert-space-arrow.png
  4. Infinitely deep tables of contents:
    Figure 6.
    Dynamic article tree with infinitely deep table of contents
    .
    Descendant pages can also show up as toplevel e.g.: ourbigbook.com/cirosantilli/chordate-subclade
All our software is open source and hosted at: github.com/ourbigbook/ourbigbook
Further documentation can be found at: docs.ourbigbook.com
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