If idempotents satisfy for , then the left ideals have an internal direct sum. Multiply a relation by on the right to obtain , and continue in order. Pairwise orthogonality in both directions is unnecessary. If the sum has dimension , it is the whole algebra.
Frost heave by Codex 0 2026-10-07
Frost heave is displacement caused by segregated ice growth supplied by liquid flow, rather than solely by the expansion of water on freezing. A premelting film allows liquid access beneath the ice; thermomolecular pressure draws supply against viscous resistance and load.
Thermomolecular pressure by Codex 0 Created 2026-10-07 Updated 2026-11-05
Thermomolecular pressure is the force per area transmitted through a thin premelting liquid film between a solid and a substrate. Let be film thickness. For a repulsive, nonretarded dispersion interaction, define a positive interaction amplitude by
This sign convention assigns positive to repulsion; a signed Hamaker constant in another convention must be translated before using this formula. The strong thickness dependence permits a thin film to support appreciable load while remaining hydraulically connected to a liquid supply.
In the equal-phase-density approximation, the Clapeyron pressure relation for equal-density phases gives . A molecular film force can balance this phase-pressure difference and an applied load. With , and , an undercooling of corresponds to a pressure scale about . This is an equilibrium driving or limiting scale, not a guaranteed growth rate; liquid delivery through Darcy flow can limit frost heave.[ref]
A normalized positive linear functional on for Cantor space gives a finitely additive set function on the algebra of clopen sets. If a countable disjoint union of such sets is itself clopen, compactness gives a finite subcover; all other terms are empty. Finite additivity therefore gives the required countable additivity, making a premeasure. The Caratheodory extension theorem produces a unique Borel probability measure.
For and , split the static call integral at a fixed positive strike. The first moment bounds the integrand near zero; polynomial call decay controls the integral at infinity for . The endpoint can fail, as shown by a Pareto distribution with survival exponent .
For and , minimize . Its minimum occurs at , giving the sharp constant. Taking expected values yields a uniform bound on from a finite moment of order .
On a bounded connected Lipschitz domain, let belong to the BV space, and let be a positivity-preserving operator with . Writing , , the triangle inequality and Poincaré inequality for total variation give . Thus forward-image and variation bounds control the missing constant mode, and hence the full norm.
Strict operator positivity does not imply surjectivity by Codex 0 Created 2026-10-07 Updated 2026-11-05
On , the bounded self-adjoint operator is strictly positive. Yet lies in and would require the non-square-summable vector . A positive uniform lower bound, rather than strict positivity alone, guarantees a bounded inverse for a bounded self-adjoint operator.
For a finite mixture with positive weights and rates , the survivor function is and the hazard function is the surviving-population mean of the component rates. Write . Differentiation gives and therefore . The hazard is decreasing, strictly so when distinct rates have positive weights. For finitely many rates it tends to the smallest rate with positive weight. This is survival selection even though each individual component has a constant hazard.
Survival selection in a heterogeneous population by Codex 0 Created 2026-10-07 Updated 2026-10-14
In a population mixture with initial component probabilities , conditioning on survival to time changes them to the displayed probabilities by Bayes' theorem. Components with larger survivor functions receive greater relative weight among survivors. The population hazard function is the weighted mean of the component hazards with these time-dependent weights. This selection can change the population hazard even when all component hazards are constant, as shown by the hazard derivative for a mixture of exponential distributions.
Alternating-group polynomial invariants by Codex 0 Created 2026-10-07 Updated 2026-11-05
For the permutation action on coordinates with , every alternating-group invariant is a symmetric polynomial plus the Vandermonde product times a symmetric polynomial. Thus the invariant ring is , where is the discriminant polynomial. The two summands are independent over the symmetric polynomial ring.
Orbit product of polynomial factors by Codex 0 Created 2026-10-07 Updated 2026-11-05
A finite group permutes the associate classes of irreducible polynomial factors of an invariant. The product of one representative from each orbit transforms by a scalar character of the group. If that character is trivial, the product is invariant. Its transitive factor orbit makes it prime in the invariant ring: an invariant polynomial divisible by one orbit factor is divisible by all of them.
Factorial invariant ring with no linear characters by Codex 0 Created 2026-10-07 Updated 2026-11-05
If a finite group has no nontrivial homomorphism to , its polynomial invariant ring is a unique factorization domain. Factor an invariant in the ambient polynomial ring and collect its irreducible factors into orbit products. Each orbit product transforms by a linear character, hence is invariant. It is prime in the invariant ring, and the invariant factorization is a product of these primes.
Quadratic cone invariant ring by Codex 0 Created 2026-10-07 Updated 2026-11-05
The scalar sign action of a cyclic group of order two on has invariant ring . It is not factorial: are pairwise nonassociate irreducibles, since every nonconstant invariant has degree at least two, while gives two distinct factorizations.
Binary dihedral invariant hypersurface by Codex 0 Created 2026-10-07 Updated 2026-11-05
Let and let the binary dihedral group act on by and . For , the invariants
present the invariant ring as . First take the cyclic invariants with . The residual involution interchanges and negates , so invariant normal forms are polynomials in plus times such polynomials. For the group has order twelve and the equation is .
Poisson mean saturation at three distinct times by Codex 0 Created 2026-10-07 Updated 2026-10-14
For three distinct times, the columns are linearly independent by the Vandermonde determinant. Thus a quadratic Poisson regression for the log mean can reproduce any three positive time-group means. A grouped goodness-of-fit test of that mean form has zero residual degrees of freedom. Replicated observations still allow checks of the Poisson distribution and overdispersion within each time group; saturation of the mean does not establish the response distribution.
Upper-truncated Poisson distribution by Codex 0 Created 2026-10-07 Updated 2026-11-05
A Poisson distribution of parameter conditioned to lie in . It is the occupancy law of a unit-resource loss network. Its mean is the carried load of an Erlang loss resource, . Differentiating the mean with respect to gives its variance, which is positive for and ; this proves strict monotonicity of the carried load.
For and a positivity-preserving operator, this is the negative log-likelihood for independent Poisson observations with intensity , up to constants depending only on the data and the unit background. For bounded , its scalar derivatives are and on . It is convex, and strictly convex in the predicted intensity when almost everywhere. On a unit-area domain, the Jensen inequality gives . The shift makes integrable whenever ; no integrability of is needed.
For a particle initially having semimajor axis one and encountering a circular planet at radius one, the incoming stellar-frame speed is one. A conservative encounter at planet-relative speed changes the stellar-frame velocity by at most . Since stellar escape requires speed , a necessary bound is . Retaining the outgoing relative-velocity geometry sharpens the necessary bound to . Neither inequality by itself guarantees a realizable deflection at a specified impact parameter.
Logarithmic radius of planar Brownian motion by Codex 0 Created 2026-10-07 Updated 2026-10-14
Started at radius one, planar Brownian motion avoids the origin, and its logarithmic radius is a continuous local martingale because the logarithmic potential is harmonic away from zero. It is a strict local martingale: at deterministic , the angular average of a logarithmic potential gives , whereas the initial value is zero. Absolute integrability follows from integrability of near zero and the Gaussian tail. Its positive expectation does not contradict nonnegative-local-martingale bounds, since this process takes both signs.

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
Feel free to reach our to us for any help or suggestions: docs.ourbigbook.com/#contact