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Let be real symmetric matrices with sum . Their matrix ranks sum to at least , because their ranges span . If the ranks sum to , those ranges form a direct sum. For in the range of , the identity and uniqueness of its range decomposition imply . Thus and for : the matrices are mutually orthogonal orthogonal projections. In a combined orthonormal basis, the forms for use disjoint sets of independent standard normal coordinates. They are independent chi-squared distributions with degrees of freedom equal to the ranks. Conversely, if all these forms have those chi-squared laws, their expectations and their sum give .
For simple shear, . The off-diagonal entry of is . Coaxiality of isotropic elastic stress therefore proves the identity for . At , material isotropy makes the stress isotropic, proving the same identity.
For an objective material isotropy law, permutation of the principal stretches permutes the labelled principal stresses. This follows by conjugating the left stretch tensor with signed permutation rotation matrices. Each principal stress is symmetric in the other two stretches, but need not be symmetric in all three. The law provides the example . In an invariant representation , the scalar coefficients are symmetric functions of the unordered stretches.
For a CM-field, put for conjugation and . The map takes values in the cyclic group of roots of unity: all conjugates have absolute value one, and the Kronecker theorem on algebraic integers in the unit disk applies. Its kernel is , while its image on is . It therefore embeds into , a group of order two. This proves the index bound without assuming that every unit is a real unit times a root of unity.
A clutching function is the equatorial transition map used in the clutching construction. For an oriented real vector bundle one may choose a fiber metric and orthonormal trivializations, so its clutching function takes values in the special orthogonal group.
Start with singleton clusters and repeatedly merge the two clusters with the smallest chosen intercluster dissimilarity. Single-linkage clustering uses the smallest cross-pair distance; complete-linkage clustering uses the largest. Merge heights and sensitivity to ties help assess a proposed number of groups.
For binary vectors, this similarity counts agreements on both presences and absences. Its complement is the normalized Hamming distance. Whether joint absences should count as similarity depends on the application; rare-presence data may call for a different coefficient.
A dissimilarity matrix records pairwise separation of observations or profiles. Usually it is symmetric, nonnegative and zero on the diagonal. A metric space additionally requires the triangle inequality and separation of distinct profiles. Agglomerative hierarchical clustering can be applied to many dissimilarity matrices that are not Euclidean distance matrices; the claimed geometry must be checked separately.
The index measures similarity of finite sets by shared presence relative to total presence. For binary profiles it ignores joint absences, unlike the simple matching coefficient. When both sets are empty, define the similarity to be one. The complementary Jaccard distance measures dissimilarity.
For a prescribed number of groups, minimize within-cluster squared Euclidean distances. At fixed assignments, differentiating the objective gives the mean as the optimal centroid. At fixed centroids, assigning each point to a nearest centroid minimizes its contribution. Alternating these steps cannot increase the objective but can converge to a local optimum, so multiple starts are useful. Empty clusters and ties need an explicit handling rule. The method favors roughly spherical groups and depends on variable scaling.
A cluster in cluster analysis is a nonempty group of observations treated as similar under the chosen representation and dissimilarity. A partition assigns each observation to exactly one cluster; agglomerative hierarchical clustering supplies a nested sequence of such partitions. An algorithmic cluster need not correspond to a distinct probabilistic population.
For a stable -point closed-string scattering amplitude on a genus- surface, let count complex unmarked worldsheet moduli and count complex dimensions of the worldsheet conformal Killing group. Integrating the vertex positions and moduli, then fixing positions, leaves complex integrations. The punctured Riemann surface moduli dimension identifies this as . Faddeev-Popov ghost fields and antighost insertions implement the removed zero modes and the surviving modulus measure; they do not add independently integrated worldsheet coordinates.
A compact interval in the real numbers is either the empty set or a closed bounded interval with . Its compactness follows from the Heine-Borel theorem.
For an irreducible closed migration process with finite population , positive departure rates and routing matrix , choose positive traffic weights satisfying . On , its stationary distribution has the displayed form. For a predecessor , its weighted transition into is . Summing over gives by the traffic equation, and summing over proves global balance for a continuous-time Markov chain. The distribution need not satisfy detailed balance.
// Target: probability-and-statistics.bigb
Represent telephone lines by a closed migration process with free-line, operator and automated-service colonies. Accepted arrivals have rate when a free line exists, operators complete at rate , and automated calls complete at rate . Define andThe product-form stationary distribution of a closed migration process and Poisson arrivals see time averages give the displayed blocking probability. This extends a single-operator model without treating the independent operators as a server with rate when fewer than calls are present.
// Target: probability-and-statistics.bigb
A primitive closed geodesic is a closed geodesic with its smallest positive period, rather than a repeated traversal of a shorter periodic geodesic. A degree- lift of a primitive base geodesic is still primitive upstairs when its monodromy permutation has a cycle of exact length : no smaller number of traversals returns to the starting sheet.
On the punctured plane, this one-form is closed and locally the differential of the polar angle. Its line integral around a closed curve is times the winding number. A once-winding circle therefore has nonzero integral, proving that no global single-valued angle potential exists and the form is not an exact differential form.
For a counterclockwise circle of radius , substitute , . The pullback of a differential form isThe radius cancels. In coordinates, and satisfy away from the origin, so there. The nonzero integral is a global obstruction to being an exact differential form, not a nonzero local exterior derivative.
Smooth local circulation scales with enclosed area, whereas a closed angular form detects winding around an excluded point
. Details. Compare this with the smooth one-form on the whole plane. Here , and its integral around a radius- circle is , the enclosed area. The Generalized Stokes theorem applies to the full disc for . For , that disc crosses the excluded origin, where the one-form is undefined. On an annulus the theorem applies, but its induced inner boundary is clockwise: the two integrals and cancel. This explains exactly why closedness and nonzero circulation can coexist.
On the utility functions converge uniformly on every bounded set to . Their preference relations remain the usual order, while the limiting utility function makes all pairs indifferent. The weak comparison in the limit cannot be approximated by comparisons from the varying graphs. Uniform convergence does guarantee the upper graph-limit condition, because convergent pairs remain in a fixed bounded set.
With gross star formation rate , constant returned mass fraction , and the instantaneous recycling approximation, the net locked mass rate is . Mass conservation gives . For constant stellar yield per unit locked mass and initially pristine gas, metal conservation gives , so gas-phase metallicity grows as . Gross star formation and permanent locking have different normalizations.
For a pristine closed-box model of galactic chemical evolution, and imply independently of the star formation rate. The resulting metallicity distribution function is exponential on . Its normalized density is . A fixed initial mass function and survival selection are needed to turn locked stellar mass into a stellar number distribution. Logarithmic abundance intervals have the additional factor .
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!
Intro to OurBigBook
. Source. We have two killer features:
- 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-calculusArticles 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/derivativeVideo 2. OurBigBook Web topics demo. Source. - 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.
- to OurBigBook.com to get awesome multi-user features like topics and likes
- as HTML files to a static website, which you can host yourself for free on many external providers like GitHub Pages, and remain in full control
Figure 2. You can publish local OurBigBook lightweight markup files to either OurBigBook.com or as a static website.Figure 3. Visual Studio Code extension installation.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. - Infinitely deep tables of contents:
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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