lacunary - Definition Index

Definition Index

This page lists all mathematical definitions found across the site. Click on any definition to jump to its location in the notes.

Found 349 definitions
Definition: A/B Test \@{ab-test}

An A/B test is a two-sample statistical inference problem. When we're running an A/B test, we have two groups of users, group A and group B.

We change some functionality for group A and leave it stable for group B. We want to see if there is a statistically significant difference between group A and group B for some metric.

TODO: finish this. Formalize the two-sample setup in terms of the two random variables X and Y, and describe the CUPED variance-reduction technique the page is named for.

Definition: Abelian \@{abelian}

Abelian groups are groups whose operation is commutative. For a,b∈G,a∗b=b∗a.

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from Groups
Definition: Absolutely Continuous Random Variable (also: continuous random variable) \@{absolutely-continuous-random-variable}

For a real valued random variable

X:Ω→R,

we call X a continuous random variable if there exists a function

fX:R→[0,∞)

such that for every measurable set A⊆R,

P(ω∈Ω:X(ω)∈A)=∫AfX(x)dx

where fX is the probability density function of X.

TODO: this definition excludes some continuous distributions like the Cantor distribution and in general isn't quite there yet in terms of measure theory. I need to revisit this when I've learned a bit more of measure theory.

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Definition: alternating group \@{alternating-group}

The subgroup of Sn consisting of all even permutations of n letters is the alternating group An on n letters. If n≥2, then this set forms a subgroup of Sn of order n!/2.

from Groups
Definition: Analytic at a point \@{analytic-at-a-point}

A complex function f is said to be analytic at a point z if it is analytic in some neighborhood of z. However, even here, the point being analytic depends on the neighborhood around the point being complex differentiable.

Definition: Archimedean \@{archimedean}

The Archimedean property is that given two positive numbers x and y, there is an integer n such that nx>y.

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Definition: Ball \@{ball}

Given x∈Rk,r>0, the open or closed ball with center x and radius r is defined as the set of points y such that |x−y|<r or |x−y|≤r, respectively.

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Definition: Base \@{base}

A collection Vα of open subsets of X is said to be a base for X if the following is true: For every x∈X and every open set G⊂X such that x∈G, we have x∈Vα⊂G for some α. In other words, every open set in X is the union of a subcollection of Vα.

Definition: Bernoulli Process \@{bernoulli-process}

A Bernoulli Process must possess the following properties:

  1. The experiment consists of repeated trials.
  2. Each trial results in a boolean outcome, which can be considered true or false, success or failure, etc.
  3. The probability of success, p, remains constant across trials.
  4. Repeated trials are independent.
Definition: Bias (also defines: unbiased estimator) \@{bias}

In an estimation problem, the bias of an estimator T(X) of a real-valued parameter ϑ of the unknown population is defined to be bT(P)=E[T(X)]−ϑ (which is denoted by bT(θ) when P is in a parametric family index by θ).

An estimator is said to be an unbiased estimator for ϑ if and only if bT(P)=0 for any P∈P.

Definition: bifurcation \@{bifurcation}

In a @dynamical-system with a smoothly varying parameter r, a sudden change in qualitative or topological behavior of the system, especially the creation, annihilation, or change of stability in its fixed points, is called a bifurcation.

Definition: bifurcation point \@{bifurcation-point}

The parameter values at which bifurcations occur are called bifurcation points.

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Definition: Binary Classification \@{binary-classification}

Binary Classification is the task of putting things into one of two categories (each called a class.)

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Definition: Binomial Coefficient \@{binomial-coefficient}

For n,k∈N,n≥k≥0, the binomial coefficient is the coefficient of the xk term in the polynomial expansion of the binomial power (1+x)n. It is denoted as (nk) and can be expressed through @factorial notation as

(nk)=n!k!(n−k)!.

Definition: Binomial Distribution \@{binomial-distribution}

A binomial distribution aggregates the outcomes of a Bernoulli process across multiple trials to tell you how likely it is to achieve a certain number of successes. The number X of successes in n Bernoulli trials is called a binomial random variable, and its probability distribution is what we call the binomial distribution.

If we let n be the number of trials, x be the number of successes, and p be the probability of success on a given trial, and q=1−p be the probability of failure on a given trial, then the probability distribution of the random variable X is

b(x,n,p)=(nx)pxqn−x,x=0,1,2,…,n.

To break this down some, there are (nx) ways to have x successes out of n trials (different orderings). For each, there are x independent events that occur with a probability of p and n−x independent events that occur with a probability of q=1−p.

The mean and variance of the binomial distribution b(x,n,p) are

μ=np, and σ2=npq.

We can use a summation over the formula above to find the probability of there being between a and b successes:

∑x=ab(nx)pxqn−x.

Definition: Bound vector \@{bound-vector}

A vector with a fixed endpoint is called a bound vector.

Definition: Boundary \@{boundary}

The points on a manifold whose neighborhoods are homeomorphic to a neighborhood in a half k-ball form the boundary of the manifold. Formally,

∂M={p∈M|there exists a chart (U,p) with φ(p)∈Rk−1×0⊂Hk}.

That is, p is a boundary point, if, in local coordinates, it maps to the edge of the half-space model.

Definition: Cantor set \@{cantor-set}

Let E0 be the interval [0,1]. Remove the segment (13,23), and let

E1=[0,13]∪[23,1].

Similarly, remove the middle thirds of these intervals, and let

E2=[0,19]∪[29,39]∪[69,79]∪[89,1].

We can continue this forever, and we get a nested sequence {En} of compact sets En where:

(a) En+1⊂En.

(b) En is the union of 2n intervals, each of length 1/3n.

Finally, the set

P=⋂n=1∞En

is called the Cantor set.

Definition: Capacity (also: channel-capacity) \@{capacity}

The capacity C of a discrete channel is given by

C=limt→∞log⁡N(t)t,

where N(t) is the number of allowed @signals of duration t.

Definition: Cardinal Number, Equivalent \@{cardinal-number-equivalent}

Given two sets, A and B, if there is a bijection (a one-to-one mapping of A onto B) between A and B, we say A and B have the same cardinal number, or that A and B are equivalent. We denote this as A∼B.

Definition: Cauchy Principal Value \@{cauchy-principal-value}

Let's say we have an integral

∫ABf(x)dx(a)

whose integrand becomes infinite at a point a in the interval of integration.

Then, (a) means, by definition

∫ABf(x)dx=limϵ→0∫Aa−ϵf(x)dx+limη→0∫a+ηBf(x)dx.

However, it may be the case that neither limit exists when both ϵ and η approach 0 independently, but that the limit

limϵ→0[∫Aa−ϵf(x)dx+∫a+ϵBf(x)dx]

does exist.

This limit is called the Cauchy principal value of the integral and is written as

pr. v. ∫ABf(x)dx.

Definition: center (group) \@{center-group}

The center of a group G is all the elements that commute with all elements of G:

Z(G)={z∈G|zg=gz for all g∈G}.

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from Groups
Definition: Characteristic equation \@{characteristic-equation}

The characteristic equation tells us how to find the @eigenvalues and is given by:

λ2−τλ+Δ=0.

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Definition: Circle of Convergence \@{circle-of-convergence}

The circle |z−z0|< in which the Taylor series converges to the function is called the circle of convergence for the Taylor series.

Definition: Class (also: category, type, kind) \@{class}

A class is a collection of individuals or individual objects. A class can be defined either by extension (specifying members) or by intension (specifying conditions).

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Definition: Classification \@{classification}

Classification is the activity of assigning objects to some pre-existing classes or categories.

Definition: Closed \@{closed}

A set E is closed if every limit point of E is a point of E.

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Definition: Closure \@{closure}

If X is a metric space, E⊂X, and E′ denotes the set of all limit points of E in X, then the closure of E is the set E―=E∪E′.

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Definition: Commensurable (also: commeasurable) \@{commensurable}

Real numbers a1,…,an are commensurable if there exists a common measure m∈R>0 such that each ai is an integer multiple of it: ai=kim,ki∈Z,i=1,…,n. Equivalently, all pairwise ratios are rational: ai/aj∈Q for all i,j (with aj≠0).

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Definition: Commutative Ring \@{commutative-ring}

A ring in which multiplication is commutative is called a commutative ring.

Definition: commutator \@{commutator}

The commutator subgroup of G is the group C generated by all elements of the set

{aba−1b−1|a,b∈G}.

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from Groups
Definition: Compact \@{compact}

A subset K of a metric space X is said to be compact if every open cover of K contains a finite subcover. More explicitly, the requirement is that if {Gα} is an open cover of K, then there are finitely many indicies α1,…,αn such that K⊂Gα1∪⋯∪Gαn.

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Definition: Complex Differentiable \@{complex-differentiable}

In the above definition of complex derivative, if the limit exists, f is said to be differentiable at the point z0.

Definition: Component Function \@{component-function}

Let f be a function that maps an open set E⊂Rn into Rm. Let {e1,…,en} and {u1,…,un} be the standard bases of Rn and Rm. The component functions of f are the real functions f1,…,fm defined by

f(x)=∑i=1mfi(x)ui(x∈E),

or, equivalently, by fi(x)=f(x)⋅ui,1≤i≤m.

Definition: Composition \@{composition}

Suppose X,Y,Z are metric spaces, E⊂X, f:E→Y, g:f(E)→Z, h:E→Z with

h(x)=g(f(x))(x∈E).

The function h is called the composition or the composite of f and g. The notation

h=g∘f

is frequently used.

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Definition: Condensation Point \@{condensation-point}

A point p in a metric space X is said to be a condensation point of a set E⊂X if every neighborhood of p contains uncountably many points of E.

Definition: Conditional Entropy \@{conditional-entropy}

Let X and Y be random variables, not necessarily independent. The probability that Y takes the value y when X takes the value x (for any specific x∈X,y∈Y) is called the conditional probability p(y|x) and is given by:

p(y|x)=p(x,y)p(x),p(x)=∑yp(x,y).

(Note that p(x,y) is the joint probability of X=x,Y=y.)

We define the conditional entropy of Y given X, H(Y|X), as the average of the entropy of Y for each value x of X weighted according to the probability of getting that particular x. That is,

H(Y|X)=−∑x∈X,y∈Yp(x,y)log⁡p(y|x).

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Definition: Conditional Mutual Information \@{conditional-mutual-information}

The conditional mutual information of random variables X and Y given Z is defined by

I(X;Y|Z)=H(X|Z)−H(X|Y,Z)=Ep(x,y,z)log⁡p(X,Y|Z)p(X|Z)p(Y|Z).

It is the uncertainty about X after learning Z minus the uncertainty about X after learning Y and Z.

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Definition: Conditional Probability \@{conditional-probability}

From this, we can give the formula for conditional probability. The probability of A given B is

P(A|B)=P(A and B)P(B).

That is to say, the probability of A occurring given B has occurred is the portion of times B occurs that A also occurs.

If P(A)=P(A|B), then A and B are independent events, and P(A)⋅P(B)=P(A and B).

Definition: Conditional Probability Distribution (also: conditional distribution, conditional probability mass function) \@{conditional-probability-distribution}

TODO: define fY|X(y|x) for the discrete and continuous cases; note it is a probability distribution in y for each fixed x with fX(x)>0. Relate to conditional probability, which states the event-level version.

Definition: Conditional Relative Entropy \@{conditional-relative-entropy}

For joint probability mass functions p(x,y) and q(x,y), the conditional relative entropy

D(p(y|x)‖q(y|x))

is the @average of the relative-entropies between the conditional probability mass functions p(y|x) and q(y|x) averaged over the probability mass function p(x). More formally,

D(p(y|x)‖q(y|x))=∑x∈Xp(x)∑y∈Yp(y|x)log⁡p(y|x)q(y|x)=Ep(x,y)log⁡p(Y|X)q(Y|X).

Definition: Confidence Interval \@{confidence-interval}

A confidence interval tells us how likely it is that a population parameter falls within a specified range, based on a statistic calculated from a sample of data. This interval provides a range of values that, with a certain level of confidence (usually expressed as a percentage like 95% or 99%), is believed to encompass the true parameter value. The width of the interval gives an idea of the precision of our estimate, with narrower intervals representing more precise estimates.

To say that the range of values has a certain level of confidence means that if we were to repeat the experiment or sampling process many times (theoretically an infinite number of times), the true population parameter would fall within that interval in the stated percentage of all trials. For example, a 95% confidence level means that 95 out of 100 such confidence intervals would contain the true population parameter (which is unknown).

If you were to repeat the sampling process an infinite number of times, each time calculating a new 95% confidence interval using the same method, about 95% of these intervals would contain the true population parameter. Each interval is calculated from a different sample and might be different in range, but the method of calculation ensures that 95% of these intervals will capture the true parameter value.

Definition: Connected \@{connected}

If X is a metric space, a set E⊂X is said to be connected if E is not a union of two nonempty separated sets.

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Definition: Connected Complex \@{connected-complex}

A set S is said to be connected if every pair of points in S can be joined by a finite number of line segments joined end to end that lie entirely within S.

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Definition: Conservative system \@{conservative-system}

Systems for which a conserved quantity exist are called conservative systems.

Definition: Conserved Quantity \@{conserved-quantity}

Given a system x˙=f(x), a conserved quantity is a @real-valued continuous function E(x) that is constant on trajectories, i.e. dE/dt=0. We also require that E(x) is nonconstant on every open set, to avoid trivial examples such as E(x)=0.

Definition: Continuous \@{continuous}

Suppose X and Y are metric spaces, E⊂X,p∈E, and f:E→Y. Then f is said to be continuous at p if for every ϵ>0 there exists a δ>0 such that

dY(f(x),f(p))<ϵ

for all points x∈E for which dX(x,p)<δ.

If f is continuous at every point of E, then f is said to be continuous on E.

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Definition: Continuous Sample Space \@{continuous-sample-space}

If a sample space contains an infinite number of possibilities equal to the number of points on a line segment, it is called a continuous sample space.

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Definition: Continuously Differentiable \@{continuously-differentiable}

A differentiable function f of an open set E⊂Rn into Rm is said to be continuously differentiable in E if f′ is a continuous function of E into L(Rn,Rm). More explicitly, it is required that to every x∈E and to every ϵ>0 corresponds a δ>0 such that

‖f′(y)−f′(x)‖<ϵ

if y∈E and |x−y|<δ.

If this is the case, we also say that f is a C′-mapping or that f∈C′(E).

Definition: Contour Integral \@{contour-integral}

Given a smooth curve C in a domain D and f(z)=u(x,y)+v(x,y)i a continuous function defined along C, we say that

∫Cf(z)dz=∫C(u+vi)(dx+dyi)=∫C(udx−vdy)+i∫C(vdx+udy).

We can parameterize C as

C:z=z(t)=x(t)+y(t)i,α≤t≤β

Then, z′(t)=x′(t)+iy′(t),

and by the chain rule,

x′(t)=dxdtdt,y′(t)=dydtdt.

Therefore,

z′(t)=dzdt=dxdt+idydt

or equivalently

dz=z′(t)dt.

Then we have

∫Cf(z)dz=∫αβf[z(t)]z′(t)dt.

Definition: Converge \@{converge}

A sequence {pn} in a metric space X is said to converge if there is a point p∈X with the following property: For every ϵ>0, there is an integer N such that n≥N implies that d(pn,p)<ϵ.

Definition: Convolution \@{convolution}

Sums of independent random variables are called convolutions.

If X and Y are continuous, the probability density function of X+Y is given by

fX+Y(x)=∫−∞∞fX(t)fY(x−t)dt.

If they are discrete, the probability mass function of X+Y is given by

fX+Y(n)=∑kfX(k)fY(n−k).

Definition: Correlation Coefficient \@{correlation-coefficient}

The correlation coefficient of X and Y, ρx,y, is given by

ρx,y=Cov(X,Y)σXσY.

Definition: coset \@{coset}

Let H be a subgroup of G. Given a∈G, the subset aH={ah|h∈H} of G is the left coset of H containing a, while the subset Ha={ha|h∈H} is the right coset of H containing a.

from Groups
Definition: Countable \@{countable}

A set A is said to be countable if there exists a bijection between A and the set of all positive integers Z>0, that is, if A∼Z>0.

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Definition: Covariance \@{covariance}

Covariance is a measure of the joint variability of two random variables.

Cov(X,Y)=E[(X−E[X])(Y−E[Y])].

If large X values go with large Y values and small X goes with small Y, covariance will be positive. The covariance will be negative if large X values go with small Y values and vice-versa. An alternative, equivalent form of covariance is:

Cov(X,Y)=E[XY]−E[X]E[Y].

Definition: Cross Product (also: Vector Product, Outer Product) \@{cross-product}

The cross product a×b (read "a cross b") of two vectors a and b is the vector v denoted by

v=a×b.

I. If a=0 or b=0, then we define v=a×b=0.

II. If both vectors are nonzero vectors, then vector v has the length

|v|=|a×b|=|a||b|sin⁡θ,(1)

where θ is the angle between a and b. Furthermore, a and b form the sides of a parallelogram on a plane in space. The area of this parallelogram is precisely given by (1), such that the length |v| of the vector v is equal to the area of the parallelogram.

III. If a and b lie in the same straight line, i.e. a and b have the same or opposite directions, then θ is 0∘ or 180∘ so that sin⁡θ=0. In that case |v|=0, so that v=a×b=0.

IV. If cases I and III do not occur, then v is a nonzero vector. The direction of v=a×b is perpendicular to both a and b such that a,b,v, precisely in this order, form a right-handed triple

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Definition: Cross-Entropy \@{cross-entropy}

Given two discrete probability distributions, p and q, that share a support X, cross-entropy measures the average number of bits needed to represent an event drawn from X when the coding scheme is optimized for an estimated distribution q rather than the true distribution p. Its formula is very similar to that of entropy, except surprisal is calculated using q while expectation uses p:

H(p,q)=−∑x∈Xp(x)log⁡q(x).

We can write it in expectation form as

H(p,q)=Ep[−log⁡q],

where Ep is expectation under p.

Definition: Cumulative Distribution Function \@{cumulative-distribution-function}

Sometimes we want to know the probability that a random variable will be less than or equal to some real number x. If we let F(x)=P(X≤x) for all real x, we define F(x) to be the cumulative distribution function of the random variable X. More formally, the cumulative distribution function F(x) of a discrete random variable X with a probability distribution f(x) is:

F(x)=P(X≤x)=∑t≤xf(t),−∞<x<∞.

Definition: Curl \@{curl}

For a vector field F=(F1,F2,F3) defined in three-dimensional space R3, with each component function Fi depending on the variables x, y, and z, the curl of F is defined as

curlF=∇×F=(∂F3∂y−∂F2∂z)i+(∂F1∂z−∂F3∂x)j+(∂F2∂x−∂F1∂y)k

Definition: cycle \@{cycle}

A permutation σ∈Sn is a cycle if it has at most one orbit containing more than one element. The length of a cycle is the number of elements in its largest orbit.

from Groups
Definition: cyclic group \@{cyclic-group}

A cyclic group is a group where there exists some g∈G such that every element in G can be generated from the group operation applied to g.

That is, G={gn|n∈Z} when we think of the operation as multiplication, or G={ng|n∈Z} when we think of the operation as addition.

from Groups
Definition: cyclic notation \@{cyclic-notation}

A cycle in Sn may be written as (a1,a2,⋯,ak) - this is called cyclic notation. It represents the permutation that sends a1→a2→⋯→ak→a1.

from Groups
Definition: cyclic subgroup \@{cyclic-subgroup}

Any subgroup of a cyclic group is also cyclic - a cyclic subgroup.

from Groups
Definition: del (also: vector differential operator, nabla) \@{del}

In Euclidean space Rn with coordinates (x1,…,xn) and standard basis (e1,…,en), del is a vector operator whose x1,…,xn components are the partial derivative operators ∂∂x1,…,∂∂xn; that is

∇=∑i=1nei∂∂xi=(∂∂x1,…,∂∂xn).

Definition: Derivation (also: proof) \@{derivation}

A derivation (or proof) in F is a finite sequence of formulas

φ1,φ2,…,φn

such that for each i≤n,

  1. Either φi∈A, or
  2. φi follows from earlier formulas in the sequence by an inference rule in R.
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Definition: Derivative Function \@{derivative-function}

While the equation defined in (a) only applies to a specific point z0, we can drop the subscript to get

f′(z)=limΔz−>0f(z+Δz)−f(z)Δz,(b)

which defines the complex derivative of f at the point z. This equation defines the complex function f′, known as the derivative function.

Definition: Diameter \@{diameter}

Let E be a nonempty subset of a metric space X, and let S be the set of all real numbers of the form d(p,q), with p,q∈E. The supremum of S is called the diameter of E.

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Definition: Difference equation \@{difference-equation}

A difference equation has the general form

xn+1=f(xn,n),

where n is a time-like variable, f and xn may be vectors, n=0,1,2,⋯=N0.

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Definition: Differentiable \@{differentiable}

Suppose E is an open set in Rn, f:E→Rm, and x∈E. If there exists a linear transformation A:Rn→Rm such that

limh→0|f(x+h)−f(x)−Ah||h|=0,(14)

then we say that f is differentiable at x and we write

f′(x)=A.

If f is differentiable at every x∈E, we say that f is differentiable in E.

Note that in (14), h∈Rn. If |h| is small enough, then x+h∈E, because E is open. Therefore, f(x+h) is defined, f(x+h)∈Rm, and since A∈L(Rn,Rm), Ah∈Rm. Therefore,

f(x+h)−f(x)−Ah∈Rm.

The norm in the numerator of (14) is that of Rm, while the norm in the denominator is the Rn-norm.

We can also rewrite (14) as

f(x+h)−f(x)=f′(x)h+r(h),(17)

where the remainder r(h) satisfies

limh→0|r(h)||h|=0.

This means that for a fixed x and a small h, the left side of (17) is approximately equal to f′(x)h, that is, to the value of a linear transformation applied to h.

Definition: Directional Derivative \@{directional-derivative}

Using the setup from the definition of component, let us fix an x∈E (with E⊂Rn,) and let u∈Rn be a unit vector. Then,

limt→0f(x+tu)−f(x)t=(∇f)(x)⋅u

is called the directional derivative of f at x in the direction of the unit vector u and is denoted as Duf(x).

Definition: Discrete Channel \@{discrete-channel}

A system whereby a sequence of choices from a finite set of elementary symbols S1,…,Sn can be transmitted from one point to another. Each of the symbols Si is assumed to have a certain duration in time ti seconds (not necessarily the same for different Si).

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Definition: Discrete Metric \@{discrete-metric}

The discrete metric is defined as:

d(x,y)={0if x=y1if x≠y

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Definition: Discrete Random Variable \@{discrete-random-variable}

A random variable is called a discrete random variable if there exists a countable set S⊆X such that

P(ω∈Ω:X(ω)∈S)=1.

In this case its state space is often called an alphabet.

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Definition: Discrete Sample Space \@{discrete-sample-space}

If a sample space contains a finite number of possibilities, or an unending sequence with as many elements as there are whole numbers (countably infinite), it is called a discrete sample space.

Definition: discrete time points (also: time mesh points, time grid points) (also defines: step size) \@{discrete-time-points}

Consider a @partition 0=t0<t1<⋯<tN=T of the time interval [0,T]. We can call the points tn the discrete time points. Then our goal is to approximate the values u(tn) with a set of quantities {un}n=0N, that is, un≈u(tn) for n=0,1,…,N. We can also write δtn=tn+1−tn to denote the step size (also: time step) between between consecutive points. For simplicity we often assume that δtn=δt for all n=0,1,…,N−1, i.e. the time steps are constant. Such a mesh is called a @uniform mesh.

Definition: disjoint (cycle) \@{disjoint-cycle}

Two or more cycles are disjoint if no element appears in more than one cycle.

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from Groups
Definition: Diverge \@{diverge}

If a sequence {pn} does not converge, it is said to diverge.

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Definition: Divergence \@{divergence}

For a vector field F=(F1,F2,F3) defined in three-dimensional space R3, the divergence is defined as

divF=∇⋅F=∂F1∂x+∂F2∂y+∂F3∂z.

Definition: Division Ring \@{division-ring}

Let R be a ring with unity. If every nonzero element of R is a unit (has a multiplicative inverse), then R is called a division ring.

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Definition: Domain \@{domain}

A domain is an open connected set. Note that this is not the same as a domain of definition of a function.

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Definition: Domain of Definition \@{domain-of-definition}

If f is a function from the set A to the set B, the set A is called the domain of f.

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Definition: Doubly Stochastic Matrix (also: bistochastic matrix) \@{doubly-stochastic-matrix}

If a matrix is both a row stochastic matrix and a column stochastic matrix, it is said to be a doubly stochastic matrix. That is, both its rows and its columns sum to 1.

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Definition: Element (also: member, point) \@{element}

The objects that make up a set are called its elements or its members.

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Definition: Empirical Distribution \@{empirical-distribution}

TODO: define this.

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Definition: Empty Set \@{empty-set}

The empty set is the set that has no elements and is denoted {} or ∅. It is the unique set with @cardinality of 0.

Definition: Entire (also: entire-function) \@{entire}

A function which is analytic on the whole complex plane is called an entire function.

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Definition: Entropy (also: uncertainty) \@{entropy}

Given a discrete random variable X, which may be any element x within the set X, and is distributed according to p:X→[0,1], the entropy is

H(X):=−∑x∈Xp(x)log⁡p(x).

We can choose different bases for the logarithm; throughout these notes a bare log means log2, giving the unit of @bits.

An alternative, equivalent definition is that entropy is the expected value of the self-information of a random variable:

H(X)=E[I(X)]=E[−log⁡p(X)].

The unit for entropy is bits per symbol.

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Definition: Entropy Rate \@{entropy-rate}

Consider a discrete source with i finite number of states, where in state i there is probability pi(j) of producing symbol j. Then, each state i will have an entropy Hi, and the entropy rate of the source will be defined as the average of these Hi weighted by the probability of the occurrence of each state (Pi):

H=∑iPiHi=−∑i,jPipi(j)log⁡pi(j).

In other words, H=E[Hi] - the expected value of the per state entropy.

This is the entropy of the source per symbol of text.

If the source (a @markoff-process) produces symbols at a definite time rate there is also an entropy per second:

H′=∑ifiHi,

where fi is the average @frequency of state i. We can also say

H′=mH,

where m is the average number of symbols produced per seconds, i.e. fi=mPi

H an H′ measure the amount of information generated by the source per symbol and per second, respectively. For log2, they represent bits per symbol and bits per second.

Definition: Entry (also: component) \@{entry}

A specific element ai in an n-tuple is called an entry of the n-tuple, and i indicates its ordinal position, i.e. ai is the ith entry in a.

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Definition: Ergodic \@{ergodic}

If for some positive integer m we have that pjk(m)>0 for all j,k=1,2,…,N, then the Markov chain is said to be ergodic.

Definition: Essential Singularity \@{essential-singularity}

An essential singularity occurs if there are infinitely many negative powers in the Laurent series.

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Definition: Estimator (also defines: estimate) \@{estimator}

Let P be a statistical model on (Ω,F), and let ϑ:P→Λ be a parameter, where (Λ,G) is a measurable space. An estimator of ϑ is a statistic T:(Ω,F)→(Λ,G). If x∈Ω is an observed data set (i.e. one value that a sample X happened to take), the value T(x) is called an estimate of ϑ.

Definition: even (permutation) \@{even-permutation}

A permutation of a finite set is even if it is the product of an even number of transpositions.

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from Groups
Definition: Event \@{event}

An event is a subset of a sample space. For example, we can say the event A that the roll of a die is odd is A={1,3,5}, the event B that the roll of a die is even is B={2,4,6}, and that the event that the roll of a die is less than or equal to 4 is C={1,2,3,4}.

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Definition: Expected Value (also: expectation) \@{expected-value}

Let X be a random variable with a probability distribution f(x). The mean or expected value of X is

μ=E(X)=∑xxf(x)

if X is @discrete, and

μ=E(X)=∫−∞∞xf(x)dx

if X is continuous.

The expected value is the "average value" we expect the random variable to take in the long run.

Note that in the discrete case, the expected value is the dot product of the vector of x values and corresponding vector of f(x) values.

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Definition: Field \@{field}

A commutative division ring is called a field.

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Definition: Finite \@{finite}

A set A is said to be finite if A∼Nn for some n.

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Definition: First-order system (also: one-dimensional system) \@{first-order-system}

A first-order system is a system of the form

x˙=f(x),

where x=x(t) is a @real-valued function of time t, and f(x) is a smooth real-valued function of x.

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Definition: Formal System \@{formal-system}

A formal system F is an ordered quadruple

F=(Σ,W,A,R)

where:

  1. Σ is a finite, nonempty alphabet (a set of symbols);
  2. W⊆Σ∗ is the set of well-formed-formulas (wffs), defined inductively by formation rules specifying which finite strings over Σ belong to W
  3. A⊆W is a distinguished subset of W, whose members are called axioms.
  4. R is a finite set of rules of inference, each of which is a relation on W determining from which formulas other formulas may be derived.
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Definition: Four Fundamental Subspaces (also defines: Column space, Nullspace, Row space, left nullspace) \@{four-fundamental-subspaces}

Any m×n matrix A determines four @subspaces (each possibly containing only the zero vector):

  • The Column space, denoted C(A), consists of all linear combinations of the columns of A and is a vector in Rm.
  • The Nullspace, denoted N(A), consists of all solutions x of the equation Ax=0 and is a subspace of Rn.
  • The Row space, denoted C(A⊤), consists of all linear combinations of the rows of A and forms a subspace of Rn. We equate this with C(A⊤), the column space of the @transpose of A.
  • The left nullspace, denoted N(A⊤), which is a subspace of Rm.
Definition: Free vector \@{free-vector}

A vector whose endpoints are not fixed at particular points is called a free vector.

Definition: Function (also: mapping, map) \@{function}

Consider two sets, A and B, whose elements may be any objects whatsoever, and suppose that with each element x of A there is associated, in some manner, any element of B, which we denote by f(x). Then f is said to be a function from A to B.

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Definition: Generalized Binomial Coefficient \@{generalized-binomial-coefficient}

For any complex number n∈C and any integer k≥0, the generalized binomial coefficient is defined by

(nk)=n(n−1)(n−2)⋯(n−k+1)k!.

Definition: Geometric Distribution \@{geometric-distribution}

A geometric random variable is a discrete random variable that models the number of independent Bernoulli trials needed to achieve the first success. The probability of success is constant (denoted by p) and the trials are independent. The probability mass function is

P(X=k)=(1−p)k−1p,

for k=1,2,3…. k represents the number of independent trials it takes to achieve the first success, and p is the probability of any given trial being successful.

The mean is 1p and the variance is 1−pp2.

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Definition: Globally stable \@{globally-stable}

A fixed point x∗ that is approached from any starting position on the real line (other than that at x∗ itself) is said to be globally stable.

Definition: Gradient \@{gradient}

Given a scalar function f:Rn→R, the gradient of f, denoted as ∇f, is defined as the vector of its partial derivatives. Specifically, for a function f(x1,x2,⋯,xn), the gradient is given by

∇f=[∂f∂x1∂f∂x2 ⋮ ∂f∂xn]

Definition: Gradient System \@{gradient-system}

If a @system can be written in the form x˙=−∇V, for some continuously differentiable, single-valued scalar function V(x), then it is said to be a gradient system with potential function V.

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Definition: Greatest lower bound (also: infimum) \@{greatest-lower-bound}

There is also a concept of a greatest lower bound, which is a lower bound that is greater than or equal to every other lower bound. The greatest lower bound is also known as the infimum.

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Definition: group \@{group}

A group is a set G together with a binary operation ∗ such that:

Closure: The set is closed under the binary operation. For all a,b∈G,a∗b∈G.

Associativity: The binary operation is associative on the set. For all a,b,c∈G,(a∗b)∗c=a∗(b∗c).

Identity: The set contains an identity element, denoted e. For all a∈G,a∗e=a.

Inverses: All elements in the set have inverse elements in the set, denoted using a−1. For all a∈G there exists a−1∈G such that a∗a−1=e.

This set/operation combination G is commonly denoted as the pair (G,∗).

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Definition: Half-open Interval \@{half-open-interval}

A half-open interval (a,b] or [a,b) is the set of all real numbers such that a<x≤b or a≤x<b, respectively.

Definition: Half-stable \@{half-stable}

A fixed point x∗ where f′(x)=0 and the stability depends on which side of x∗ x0 lies on is called half-stable. It is denoted with a half-filled circle.

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Definition: Hamiltonian System \@{hamiltonian-system}

A Hamiltonian system is one where H(p,q) is a smooth, real-valued function and we have that

q˙=∂H∂p,p˙=−∂H∂q.

The function H is called the Hamiltonian.

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Definition: Hamming Distance \@{hamming-distance}

Given a string of m symbols, the Hamming Loss is the number of positions for which the symbols differ. For binary strings, this is

dH(y^,y)=∑i=1m|y^(i)−y(i)|.

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Definition: Hamming Loss \@{hamming-loss}

The Hamming Loss is the Hamming Distance divided by the length of the strings being compared. For strings of length m, it is

LHamming=1mdh(y^,y).

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Definition: Hessian Matrix (also: Hessian) \@{hessian-matrix}

Suppose f : Rn→R is a function taking as input a vector x∈Rn and outputting a scalar f(x)∈R. If all second-order partial derivatives of f exist, then the Hessian matrix H of f is a square n×n matrix, usually defined and arranged as

Hf=[∂2f∂x12∂2f∂x1∂x2⋯∂2f∂x1∂xn∂2f∂x2∂x1∂2f∂x22⋯∂2f∂x2∂xn⋮⋮⋱⋮∂2f∂xn∂x1∂2f∂xn∂x2⋯∂2f∂xn2].

That is, the entry of the ith row and the jth column is

(Hf)i,j=∂2f∂xi∂xj.

For a function f : R3→R, this is

H=[∂2f∂x2∂2f∂x∂y∂2f∂x∂z∂2f∂y∂x∂2f∂y2∂2f∂y∂z∂2f∂z∂x∂2f∂z∂y∂2f∂z2].

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Definition: Heteroclinc Trajectory \@{heteroclinc-trajectory}

Trajectories that connect two fixed point are called heteroclinic orbits.

Definition: Heteroclinic trajectories \@{heteroclinic-trajectories}

Pairs of orbits connecting twin @saddle-points are called heteroclinic trajectories.

Definition: Homeomorphism (also: homeomorphic) \@{homeomorphism}

A homeomorphism is a bijective and continuous function between @topological-spaces that has a continuous @inverse-function.

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Definition: Homoclinic orbit \@{homoclinic-orbit}

A trajectory that starts and ends at the same fixed point is called a homoclinic orbit.

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Definition: Homoclinic Orbit \@{homoclinic-orbit}

Trajectories that start and end at the same fixed point are called homoclinic orbits.

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Definition: homomorphism (group) \@{homomorphism-group}

A homomorphism is a map ϕ:G→G′ between groups (not necessarily a bijection), ⟨G,∗⟩ and ⟨G′,∗′⟩, that satisfies the homomorphism property:

ϕ(a∗b)=ϕ(a)∗′ϕ(b), ∀a,b∈G.

from Groups
Definition: Hyperbolic Fixed Point \@{hyperbolic-fixed-point}

A hyperbolic fixed point is a fixed point for which the real part of both eigenvalues is non-zero.

Definition: Hypergeometric Distribution \@{hypergeometric-distribution}

The Hypergeometric distribution is similar to the binomial distribution, but is performed without replacement. So, if success is drawing an ace from a deck of cards, in a Binomial situation the card drawn each trial would be put back into the deck; in the Hypergeometric it would not be. Thus, the trials for a Hypergeometric distribution are not independent.

A Hypergeometric experiment has the following properties:

  1. A random sample of size n is selected without replacement from N items.
  2. Of the N items, k may be classified as successes and N−k are classified as failures.

The number X of successes of a Hypergeometric experiment is called a Hypergeometric random variable, and its probability distribution is called the Hypergeometric distribution.

The probability distribution of X, the probability of x successes in n draws, without replacement, from a finite population of size N that contains exactly k successful items and N−k failure items, is

h(x,N,n,k)=(kx)(N−kn−x)(Nn),max(0,n−(N−k))≤x≤min(n,k).

The mean and variance of the Hypergeometric distribution h(x,N,n,k) are

μ=nkN and σ2=N−nN−1⋅n⋅kN(1−kN).

It's worth noting that when n is small compared to N, the lack of replacement in a hypergeometric process doesn't cause much impact to the distribution, and in these cases, the hypergeometric distribution is similar to the binomial distribution. In fact, for large values of N and small values of n, the binomial distribution approximates the hypergeometric distribution.

To do this approximation, just use the binomial PMF with p=k/N.

Definition: Identically Distributed \@{identically-distributed}

Given random variables X and Y, we say X and Y are identically distributed if they have the same probability law, i.e. X=dY if P(X∈A)=P(Y∈A)

for every measurable set A in their common state space. For discrete random variables this reduces to P(X=x)=P(Y=x) for every possible value of x. Equivalently, if they have the same probability mass function in the discrete case or the same cumulative distribution function in the real-valued case: FX(t)=FY(t) ∀t.

Definition: Identifiable \@{identifiable}

A parameterization π is identifiable if the @identity map on Θ satisfies the condition in Parameters Factor Through the Parameterization, that is, if π is injective. Then π−1:P→Θ is a parameter, the indexing parameter, and Θ is its range.

Definition: incompressible \@{incompressible}

Let v be the velocity vector of of the motion of particles in a fluid. If divv=0, then the fluid has constant density and is said to be incompressible.

Definition: Independent and Identically Distributed (also: i.i.d.) \@{independent-and-identically-distributed}

Random variables X1,…,Xn are said to be independent and identically distributed if they are mutually independent and identically distributed; equivalently, if their joint cumulative distribution function factors as FX1,…,Xn(x1,…,xn)=∏i=1nF(xi), where F is the @common cumulative distribution function shared by every Xi and x1,…,xn are real numbers.

Definition: index \@{index}

The number of left cosets of a subgroup H in a group G is the index (G:H) of H in G.

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Definition: Inference (also: prediction) \@{inference}

Applying a trained model fθ to an unseen x to produce a predicted @label is called inference or prediction.

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Definition: Injective (also: one-to-one, injection) (also defines: Surjective, Bijective) \@{injective}

A function f:A→B is

Injective (also: one-to-one, injection) if for all a,a′∈A,a≠a′⟹f(a)≠f(a′).
Surjective (also: onto, surjection) if for every b∈B there is an a∈A with f(a)=b.
Bijective (also: bijection) if f is both injective and surjective.
Definition: Inner product (also: Dot Product, Scalar product of two vectors) \@{inner-product}

If x and y are vectors in Rn, then their inner product is defined as

X⋅y=∑i=1nxiyi.

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Definition: Integers Notation: Z \@{integers}

The integers Z={…,−2,−1,0,1,2,…} are the natural numbers together with their negatives and zero.

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Definition: Interior Point \@{interior-point}

A point p is an interior point of E if there is a neighborhood N of p such that N⊂E.

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Definition: Inverse Image (also: pre-image, preimage) \@{inverse-image}

If f:A→B and E⊂(B), then f−1(E) denotes the set of all x∈A such that f(x)∈E. We call f−1(E) the inverse image of E under f.

Definition: Irrotational \@{irrotational}

If the curl of a vector field is 0, i.e. if curlv=0, the field is said to be irrotational.

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Definition: Isolated Point \@{isolated-point}

If p∈E and p is not a limit point of E, then p is called an isolated point of E.

Definition: Jacobian Matrix (also: Jacobian, Total Derivative) \@{jacobian-matrix}

Let f : Rn→Rm be a function such that each of its first-order partial derivatives exists on Rn. This function takes a point x=(x1,…,xn)∈Rn as input and produces the vector f(x)=(f1(x),…,fm(x))∈Rm as output. Then the Jacobian matrix of f, denoted Jf, is the m×n matrix whose (i,j) entry is ∂fi∂xj; explicitly

[∂f∂x1⋯∂f∂xn]=[∇Tf1⋮∇Tfm]=[∂f1∂x1⋯∂f1∂xn⋮⋱⋮∂fm∂x1⋯∂fm∂xn],

where ∇Tfi is the @transpose (@row-vector) of the gradient of the i-th component.

Definition: Joint Entropy \@{joint-entropy}

The joint entropy H(X,Y) of a pair of @discrete random variables (X,Y) with a joint distribution p(x,y) is defined as

H(X,Y)=−∑x∈X∑y∈Yp(x,y)log⁡p(x,y),

which can also be expressed as

H(X,Y)=−E[log⁡p(X,Y)].

Definition: Joint Probability Distribution (also: joint distribution, joint probability mass function, joint probability) \@{joint-probability-distribution}

Two random variables X and Y can be paired as a single random vector or bivariate random variable. If it's discrete (i.e. both X and Y are discrete) it has a joint probability mass function and if it's continuous (X and Y are both continuous) it has a joint probability density function.

In the discrete case, f(x,y)=P(X=x,Y=y).

Definition: k-cell \@{k-cell}

Given a,b∈Rk, if ai<bi for all i=1,2,…,k, then the set of all points x who satisfy ai≤xi≤bi, i=1,2,…,k, is called a k-cell. So, a 1-cell is an interval, a 2-cell is a rectangle, and so on.

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Definition: kernel \@{kernel}

The kernel of a homomorphism ϕ is the set of elements that ϕ sends to e′, and it is denoted by ker⁡(ϕ). It is a normal subgroup of G.

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from Groups
Definition: KL Divergence (also: relative-entropy, Kullback-Leibler divergence) \@{kl-divergence}

For discrete probability distributions, p and q, on a common alphabet X, the relative entropy from q to p is defined to be

DKL(p‖q)=∑x∈Xp(x)log⁡p(x)q(x),

which is just cross-entropy minus entropy:

D(p‖q)=H(p,q)−H(p).

Note that we don't always use the KL subscript where it's obvious from the context.

We can also write it as

D(p‖q)=Ep[−log⁡q]−Ep[−log⁡p]=Ep[log⁡pq],

which makes it clear that it's the expected inefficiency in an encoding optimized for q rather than p.

Definition: Known \@{known}

The population P is known if and only if P(A) is a known value for every event A∈F.

Definition: Laplacian \@{laplacian}

The Laplace operator is a second-order differential operator in the n-dimensional Euclidean space, defined as the divergence (∇⋅) of the gradient (∇f). Thus, if f is a twice differentiable real-valued function, then the Laplacian of f is the real-valued function defined by

Δf=∇2f=∇⋅∇f.

The Laplacian of f is the sum of all the unmixed second partial derivatives in the Cartesian coordinates xi:

∇2f=∑i=1n∂2f∂xi2.

In two dimensions, using Cartesian coordinates, the Laplace operator is given by

∇2f=∂2f∂x2+∂2f∂y2

and in three dimensions by

∇2f=∂2f∂x2+∂2f∂y2+∂2f∂z2

Definition: Layer \@{layer}

A layer in a neural network is a collections of neurons that operate in parallel on the same input vector.

A layer with nℓ−1 inputs and nℓ neurons defines a function

Fℓ:Rℓ−1→Rℓ

of the form

Fℓ(x)=ϕℓ(Wℓx+bℓ),

where:

  • Wℓ∈Rnℓ×nℓ−1 is the weight matrix (with the ith row representing the weights for the inputs to the ith neuron in the layer),
  • bℓ∈Rnℓ is the bias vector (with the ith entry representing the bias on the ith neuron in the layer,
  • ϕℓ:R→R is an activation function, applied @componentwise,
  • each coordinate of Fℓ(x) is the output of a single neuron in that layer.

A layer takes an input vector, applies the same affine transformation to all neurons (via a shared weight matrix and bias vector), and then applies an @activation-function to each neuron's output.

Its output is the vector of all neuron outputs in that layer, and in this way, we can view a layer as a vector of neurons.

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Definition: Least upper bound (also: supremum) \@{least-upper-bound}

The number L is said to be the least upper bound of the set A if it's an upper bound of A and if L≤m for all upper bounds m of A.

The least upper bound is also known as the supremum.

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Definition: Left Stochastic Matrix (also: column stochastic matrix) \@{left-stochastic-matrix}

A left stochastic matrix is a @square-matrix A=(aij)∈Rn×n with non-negative entries whose columns each sum to one: aij≥0for all i,j,∑iaij=1for all j. Equivalently, 1⊤A=1⊤ with A≥0 entrywise, where 1 is the all-ones vector.

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Definition: length of open interval Notation: ℓ \@{length-of-open-interval}

The length ℓ(I) of an @open interval I is defined by

{b−a if I=(a,b) for some a,b∈R with a<b,0 if I=∅,∞ if I=(−∞,a) or I=(a,∞) for some a∈R,∞ if I=(−∞,∞)

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Definition: Level Surface \@{level-surface}

Let S be a surface represented by f(x,y,z)=c, where c is constant and f is differentiable. Such a surface is called a level surface of f, and for different c, we get different level surfaces.

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Definition: Liapunov Function (also: Lyapunov function) \@{liapunov-function}

Consider a system x˙=f(x) with a fixed point at x∗. If it has a function with the following properties:

  1. V(x)>0 for all x≠x∗, and V(x∗)=0. (i.e. V is @positive-definite.)
  1. V˙<0 for all x≠x∗. (All trajectories flow "downhill" toward x∗.

Then such a function is called a Liapunov function.

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Definition: Limit \@{limit}

Let X and Y be metric spaces; suppose E⊂X, f:E→Y, and p is a limit point of E. We write f(x)→q as x→p, or

limx→pf(x)=q

if there is a point q∈Y with the following property: For every ϵ>0, there exists a δ>0 such that

dY(f(x),q)<ϵ

for all points x∈E for which

0<dX(x,p)<δ.

Definition: Limit cycle \@{limit-cycle}

A limit cycle is an isolated closed trajectory. Isolated means that @neighboring trajectories are not closed; they spiral toward or away from the limit cycle.

Definition: Limit Point \@{limit-point}

A point p is a limit point of the set E if every neighborhood of p contains a point q≠p such that q∈E.

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Definition: Line Integral \@{line-integral}

If f is defined on a smooth curve C given by x=x(t),y=y(t),a≤t≤b, and f if defined on C, then the line integral of f along C is defined as:

∫Cf(x,y)ds=limn→inf∑i=1nf(xi,yi)Δsi

Definition: Line Integral of Vector Function \@{line-integral-of-vector-function}

A line integral of a vector function F(r) over a curve C:r(t) is defined by

∫CF(r)⋅dr=∫abF(r(t))⋅r′(t)dt(a)

where r(t) is the parametric representation of C.

Writing (a) in terms of components, with dr=[dx,dy,dz] and ′=d/dt, we get

∫C∫CF(r)⋅dr=∫C(F1dx+F2dy+F3dz)=∫ab(F1x′+F2y′+F3z′)dt).

Definition: Linear Function (also: linear map, linear transformation) \@{linear-function}

TODO: define this.

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Definition: Linear Transformation (also: linear) (also defines: additivity, homogeniety) \@{linear-transformation}

Let V and W be vector spaces over a field F. We call a function

T:V→W a linear transformation from V to W if for all x,y∈V and all c∈F, we have

  1. (a) T(x+y)=T(x)+T(y) and
  2. (b) T(cx)=cT(x)

The first condition is called additivity and the second is called homogeniety.

Definition: Lipschitz Continuous (also defines: Lipschitz constant, K-Lipschitz) \@{lipschitz-continuous}

Given two metric spaces (X,dX) and (Y,dY), a function f:X→Y is called Lipschitz continuous if there exists a real constant K≥0 such that, for all x1,x2∈X,

dY(f(x1),f(x2))≤KdX(x1,x2).

Any such K is referred to as a Lipschitz constant for the function f, and f may also be referred to as K-Lipschitz.

Definition: Log Probability \@{log-probability}

A log probability is just a logarithm of a probability.

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Definition: Logarithm \@{logarithm}

For b>1, y>0 the unique real x such that bx=y is called the logarithm of y to the base b and is denoted as

logb⁡(y).

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Definition: Lower bound \@{lower-bound}

The number m is said to be a lower bound of a nonempty set A if x≥m for all x∈A.

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Definition: Maclaurin series \@{maclaurin-series}

The special case of the Taylor series in which z0 = 0

f(z)=∑n=0∞f(n)(0)n!zn

is called the Maclaurin series of f.

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Definition: Magnitude (also: norm, length) \@{magnitude}

Let x=(x1,x2,⋯,xn)∈Rn. The magnitude, or length, x is denoted as ‖x‖ and is defined as:

‖x‖=x12+x22+⋯+xn2=x⋅x=∑i=1nxi2

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Definition: Manifold \@{manifold}

A manifold is a @topological-space that resembles @euclidean-space near each point. That is, an n-dimensional manifold is a topological space with the property that each point has a neighborhood that is homeomorphic to an open subset of n-dimensional Euclidean space.

Definition: Marginalization (also: marginal distribution, marginal probability mass function) \@{marginalization}

We can marginalize over Y to find solely the distribution of X, we denote this fX(x) and give it as

fX(x)=∑yf(x,y).

We can similarly find fY(y) by marginalizing over X:

fY(y)=∑xf(x,y).

Definition: Markov Chain \@{markov-chain}

If we have a system with N states and for each state, a set of N probabilities from transitioning from that state to another state (including itself) we end up with an N×N matrix P where the entry Pjk,j,k∈{1,…,N} represents the probability of transitioning from state j to state k.

Starting with some state, we can transition to another state, then another, with the probability of picking the next state dependent only on the existing state and the matrix P. We call this sequence of random events a Markov Chain.

More formally, the sequence or random variables X1,X2,…,Xn is called a Markov Chain if

P(Xn+1=k|Xn=j,Xn−1=jn−1,…,X0=j0)=P(Xn+1=k|Xn=j).

We write

pjk=P(Xn+1=k|Xn=j),

and note that

pjk≥0

and

∑k=1Npjk=1

for j=1,2,…,N. We call the pjk values the transition probabilities of the Markov chain.

Alternatively, we can say the sequence or random variables X,Y,Z is said to form a Markov Chain (denoted X→Y→Z) if and only if X and Z are conditionally independent given Y. Specifically, X,Y and Z form a Markov Chain X→Y→Z if the joint probability mass function can be written as

p(x,y,z)=p(x)p(y|x)p(z|y).

Definition: matrix product (also: product, matrix multiplication) \@{matrix-product}

Let A be an m×n matrix and B be an n×p matrix. We define the product of A an B, denoted AB, to be the m×p matrix such that

(AB)i,j=∑k=1nAi,kBk,jfor 1≤i≤m,1≤j≤p.

Definition: Membership criterion \@{membership-criterion}

The membership criterion for a set X is a statement of the form x∈X⟺P(x), where P(x) is a proposition that is true for precisely for those objects x that are elements of X, and no others.

Definition: Metric Space \@{metric-space}

A set X, whose elements we'll call points, together with a distance function d:X×X→R is called a metric space and the distance function d is called a metric, if the following conditions, called the metric axioms, hold for p,q,r∈X:

  • If p≠q,d(p,q)>0. (distance is always positive between two distinct points.)
  • d(p,p)=0. (distance is always zero between a point and itself.)
  • d(p,q)=d(q,p). (the distance from p to q is the same as the distance from q to p.)
  • d(p,q)≤d(p,r)+d(r,p) (triangle inequality.)

We can denote a metric space on set X with metric d as the tuple (X,d).

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Definition: Minimal Sufficient Statistic \@{minimal-sufficient-statistic}

A statistic T(X) is a minimal sufficient statistic relative to {fθ(x)} if it is a function of every other sufficient statistic U.

Definition: Model pipeline (also: classifier pipeline) \@{model-pipeline}

This overall process of preparing features, training fθ, and evaluating results is called a classifier pipeline or model pipeline.

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Definition: Model Training (also: learning) \@{model-training}

Then, the job of machine learning in binary classification is to produce a good function f. This is called model training or learning. More formally, if fθ(x):Rn→0,1 is a parameterized function, model training is the task of minimizing loss, that is, we want to find the set of parameters θ that minimizes

∑i=1mL(fθ(x(i)),y(i))

where L is a loss function, for example, cross-entropy loss.

Definition: Moment Generating Function \@{moment-generating-function}

If X is a random variable, then its moment generating function is a real-valued function on the reals defined as

MX(t)=E[etX].

If X is discrete, this is then

MX(t)=∑xetxf(x)

and if X is continuous, then this is

MX(t)=∫−∞∞etxf(x).

Definition: Multiclass Classification (also: multinomial classification) \@{multiclass-classification}

Multiclass classification is the task of putting things into one of three or more classes.

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Definition: Multinomial Coefficient \@{multinomial-coefficient}

The multinomial distribution uses the multinomial coefficient, which is defined as

(nn1,n2,…,nr)=n!n1!n2!⋯nr!.

Definition: Multinomial Distribution \@{multinomial-distribution}

For a sequence of n independent, identical experiments with each one of the experiments resulting in r outcomes with probabilities p1,p2,…,pr, respectively, where ∑i=1rpi=1, we let Xi count the number of the n experiments that result in the ith of the r outcomes. Then

P(X1=n1,X2=n2,…,Xr=nr)=(nn1,n2,…,nr)p1n1p2n2⋯prnr,

where ∑i=1rni=n.

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Definition: Multiplicative Inverse \@{multiplicative-inverse}

For some element a in a ring with unity R where 1≠0, if a−1∈R such that aa−1=a−1a=1, a−1 is said to be the multiplicative inverse of a.

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Definition: Mutual Independence (also: mutually independent) \@{mutual-independence}

Random variables X1,…,Xn are said to be mutually independent if their joint cumulative distribution function factors as FX1,…,Xn(x1,…,xn)=∏i=1nFXi(xi) for all x1,…,xn∈R, where FXi(x)=P(Xi≤x) is the cumulative distribution function of Xi.

Events A1,…,An are said to be mutually independent if P(⋂i∈SAi)=∏i∈SP(Ai) for every S⊆[n] with |S|≥2, where [n]={1,…,n} and |S| denotes the number of elements of S.

An infinite collection is said to be mutually independent if every finite subfamily is.

Definition: Mutual Information \@{mutual-information}

Consider two random variables X and Y with joint probability mass function p(x,y) and marginal probability mass functions p(x) and p(y). The mutual information I(X;Y) is the relative-entropy between the joint distribution and the product distribution p(x)p(y):

I(X;Y)=∑x∈X∑y∈Yp(x,y)log⁡p(x,y)p(x)p(y)=D(p(x,y)‖p(x)p(y))=Ep(x,y)log⁡p(X,Y)p(X)p(Y).

Definition: n-tuple \@{n-tuple}

An object of the form (a1,a2,…,an) where the entries a1,a2,…,an are elements of a field F, is called an n-tuple with

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Definition: Natural Numbers (also: naturals) Notation: N \@{natural-numbers}

The natural numbers N={1,2,3,…} are the counting numbers.

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Definition: Negative Binomial Distribution \@{negative-binomial-distribution}

The negative binomial random variable generalizes the geometric random variable by giving the probability that it takes n independent trials to get r successes. Its pmf is

P(X=n)=(n−1r−1)pr(1−p)n−r.

Definition: Neighborhood \@{neighborhood}

A neighborhood, or r-neighborhood of p is a set Nr(p) consisting of all q such that d(p,q)<r for some r>0. This subset of X is all the points within a circle of radius r - the open ball of radius r centered at p.

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Definition: Neural Network \@{neural-network}

A neural network is a function obtained by @composing @finitely-many neurons arranged in layers:

F(x)=(ϕL∘AL)∘⋯∘(ϕ1∘A1)(x),

where each

  • ϕℓ is an @activation-function applied @componentwise,
  • and Wℓ,bℓ are learnable parameters.
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Definition: Neuron \@{neuron}

In a neural network, a neuron N is a computation unit that takes n input values, applies an affine transformation, then a typically non-linear activation function, and returns a single value.

That is, it is a function of the form

N:Rn→R,N(x)=ϕ(w⋅x+b),

where

  • n is the number of inputs to the neuron
  • w∈Rn is a vector of weights,
  • b∈R is a bias value, and
  • ϕ:R→R is an activation function.
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Definition: normal \@{normal}

A subgroup H of a group G is normal if its left and right cosets coincide, that is, if gH=Hg, i.e. gHg−1=H, for all g∈G.

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from Groups
Definition: Normal Derivative \@{normal-derivative}

The normal derivative is the directional derivative in the direction of the @normal-vector.

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Definition: Normal Distribution \@{normal-distribution}

The normal distribution or Gaussian distribution is the classic bell-shaped distribution.

The density of the normal random variable X, with mean μ and variance σ2, is

n(x;μ,σ)=12πσe−12σ2(x−μ)2,−∞<x<∞.

The mean and variance of n(x;μ,σ) are μ and σ2, respectively.

Definition: Null and Alternative Hypotheses \@{null-alternative-hypothesis}

We could say that our null hypothesis is that the population mean is what we expect:

H0:μ=μ0,

and that the alternative hypothesis is that it is different from what we expect:

H1:μ≠μ0.

Definition: Null Space (also: kernel) (also defines: range of a linear transformation) \@{null-space}

Let V and W be vector spaces and let T:V→W be linear.

We define the null space (also: kernel) N(T) of T to be the set of all vectors x∈V such that T(x)=0, that is, N(T)={x∈V:T(x)=0.}

We define the range of a linear transformation (also: image of a linear transformation) R(T) of T to be the subset of W consisting of all @images (under T) of vectors in V, that is, R(T)={T(x):x∈V}.

Definition: Nullcline \@{nullcline}

The nullclines of a planar system are the curves where either x˙=0 or y˙=0 and indicate where the flow is either purely horizontal or purely vertical. fixed points occur at intersections of nullclines.

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Definition: odd (permutation) \@{odd-permutation}

A permutation of a finite set is odd if it is the product of an odd number of transpositions.

from Groups
Definition: Odds Notation: odds \@{odds}

The odds of an event A occurring are defined as

odds(A)=P(A)P(Ac)=P(A)1−P(A)

that is, the probability A occurs divided by the probability of the complement of A (i.e., the probability that A does not occur.)

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Definition: Open \@{open}

A set E is open if every point of E is an interior point of E.

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Definition: Open Cover \@{open-cover}

An open cover of a set E in a metric space X is a collection {Gα} of open subsets of X such that E⊂⋃αGα.

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Definition: Open Relative \@{open-relative}

Suppose E⊂Y⊂X, and X is a metric space. We say that E is open relative to Y if to each p∈E there is associated an r>0 such that q∈E,q∈Y whenever d(p,q)<r.

Definition: orbit \@{orbit}

Let σ be a permutation of A. The equivalence classes in A determined by the equivalence relation "~" are the orbits of σ.

from Groups
Definition: orbit (also: solution) \@{orbit}

A sequence (x0,x1,x2,…) is called the orbit (or solution) starting from x0. This is analogous to a trajectory in a continuous time dynamical system.

Definition: orbit containing a point \@{orbit-containing-a-point}

Let σ be a permutation of A, the orbit of σ containing a∈A is the set

{⋯,σ−2(a),σ−1(a),a,σ(a),σ2(a),⋯}={σn(a)|n∈Z}.

So, a,b∈A are in the same orbit of σ, written as a∼b, if and only if b=σn(a) for some n∈Z.

The relation "~" is an equivalence relation (reflexive, symmetric, transitive). This means A can be partitioned into orbits of σ.

from Groups
Definition: order \@{order}

The order of a finite group is the number of its elements. The order of group G is denoted as ord(G) or |G|. The order of an element a (also called period length or period) is the number of elements in the subgroup generated by a, and is denoted by ord(a) or |a|.

from Groups
Definition: outer measure \@{outer-measure}

The outer measure |A| of a set A⊂R is defined by

|A|=inf{∑k=1∞ℓ(Ik):I1,I2,… are open intervals such that A⊂⋃k=1∞Ik}.

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Definition: p-value \@{p-value}

The p-value is the probability of getting a test statistic (z) this extreme or more extreme if the actual mean is μ0.

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Definition: Pairwise Independence (also: pairwise independent) \@{pairwise-independence}

Random variables X1,…,Xn are said to be pairwise independent if Xi and Xj are independent for every {i,j}∈([n]2), that is, if FXi,Xj(x,y)=FXi(x)FXj(y) for all x,y∈R, where FXi,Xj(x,y)=P(Xi≤x,Xj≤y) is the joint cumulative distribution function of the pair.

Events A1,…,An are said to be pairwise independent if P(Ai∩Aj)=P(Ai)P(Aj) for every {i,j}∈([n]2).

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Definition: Parallel \@{parallel}

Two vectors x and y are said to be parallel if x is a scalar multiple of y, i.e., if there exists some scalar c where x=cy.

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Definition: Parameter \@{parameter}

Let P be a statistical model. A parameter is a function ϑ:P→Λ into some set Λ. For P∈P, the element ϑ(P) is the value of the parameter at P.

Definition: Parameter Space \@{parameter-space}

The parameter space of a parameterization π:Θ→P is its domain Θ.

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Definition: Parameterization \@{parameterization}

A parameterization of a statistical model P is a surjective map π:Θ→P written Pθ=π(θ).

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Definition: Parametric Family \@{parametric-family}

A statistical model P on a measurable space (Ω,F) is a parametric family if it has a parameterization θ↦Pθ whose parameter space satisfies Θ⊆Rd for some fixed positive integer d.

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Definition: Partial Derivative \@{partial-derivative}

Using the setup from the definition of component, for x∈E,1≤i≤m,1≤j≤n, we define

(Djfi)(x)=limt→0fi(x+tej)−fi(x)t,

provided the limit exists. Writing fi(x1,…,xn) in place of fi(x), we see that Djfi is the derivative of fi with respect to xj, keeping the other variables fixed. The notation

∂fi∂xj

is therefore often used in place of Djfi, and Djfi is called a partial derivative.

Definition: Path Independent (also: independent of path) \@{path-independent}

We say that line integral 4.7 is independent of path in a domain D if for any two points A and B in D, the value of the line integral is the same for all piecewise smooth curves in D from A to B.

Definition: permutation multiplication \@{permutation-multiplication}

Permutations can be "multiplied", which is just composition. So if we have two permutations on A, called σ and τ, στ means their multiplication, and we apply from right to left, so τ applies first and then σ. The result will also be a permutation in A.

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from Groups
Definition: Phase Portrait \@{phase-portrait}

A drawing that shows the different trajectories taken from different phase points in a system is called a phase portrait.

Definition: Point Singularity (also: Isolated Singularity) \@{point-singularity}

A singularity z0 of a complex function f is said to be a point singularity or isolated singularity if there exists a neighborhood of z0 in which z0 is the only singularity of f.

Alternatively, a point singularity of a function f is a complex number z0 such that f is defined in a neighborhood of z0 but not at the point z0 itself.

Definition: Poisson Distribution \@{poisson-distribution}

Experiments that give numerical values of a random variable X, the number of outcomes during a given time interval or in a specified region, are called Poisson experiments. For example, the number of phone calls per hour an office receives or the number of field mice per acre in a pasture. Note that while binomial and hypergeometric experiments dealt with discrete sequence of events (and give probabilities for discrete outcomes), Poisson experiments deal with continuous domains (and also give probabilities for discrete outcomes).

A Poisson process possesses the following properties

  1. The number of outcomes occurring in one time/space region is independent of the number of outcomes occurring in any other disjoint time/space region, i.e., the Poisson process has no memory.
  2. The probability that a single outcome will occur within a small region is proportional to the size of the region and does not depend on the number of outcomes occurring outside the region, or the relative position of the region.
  3. In a very small region, the probability of more than one event occurring is negligible.

The probability distribution of the Poisson random variable X, representing the number of outcomes occurring in a given time interval or specified region denoted by t, is

p(x,λt)=e−λt(λt)xx!.

Both the mean and variance of the Poisson distribution p(x,λt) are λt.

Definition: Pole \@{pole}

A pole is present if the Laurent series has a finite number of negative power terms. The largest negative exponent (in absolute value) indicates the order of the pole.

Definition: Potential Function \@{potential-function}

A potential function is a scalar function whose gradient is a vector field. They allow representing certain vector fields in a simpler, more fundamental form.

In other words, given a vector field F, a potential function ϕ is a scalar function such that

F=−gradϕorF=gradϕ.

Definition: Power Series \@{power-series}

A power series in powers of z−z0 is a series of the form

∑n=0∞an(z−z0)n=a0+a1(z−z0)+a2(z−z0)2+⋯,

where z is a complex variable, a0,a1,…, are complex constants, called the coefficients of the series, and z0 is a complex constant, called the center of the series.

Definition: Probability \@{probability}

Note: This applies to sample spaces of discrete events and is a bit hand wavy.

We can assign a probability or weight to each sample point in a sample space by giving it a value ranging from 0 to 1. Events that are more likely to occur have a probability closer to 1, and events that are less likely to occur have a probability closer to 0. We give a probability to all sample points in a sample space such that the sum of the probabilities of all sample points in a sample space is 1.

Then, the probability of an event A is the sum of the probabilities of all sample points in A. Therefore,

0≤P(A)≤1,P(∅)=0,P(S)=1.

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Definition: Probability Density Function \@{probability-density-function}

The function f(x) is a probability density function (pdf) for the continuous random variable X, defined on the reals, if

  1. f(x)≥0 for all x∈R
  2. ∫−∞∞f(x)dx=1
  3. P(a<X<b)=∫abf(x)dx
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Definition: Probability Distribution (also: probability mass function, probability function) \@{probability-distribution}

A discrete random variable takes each of its values with a certain probability. The function f(x) that gives the probability of each value x of a random variable X occurring is called the probability function, probability mass function, or probability distribution. More formally, the set of ordered pairs (x,f(x)) is a probability distribution of the discrete random variable X if, for each possible outcome x:

  1. f(x)≥0
  2. ∑xf(x)=1
  3. P(X=x)=f(x)
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Definition: Probability of Error \@{probability-of-error}

Given a discrete random variable X, if X^ is an estimate of X, then we define the probability of error as

Pe=Pr(X^≠X).

Definition: Product Distribution (also: product measure) \@{product-distribution}

A probability distribution μ on X1×⋯×Xn is a product distribution if there are distributions μ1,…,μn on X1,…,Xn respectively such that μ(x1,…,xn)=∏i=1nμi(xi) for every tuple (x1,…,xn).

Such a distribution is written μ1⊗⋯⊗μn, or μ⊗n when every factor is equal to a common distribution μ.

Definition: projection (also: vector projection, orthogonal projection) (also defines: scalar projection, rejection) \@{projection}

Take two vectors in Rn, u and v, with v≠0.

The scalar projection (also: scalar component) of u onto b is a scalar equal to a1=‖a‖cos⁡θ, where θ is the @angle between a and b. It is denoted as follows, with an equivalent formula:

compvu=‖projvu‖=⟨u,v⟩‖v‖

The projection of u onto v is the vector whose magnitude is the scalar projection of u onto v with the same direction as v:

projvu=⟨u,v⟩‖v‖2v=(‖a‖cos⁡θ)b^.

The rejection (also: vector rejection) of u from v is the component of u that is orthogonal to v and is given as

oprojvu=u−projvu.

Definition: Random Variable (also: variate) \@{random-variable}

A random variable is a function that maps from a sample space to a state space. Often, but not always, the state space is a set of real numbers. For sample space Ω, we have X:Ω→X and for ω∈Ω, we have x=X(ω), where x is a value of the random variable and an element of the state space X.

In other words, a random variable is a function whose domain is a sample space and whose @codomain is a state space (called an alphabet when the state space is @discrete).

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Definition: Range (sequence) \@{range-sequence}

The set of all points pn of a sequence {pn}(n=1,2,3,…) is the range of {pn}.

Definition: rank (also defines: nullity) Notation: rank \@{rank}

Let V and W be vector spaces and let T:V→W be linear. If N(T) and R(T) (null space and range of T, respectively) are @finite dimensional, the we define the nullity of T, denoted nullity(T), and the rank of T, denoted rank(T), to be the @dimensions of N(T) and R(T), respectively.

Definition: Real Numbers (also: reals) Notation: R \@{real-numbers}

The real numbers R are a set of objects along with two binary operations +:R×R→R and ⋅:R×R→R that satisfy the 9 field axioms along with the Order axiom and the Completeness axiom. That is, the reals are an ordered, complete field.

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Definition: Real Sequence \@{real-sequence}

A real sequence of numbers if a function f from N to R.

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Definition: recursive \@{recursive}

The system F is said to be recursive (or effectively generated) if W, A, and R are all @recursively-enumerable sets, so that derivations can be verified by a finite mechanical procedure.

Definition: Removable Singularity (also: removable) \@{removable-singularity}

A removable singularity occurs if all negative powers in the Laurent series are zero and the function can be redefined at the singularity to be analytic.

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Definition: Residue \@{residue}

Given a convergent @laurent-series

f(z)=∑n=0∞an(z−z0)n+b1z−z0+b2(z−z0)2+⋯,

the coefficient b1 of the first negative power of 1/(z−z0) is called the residue of f(z) at z=z0. It is denoted by

b1=Resz=z0f(z).

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Definition: Reversible System \@{reversible-system}

A reversible system is any second-order system that is invariant under t→−t and y→−y.

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Definition: Ring \@{ring}

A ring is a set together with two binary operations + and ⋅, which we will call addition and multiplication, such that the following axioms are satisfied:

  1. ⟨R,+⟩ is an Abelian group.
  1. Multiplication is associative.
  1. For all a,b,c∈R, the left distributive law and the right distributive law hold, i.e.

a⋅(b+c)=(a⋅b)+(a⋅c),(a+b)⋅c=(a⋅c)+(b⋅c).

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Definition: Ring Homomorphism \@{ring-homomorphism}

A ring homomorphism ϕ:R→R′ must satisfy the following two properties:

  1. ϕ(a+b)=ϕ(a)+ϕ(b).
  1. ϕ(ab)=ϕ(a)ϕ(b).
Definition: Ring with Unity \@{ring-with-unity}

A ring that has a multiplicative identity element is called a ring with unity.

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Definition: Saddle-Node \@{saddle-node}

The defining feature of a saddle-node bifurcation is that as r crosses the bifurcation point, two fixed points are created or destroyed (depending on the direction of approach.) If approaching from the direction in which the fixed points exist, they will grow closer to each other, until they reach other at the bifurcation point, forming a half-stable point, and then they will be destroyed as r continues on the other side of the bifurcation point.

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Definition: Sample \@{sample}

A data set or the @random element that produces the data is called a sample from P.

Definition: Sample Size \@{sample-size}

The size of the data set is called the sample size.

Definition: Sample Space \@{sample-space}

The set of all possible outcomes of a statistical experiment is called the sample space and is represented by the symbol S. Each outcome in a sample space is called an element or member of the sample space or simply a sample point.

A sample space must be non-empty.

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Definition: Scalar \@{scalar}

A scalar is an element of a field used to define a vector space.

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Definition: Scalar Function (also: scalar field) \@{scalar-function}

Let P be any point in a domain of definition. Then we define a scalar function f, whose values are scalars, that is,

f=f(p)

that depends on P.

A scalar function depends only on the point P, not on the coordinate system chosen to represent it.

Definition: Segment \@{segment}

A segment (a,b) is the set of all real numbers x such that a<x<b.

Definition: Self-Information (also: surprisal, Shannon information, Information content) \@{self-information}

Given a real number b>1 and an outcome x of a discrete random variable X with probability mass function p, the self-information of x is defined as the negative log probability

I(x):=−logb⁡p(x).

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Definition: Separated \@{separated}

Two subsets A and B of a metric space X are said to be separated if both A∩B― and A―∩B are empty, i.e., if no point of A lies in the closure of B and no point of B lies in the closure of A.

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Definition: Separatrix \@{separatrix}

A separatrix is the boundary that separating two modes of behavior in a dynamical system.

Definition: Sequence \@{sequence}

A sequence is a function f defined on the set J of all positive integers.

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Definition: Set (also: collection, family) \@{set}

A set is a collection of objects, considered as a whole.

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Definition: simple \@{simple}

A group G is simple if it has no proper nontrivial normal subgroups, that is, if |G|>1 and the only normal subgroups of G are {e} and G itself.

from Groups
Definition: Singularity \@{singularity}

A point z0 is called a singularity of a complex function f if f is not analytic at z0, but every neighborhood of z0 contains at least one point at which f is analytic.

Definition: Stable \@{stable}

A fixed point where nearby points flow towards it is said to be stable.

Definition: Stable limit cycle (also: attracting limit cycle) \@{stable-limit-cycle}

If all neighboring trajectories approach the limit cycle, we say the limit cycle is stable or attracting.

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Definition: Standard Deviation \@{standard-deviation}

The positive square root of the variance, σ, is called the standard deviation of X.

Definition: Standard Normal Distribution \@{standard-normal-distribution}

The standard normal distribution is the distribution of a normal random variable with mean 0 and variance 1. We can transform a normal random variable X into a standard normal random variable by

Z=X−μσ.

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Definition: State Space (also: alphabet) \@{state-space}

The set of values a random variable can take is called its state space.

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Definition: Statistic \@{statistic}

Assume that we have a data set that is a realization of a sample X (a @random vector) from an unknown population P on a @probability space.

A @measurable function of X, T(X), is called a statistic if T(X) is a known value whenever X is known, i.e., the function T is a known function (i.e. T doesn't depend on the unknown P.)

Definition: Statistical Model \@{statistical-model}

A statistical model P is a collection of @probability measures on a common measurable space (Ω,F).

Equivalently, P⊆P(Ω,F), where P(Ω,F) denotes the set of all probability measures on (Ω,F).

In other words, a statistical model is a set of populations constrained by some set of assumptions about the populations, or, is the assumptions themselves.

Definition: statistical problem \@{statistical-problem}

In a statistical problem, the population P is at least partially unknown and we would like to deduce some properties of P based on the available sample.

Definition: Stochastic Matrix (also: probability matrix, transition matrix, Markov matrix, right stochastic matrix, row stochastic matrix) \@{stochastic-matrix}

A stochastic matrix (actually, a right stochastic matrix) is a @square-matrix A=(aij)∈Rn×n with non-negative entries whose rows each sum to one:

aij≥0for all i,j,∑jaij=1for all i.

Equivalently, A1=1 with A≥0 entrywise, where 1 is the all-ones vector.

Definition: Strictly Convex Function \@{strictly-convex-function}

Starting with convex function, φ is strictly convex if the inequality is strict whenever x≠y.

Definition: Subsequential limit \@{subsequential-limit}

If a subsequence {pni} of {pn} converges, its limit (sequence) is called a subsequential limit of {pn}.

Definition: subset \@{subset}

If X and Y are sets such that every element of X is also an element of Y, then we say X is a subset of Y, denoted as X⊂Y. Formally,

X⊂Y⟺(∀x)(x∈X⟹x∈Y)

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Definition: Sufficient Statistic \@{sufficient-statistic}

A function T(X) is said to be a sufficient statistic relative to the family {fθ(x)} if X is conditionally independent of θ given T(X) for any probability distribution on θ, that is, θ→T(X)→X forms a Markov chain.

Definition: superset \@{superset}

If X and Y are sets such that every element of Y is also an element of X, then we say X is a superset of Y, denoted as X⊃Y. This is the same as Y⊂X.

Definition: Surface Integral over Vector Field (also: surface integral, flux integral) \@{surface-integral-over-vector-field}

Given a piecewise smooth surface S, we can parameterize it as

r(u,v)=⟨x(u,v),y(u,v),z(u,v)⟩=x(u,v)i+y(u,v)j+z(u,v)k,

with u0≤u<u1 and v0≤v≤v1 (i.e. u and v vary over a region R in the uv-plane).

Now, S has a @normal-vector and unit @normal-vector, respectively, as

N=ru×rv,n=1|N|N

at every point, except perhaps for some edges or cusps, such as for cubes and cones. For a given vector function F we can now define the surface integral over S by

∬SF⋅ndA=∬RF(r(u,v))⋅N(u,v)dudv.

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Definition: Surface Normal \@{surface-normal}

Given a tangent plane to a surface S at P, the normal to this plane (the straight line through P perpendicular to the tangent plane) is called the surface normal to S at P.

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Definition: Surface Normal Vector \@{surface-normal-vector}

A vector in the direction of the surface normal of a surface S at point P is called a surface normal vector of S at P.

Definition: symmetric group \@{symmetric-group}

When A is the finite set {1,2,3,⋯,n}, the group of all permutations of A is the symmetric group on n letters, and is denoted by Sn. It has n! elements.

from Groups
Definition: System of Differential Equations \@{system-of-differential-equations}

A system of differential equations is a collection of one or more equations relating the derivatives of one or more functions. It is required that all the functions in the system depend on the same set of variables.

Definition: Tangent Plane \@{tangent-plane}

If S is a level surface of a function f, and P is a point of S, then the set of all tangent vectors of all curves passing through P will generally form a plane, called the tangent plane of S at P.

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Definition: Tangent Space \@{tangent-space}

If M is locally given by a smooth parametrization

φ:U⊂Rk→M⊂Rn,

and p=φ(u0), then

TpM=span{∂φ∂u1(u0),∂φ∂u2(u0),…,∂φ∂uk(u0)}.

So it’s the collection of all possible velocity vectors of curves on the manifold passing through p, and is a k-dimensional linear subspace of Rn.

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Definition: Tangent Vector \@{tangent-vector}

For a space curve given parametrically by r(t), the tangent vector (or specifically, the unit tangent vector) at the point r(t) is the unit vector defined by:

T(t)=r′(t)‖r′(t)‖

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Definition: Tangential Intersection \@{tangential-intersection}

Two functions f and g are said to have a tangential intersection at a point p if both their values and the values of their first @derivatives are equal at p. That is, if

f(p)=g(p)ANDf′(p)=g′(p).

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Definition: Target Class \@{target-class}

In binary classification, the task is to determine whether or not an object belongs to a class, which we call the target class.

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Definition: Taylor series \@{taylor-series}

The expansion

f(z)=∑n=0∞f(n)(z0)n!(z−z0)n

is called the Taylor series of f about z0.

Definition: Term \@{term}

If f is a sequence denoted as {xn}, the values of f, that is, the elements xn, are called the terms of the sequence.

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Definition: theorem \@{theorem}

A formula ψ∈W is a theorem (or provable formula) of F if there exists such a derivation ending with ψ. We then write

⊢Fψ.

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Definition: Total Derivative \@{total-derivative}

The derivative defined above in differentiable is called the total derivative of f at x, or the differential of f at x.

Definition: Transcritical \@{transcritical}

A transcritical bifurcation occurs when a given x∗ is always a fixed point, but its stability changes when crossing the bifurcation point r∗. At all values of r other than r∗, there are two fixed points (and at r∗ one degenerate fixed point), but their stability is exchanged at the crossing.

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Definition: translation \@{translation}

If t∈R and A⊂R, then the translation t+A is defined by

t+A={t+a:a∈A}.

Definition: transposition \@{transposition}

A cycle of length 2 is a transposition.

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from Groups
Definition: Uniform Distribution \@{uniform-distribution}

The uniform distribution has a "flat" density function and thus a uniform probability in a closed interval [A,B].

The density function of the continuous uniform random variable X on the interval [A,B] is

f(x;A,B)={1B−Afor A≤x≤B0otherwise

The mean and variance of the uniform distributions are

μ=A+B2,σ2=(B−A)212.

The cumulative distribution function for a uniform distribution is

F(x)=x−AB−A,A≤x≤B

and the probability that a value falls between a and b is

∫ab1B−Adx=b−aB−A,A≤a,b≤B

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Definition: Unit \@{unit}

If a has a multiplicative inverse in R, a is said to be a unit in R.

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Definition: unity \@{unity}

The element 1 is also called unity.

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Definition: Unstable \@{unstable}

A fixed point where nearby points flow away from it is said to be unstable.

Definition: Unstable limit cycle \@{unstable-limit-cycle}

If a limit cycle is not stable, we say it is an unstable limit cycle, or in exceptional cases, half-stable.

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Definition: Upper bound \@{upper-bound}

The number m is said to be an upper bound of a nonempty set A if x≤m for all x∈A.

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Definition: Value \@{value}

If f is a function from the set A to the set B, the elements f(x)∈B are called the values of f.

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Definition: Vector \@{vector}

A vector is an element in a vector space.

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Definition: Vector Addition \@{vector-addition}

We perform vector addition by adding two vectors x=(x1,x2,⋯,xn) and y=(y1,y2,⋯,yn) according to the following rule:

x+y=(x1+y1,x2+y2,⋯,xn+yn)

that is, by making a new vector where the coordinates are the sums of the respective coordinates in the vectors being summed.

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Definition: Vector Equality \@{vector-equality}

Two vectors are equal if they have the same coordinates (or equivalently, the same length and direction).

Definition: Vector Function \@{vector-function}

Let P be any point in a domain of definition. Then we define a vector function v whose values are vectors, that is,

v=v(P)=[v1(P),v2(P),v3(P)]

that depends on points P in space. A vector function depends only on the point P, not on the coordinate system chosen to represent its components.

Definition: Vector Multiplication by a Scalar \@{vector-multiplication-by-a-scalar}

We can multiply vectors by a scalar. Given the scalar c:

cx=(cx1,cx2,⋯,cxn)

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Definition: Vector Space \@{vector-space}

A vector space over a field F is a set V together with two operations:

satisfying the following axioms:

  1. (V,+) is an abelian group
  1. Scalar multiplication is associative: a(bv)=(ab)v
  1. Distributive laws hold
  1. Identity: 1v=v for all v∈V
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Definition: Vector Subtraction \@{vector-subtraction}

Similarly, vector subtraction can be performed as:

x−y=(x1−y1,x2−y2,⋯,xn−yn)

Definition: Volume Integral (also: triple integral) \@{volume-integral}

If T is a closed, bounded, three-dimensional region of space, and f(x,y,z) is defined and continuous in a domain containing T, then the volume integral of f(x,y,z) over the region T is denoted by

∭Tf(x,y,z)dxdydz=∭Tf(x,y,z)dV.

Such integrals can be evaluated via three successive integrations.

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Definition: Weakly Nonlinear Oscillator \@{weakly-nonlinear-oscillator}

Equations of the form

x˙+x+ϵh(x,x˙)=0(a)

where 0≤ϵ≪1 and h(x,x˙) is an arbitrary smooth function represent small @perturbations of the linear @oscillator x˙+x=0 and are therefore called weakly nonlinear oscillators.

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Definition: Zero Vector \@{zero-vector}

The zero vector (0,0,⋯,0) is denoted as 0 and has no direction.

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Definition: Zero-Eigenvalue Bifurcation \@{zero-eigenvalue-bifurcation}

We say a zero-eigenvalue bifurcation occurs when one of the eigenvalues equals zero, or equivalently, when Δ=0. They always occur when two or more fixed points collide as a parameter is varied.