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Disk (mathematics)
Disk (mathematics)
from Wikipedia
Disk with
  diameter D
  radius R
  center or origin O

In geometry, a disk (also spelled disc)[1] is the region in a plane bounded by a circle. A disk is said to be closed if it contains the circle that constitutes its boundary, and open if it does not.[2]

For a radius , an open disk is usually denoted as , and a closed disk is . However in the field of topology the closed disk is usually denoted as , while the open disk is .

Formulas

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In Cartesian coordinates, the open disk with center and radius R is given by the formula[1] while the closed disk with the same center and radius is given by

The area of a closed or open disk of radius R is πR2 (see area of a disk).[3]

Properties

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The disk has circular symmetry.[4]

The open disk and the closed disk are not topologically equivalent (that is, they are not homeomorphic), as they have different topological properties from each other. For instance, every closed disk is compact whereas every open disk is not compact.[5] However from the viewpoint of algebraic topology they share many properties: both of them are contractible[6] and so are homotopy equivalent to a single point. This implies that their fundamental groups are trivial, and all homology groups are trivial except the 0th one, which is isomorphic to Z. The Euler characteristic of a point (and therefore also that of a closed or open disk) is 1.[7]

Every continuous map from the closed disk to itself has at least one fixed point (we don't require the map to be bijective or even surjective); this is the case n=2 of the Brouwer fixed-point theorem.[8] The statement is false for the open disk:[9]

Consider for example the function which maps every point of the open unit disk to another point on the open unit disk to the right of the given one. But for the closed unit disk it fixes every point on the half circle

As a statistical distribution

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The average distance to a location from points on a disc

A uniform distribution on a unit circular disk is occasionally encountered in statistics. It most commonly occurs in operations research in the mathematics of urban planning, where it may be used to model a population within a city. Other uses may take advantage of the fact that it is a distribution for which it is easy to compute the probability that a given set of linear inequalities will be satisfied. (Gaussian distributions in the plane require numerical quadrature.)

"An ingenious argument via elementary functions" shows the mean Euclidean distance between two points in the disk to be 128/45π ≈ 0.90541,[10] while direct integration in polar coordinates shows the mean squared distance to be 1.

If we are given an arbitrary location at a distance q from the center of the disk, it is also of interest to determine the average distance b(q) from points in the distribution to this location and the average square of such distances. The latter value can be computed directly as q2+1/2.

Average distance to an arbitrary internal point

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The average distance from a disk to an internal point

To find b(q) we need to look separately at the cases in which the location is internal or external, i.e. in which q ≶ 1, and we find that in both cases the result can only be expressed in terms of complete elliptic integrals.

If we consider an internal location, our aim (looking at the diagram) is to compute the expected value of r under a distribution whose density is 1/π for 0 ≤ rs(θ), integrating in polar coordinates centered on the fixed location for which the area of a cell is r dr ; hence

Here s(θ) can be found in terms of q and θ using the Law of cosines. The steps needed to evaluate the integral, together with several references, will be found in the paper by Lew et al.;[10] the result is that where K and E are complete elliptic integrals of the first and second kinds.[11] b(0) = 2/3; b(1) = 32/ ≈ 1.13177.

Average distance to an arbitrary external point

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The average distance from a disk to an external point

Turning to an external location, we can set up the integral in a similar way, this time obtaining

where the law of cosines tells us that s+(θ) and s(θ) are the roots for s of the equation Hence We may substitute u = q sinθ to get using standard integrals.[12]

Hence again b(1) = 32/, while also[13]

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
In mathematics, a disk (or disc) is a fundamental geometric object in Euclidean space, defined as the set of all points within a specified distance from a fixed center point. Specifically, an n-dimensional disk of radius r consists of all points x in Rn\mathbb{R}^n such that the Euclidean distance xcr\|x - c\| \leq r for a center cc (closed disk) or <r< r (open disk). In two dimensions, this corresponds to the region enclosed by a circle, including or excluding the boundary circle itself. The disk plays a central role in geometry and topology, where the standard n-disk, often denoted DnD^n, is the closed unit disk with center at the origin and radius 1, i.e., {xRn:x1}\{x \in \mathbb{R}^n : \|x\| \leq 1\}. For n3n \geq 3, the n-disk is commonly referred to as an n-ball, with its boundary being an (n1)(n-1)-sphere Sn1S^{n-1}. Topologically, the disk is contractible and simply connected, meaning it can be continuously shrunk to a point without leaving the space, and every loop within it can be contracted to a point. This makes it a basic building block in manifold theory and homotopy, where quotients like Dn/Sn1D^n / S^{n-1} yield the n-sphere SnS^n. In complex analysis, the disk—particularly the open unit disk {zC:z<1}\{z \in \mathbb{C} : |z| < 1\}—is essential for studying and . It serves as a model domain due to the , which states that any simply connected domain in the complex plane (other than the whole plane) can be conformally mapped onto the unit disk. Properties like the and are formulated and proven on disks, highlighting their role in bounding . Punctured disks, excluding the center, arise in the study of isolated singularities. Disks also appear in higher-dimensional geometry and physics, such as in the Poincaré disk model for hyperbolic geometry, where geodesics and curvature are defined within the unit disk using a conformal metric. Their volume scales with dimension via formulas like Vn(r)=πn/2Γ(n/2+1)rnV_n(r) = \frac{\pi^{n/2}}{\Gamma(n/2 + 1)} r^n, illustrating paradoxical behaviors in high dimensions.

Definitions and Basic Concepts

Two-dimensional disk

In Euclidean plane geometry, the two-dimensional disk is defined as the set of all points whose distance from a fixed center point cc is at most a given radius r>0r > 0. This region encompasses both the interior points and the boundary, forming a solid, circular shape in the plane. The closed disk, denoted D(c,r)={zR2:zcr}\overline{D}(c, r) = \{ z \in \mathbb{R}^2 : \|z - c\| \leq r \}, includes all points satisfying this inequality, making it a bounded and . In contrast, the open disk D(c,r)={zR2:zc<r}D(c, r) = \{ z \in \mathbb{R}^2 : \|z - c\| < r \} excludes the boundary, consisting solely of the interior points. The boundary of the disk is precisely the circle of radius rr centered at cc, which is the set of points exactly at distance rr from the center. This distinction clarifies that the disk refers to the filled area, whereas the circle denotes only the perimeter curve. Similarly, the disk differs from an annulus, a ring-shaped region bounded by two concentric circles of different radii sharing the same center; the disk, by contrast, extends uniformly from the center to the full radius without an inner boundary. The term "disk" emerged in modern geometry texts to specify this filled region and avoid conflation with "circle," which traditionally could imply the bounded area in older usages but now strictly means the boundary. Visually, the disk resembles a uniformly shaded circle, representing a convex set where any line segment connecting two points within it lies entirely inside; the closed form is both convex and compact. This two-dimensional case serves as the foundational analog for higher-dimensional balls in Euclidean space.

Higher-dimensional disks

In higher dimensions, the concept of a disk generalizes to the n-ball or n-disk in n-dimensional Euclidean space Rn\mathbb{R}^n. The closed n-ball of radius r>0r > 0 centered at a point cRnc \in \mathbb{R}^n is defined as the set {xRn:xcr}\{ x \in \mathbb{R}^n : \|x - c\| \leq r \}, where \| \cdot \| denotes the Euclidean norm. The corresponding open n-ball replaces the inequality with strict less-than: {xRn:xc<r}\{ x \in \mathbb{R}^n : \|x - c\| < r \}. This builds on the two-dimensional disk as the foundational case, extending the filled circular region to arbitrary dimensions without altering the core idea of points within a fixed distance from the center. Terminology varies slightly across mathematical contexts, but the n-ball is the standard term for this object in n dimensions, sometimes interchangeably called the n-disk. Specifically, the 2-ball is commonly referred to as a disk, while the 3-ball is known as a ball or solid ball. In general, for n3n \geq 3, the term n-ball prevails to emphasize the higher-dimensional filling. Illustrative examples clarify the structure across low dimensions. The 1-ball of radius rr centered at cc is simply a closed line segment of length 2r2r from crc - r to c+rc + r along the real line. In three dimensions, the 3-ball is the familiar solid ball, encompassing all points inside and on a spherical surface of radius rr. These cases demonstrate how the n-ball fills the interior region bounded by a hypersurface in Rn\mathbb{R}^n. The boundary of the closed n-ball is the (n-1)-sphere, defined as {xRn:xc=r}\{ x \in \mathbb{R}^n : \|x - c\| = r \}, which forms the "surface" enclosing the n-ball. This boundary is itself an (n-1)-dimensional manifold, reducing to a pair of points for the 1-ball and a circle for the 2-ball.

Geometric Formulas

Area and perimeter

The area of a two-dimensional disk of radius rr is given by A=πr2A = \pi r^2. This formula can be derived by integrating the circumferences of infinitesimal concentric rings composing the disk. The circumference at radius ss is 2πs2\pi s, and the infinitesimal area of a ring of width dsds is 2πsds2\pi s \, ds. Thus, A=0r2πsds=πr2.A = \int_0^r 2\pi s \, ds = \pi r^2. An alternative derivation uses Green's theorem, which states that the area enclosed by a positively oriented, piecewise smooth, simple closed curve CC bounding region DD is A=12C(xdyydx).A = \frac{1}{2} \oint_C (x \, dy - y \, dx). For the disk, parametrize the boundary circle as x=rcosθx = r \cos \theta, y=rsinθy = r \sin \theta for θ[0,2π]\theta \in [0, 2\pi]. Substituting yields dx=rsinθdθdx = -r \sin \theta \, d\theta, dy=rcosθdθdy = r \cos \theta \, d\theta, so A=1202π(rcosθrcosθrsinθ(rsinθ))dθ=1202πr2(cos2θ+sin2θ)dθ=πr2.A = \frac{1}{2} \int_0^{2\pi} \left( r \cos \theta \cdot r \cos \theta - r \sin \theta \cdot (-r \sin \theta) \right) d\theta = \frac{1}{2} \int_0^{2\pi} r^2 (\cos^2 \theta + \sin^2 \theta) d\theta = \pi r^2. The perimeter of the disk, which is the circumference of its bounding circle, is C=2πrC = 2\pi r. This follows from the arc length formula for a parametric curve r(θ)=(rcosθ,rsinθ)\mathbf{r}(\theta) = (r \cos \theta, r \sin \theta), θ[0,2π]\theta \in [0, 2\pi]: C=02π(dxdθ)2+(dydθ)2dθ=02π(rsinθ)2+(rcosθ)2dθ=02πrdθ=2πr.C = \int_0^{2\pi} \sqrt{ \left( \frac{dx}{d\theta} \right)^2 + \left( \frac{dy}{d\theta} \right)^2 } \, d\theta = \int_0^{2\pi} \sqrt{ ( -r \sin \theta )^2 + ( r \cos \theta )^2 } \, d\theta = \int_0^{2\pi} r \, d\theta = 2\pi r.
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