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Unit sphere

 
Sci-Tech Dictionary: unit sphere
(′yü·nət ′sfir)

(mathematics) The set of points in three-space (more generally n-space) which are precisely one unit distance from the origin.


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In mathematics, a unit sphere is the set of points of distance 1 from a fixed central point, where a generalized concept of distance may be used; a closed unit ball is the set of points of distance less than or equal to 1 from a fixed central point. Usually a specific point has been distinguished as the origin of the space under study and it is understood that a unit sphere or unit ball is centered at that point. Therefore one speaks of "the" unit ball or "the" unit sphere.

A unit sphere is simply a sphere of radius one. The importance of the unit sphere is that any sphere can be transformed to a unit sphere by a combination of translation and scaling. In this way the properties of spheres in general can be reduced to the study of the unit sphere.

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Unit spheres and balls in Euclidean space

In Euclidean space of n dimensions, the unit sphere is the set of all points (x_1, \ldots, x_n) which satisfy the equation

 x_1^2 + x_2^2 + \cdots + x_n ^2 = 1

and the closed unit ball is the set of all points satisfying the inequality

 x_1^2 + x_2^2 + \cdots + x_n ^2 \le 1.

General area and volume formulas

The classical equation of a unit sphere is that of the ellipsoid with a radius of 1 and no alterations to the x-, y-, or z- axes:

f(x,y,z) = x2 + y2 + z2 = 1

The volume of the unit ball in n-dimensional Euclidean space, and the surface area of the unit sphere, appear in many important formulas of analysis. The volume of the unit ball in n dimensions, which we denote Vn, can be expressed by making use of the Gamma function. It is

V_n = \frac{\pi ^ {n/2}}{\Gamma(1+n/2)} = \left\lbrace \begin{array}{cl}
{\pi^{n/2}}/{(n/2)!} & \mathrm{if~}n \ge 0\mathrm{~is~even,} \\
~\\
{\pi^{\lfloor n/2 \rfloor}2^{\lceil n/2 \rceil}}/{n!!} & \mathrm{if~}n \ge 0\mathrm{~is~odd,}
\end{array}\right.

where n!! is the double factorial.

The surface area of the unit sphere in n dimensions, which we denote An, can be expressed as

A_n = n V_n = \frac{n \pi ^ {n/2}}{\Gamma(1+n/2)} = \frac{2 \pi ^ {n/2}}{\Gamma(n/2)}\,,

where the last equality holds only for n > 0.

The surface areas and the volumes for some values of n are as follows:

n An (surface area) Vn (volume)
0 0(1 / 0!)π0 0.000 (1 / 0!)π0 1.000
1 1(21 / 1!!)π0 2.000 (21 / 1!!)π0 2.000
2 2(1 / 1!)π1 = 2π 6.283 (1 / 1!)π1 = π 3.142
3 3(22 / 3!!)π1 = 4π 12.57 (22 / 3!!)π1 = (4 / 3)π 4.189
4 4(1 / 2!)π2 = 2π2 19.74 (1 / 2!)π2 = (1 / 2)π2 4.935
5 5(23 / 5!!)π2 = (8 / 3)π2 26.32 (23 / 5!!)π2 = (8 / 15)π2 = 5.264
6 6(1 / 3!)π3 = π3 31.01 (1 / 3!)π3 = (1 / 6)π3 5.168
7 7(24 / 7!!)π3 = (16 / 15)π3 33.07 (24 / 7!!)π3 = (16 / 105)π3 4.725
8 8(1 / 4!)π4 = (1 / 3)π4 32.47 (1 / 4!)π4 = (1 / 24)π4 4.059
9 9(25 / 9!!)π4 = (32 / 105)π4 29.69 (25 / 9!!)π4 = (32 / 945)π4 3.299
10 10(1 / 5!)π5 = (1 / 12)π5 25.50 (1 / 5!)π5 = (1 / 120)π5 2.550

where the decimal expanded values for n ≥ 2 are approximate.

Recursion

The An values satisfy the recursion:

A0 = 0
A1 = 2
A2 = 2π
A_n = \frac{2 \pi}{n-2} A_{n-2} for n > 2.

The Vn values satisfy the recursion:

V0 = 1
V1 = 2
V_n = \frac{2 \pi}{n} V_{n-2} for n > 1.

Fractional dimensions

The formulae for An and Vn can be computed for any real number n ≥ 0, and there are circumstances under which it is appropriate to seek the sphere area or ball volume when n is not a non-negative integer.

This shows the surface area of a sphere in x dimensions as a continuous function of x.
This shows the volume of a ball in x dimensions as a continuous function of x.

Other radii

The surface area of the sphere in n dimensions with radius r is An rn−1 and the volume of the ball in n dimensions with radius r is Vn rn. For instance, the surface area is A = 4πr 2 for the sphere of radius r in three dimensions and the volume is V = 4πr 3 / 3 for the three-dimensional ball of radius r.

Unit balls in normed vector spaces

More precisely, the open unit ball in a normed vector space V, with the norm \|\cdot\|, is

 \{ x\in V: \|x\|<1 \}.

It is the interior of the closed unit ball of (V,||·||),

 \{ x\in V: \|x\|\le 1\}.

The latter is the disjoint union of the former and their common border, the unit sphere of (V,||·||),

 \{ x\in V: \|x\| = 1 \}.

The 'shape' of the unit ball is entirely dependent on the chosen norm; it may well have 'corners', and for example may look like [−1,1]n, in the case of the norm l in Rn. The round ball is understood as the usual Hilbert space norm, based in the finite dimensional case on the Euclidean distance; its boundary is what is usually meant by the unit sphere. Here are some images of the unit ball for the two-dimensional \ell^p space for various values of p (the unit ball being concave for p < 1 and convex for p >= 1):

Minkowski2.png

Note that for the circumferences Cp of the two-dimensional unit balls we have:

C_{p} = C_{1/p} \,
C_{0} = 4 * 2 = C_{\infty} is algebraic (maximal circumference)
C_{1} = 4 * \sqrt{2} is algebraic (minimal circumference)
C_{2} = 4 * (\pi /2) = C_{1/2} \, is transcendental.

Are all the others circumferences transcendental?

Generalizations

Metric spaces

All three of the above definitions can be straightforwardly generalized to a metric space, with respect to a chosen origin. However, topological considerations (interior, closure, border) need not apply in the same way (e.g., in ultrametric spaces, all of the three are simultaneously open and closed sets), and the unit sphere may even be empty in some metric spaces.

Quadratic forms

If V is a linear space with a real quadratic form F:V → R, then { x ∈ V : F(x) = 1 } is sometimes called the unit sphere of V. Two-dimensional examples occur with split-complex numbers and dual numbers. When F takes negative values, then {x ∈ V: F(x) = − 1} is called the counter-sphere.

See also

References

External links


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