Hypersphere
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In mathematics, a hypersphere is a sphere which has dimension 3 or higher. The term [n]-sphere is used for a sphere of dimension [n], for any positive integer [n]. An origin-centered sphere of radius [R] consists of all points in n-dimensional Euclidean space for which the sum of the squares of every coordinate is constant. The constant is [R^2], and its square root is the Euclidean distance of every point on the sphere from the origin. The set of all points on this sphere has dimension [n-1], so it is called the [(n-1)]-sphere and is denoted [\mathbb S^]. It may be written as [(x_1,x_2,...,x_n)] where
- [R^2=\sum_^n x_i^2.\,]
Hyperspherical volume
The hyperdimensional volume of the space which a [(n-1)]-sphere encloses (the [n]-ball) is:
- [V_n=R^n\over\Gamma(n/2+1)}]
The "surface area" of this sphere is
- [S_n=\frac=\frac=R^\over\Gamma(n/2)}]
Hyperspherical volume - some examples
For small values of [n], the volumes, [V_n] , of the unit [n]-ball ([R=1]) are:
[V_1\,] = [2\,] [V_2\,] = [\pi\,] = [3.14159\ldots\,] [V_3\,] = [\frac\,] = [4.18879\ldots\,] [V_4\,] = [\frac\,] = [4.93480\ldots\,] [V_5\,] = [\frac\,] = [5.26379\ldots\,] [V_6\,] = [\frac\,] = [5.16771\ldots\,] [V_7\,] = [\frac\,] = [4.72478\ldots\,] [V_8\,] = [\frac\,] = [4.05871\ldots\,] [\lim_ V_n\,] = [0\,] If the dimension, [\ n] , is not limited to integral values, the hypersphere volume is a continuous function of [\ n] with a global maximum for the unit sphere in "dimension" n = 5.2569464... where the "volume" is 5.277768...
The hypercube circumscribed around the unit n-sphere has an edge length of 2 and hence a volume of 2n; the ratio of the volume of the hypersphere to its circumscribed hypercube decreases monotonically as the dimension increases.
Hyperspherical coordinates
We may define a coordinate system in an n-dimensional Euclidean space which is analogous to the spherical coordinate system defined for 3-dimensional Euclidean space, in which the coordinates consist of a radial coordinate [\ r], and [\ n-1] angular coordinates [\ \phi _1 , \phi _2 , ... , \phi _]. If [\ x_i] are the Cartesian coordinates, then we may define
- [x_1=r\cos(\phi_1)\,]
- [x_2=r\sin(\phi_1)\cos(\phi_2)\,]
- [x_3=r\sin(\phi_1)\sin(\phi_2)\cos(\phi_3)\,]
- [\cdots\,]
- [x_=r\sin(\phi_1)\cdots\sin(\phi_)\cos(\phi_)\,]
- [x_n~~\,=r\sin(\phi_1)\cdots\sin(\phi_)\sin(\phi_)\,]
- [d^nr = \left|\det\frac\right|dr\,d\phi_1 \, d\phi_2\ldots d\phi_]
- [=r^\sin^(\phi_1)\sin^(\phi_2)\cdots \sin(\phi_)\,dr\,d\phi_1 \, d\phi_2\cdots d\phi_]
- [V_n=\int_^R \int_^\pi\cdots \int_=0}^\pi\int_=0}^d^nr. \,]
Stereographic projection
Just as a two dimensional sphere embedded in three dimensions can be mapped onto a two-dimensional plane by a stereographic projection, an n-dimensional hypersphere can be mapped onto an n-dimensional hyperplane by the n-dimensional version of the stereographic projection. For example, the point [\ [x,y,z]] on a two-dimensional sphere of radius 1 maps to the point [\ [x,y,z] \mapsto \left[frac,fracright]] on the [\ xy] plane. In other words:
- [\ [x,y,z] \mapsto \left[frac,fracright]]
- [[x_1,x_2,ldots,x_n] \mapsto \left[frac,frac,ldots,frac}right]]
See also
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