Hill tetrahedron explained

In geometry, the Hill tetrahedra are a family of space-filling tetrahedra. They were discovered in 1896 by M. J. M. Hill, a professor of mathematics at the University College London, who showed that they are scissor-congruent to a cube.

Construction

For every

\alpha\in(0,2\pi/3)

, let

v1,v2,v3\inR3

be three unit vectors with angle

\alpha

between every two of them.Define the Hill tetrahedron

Q(\alpha)

as follows:

Q(\alpha)=\{c1v1+c2v2+c3v3\mid0\lec1\lec2\lec3\le1\}.

A special case

Q=Q(\pi/2)

is the tetrahedron having all sides right triangles, two with sides

(1,1,\sqrt{2})

and two with sides

(1,\sqrt{2},\sqrt{3})

. Ludwig Schläfli studied

Q

as a special case of the orthoscheme, and H. S. M. Coxeter called it the characteristic tetrahedron of the cubic spacefilling.

Properties

Q

.[1]

Q(\alpha)

can be dissected into three polytopes which can be reassembled into a prism.

Generalizations

In 1951 Hugo Hadwiger found the following n-dimensional generalization of Hill tetrahedra:

Q(w)=\{c1v1+ … +cnvn\mid0\lec1\le\lecn\le1\},

where vectors

v1,\ldots,vn

satisfy

(vi,vj)=w

for all

1\lei<j\len

, and where

-1/(n-1)<w<1

. Hadwiger showed that all such simplices are scissor congruent to a hypercube.

References

External links

Notes and References

  1. Web site: Space-Filling Tetrahedra - Wolfram Demonstrations Project.