Mathematical Problems : $b Lecture delivered before the International Congress of Mathematicians at Paris in 1900Hilbert, David
Science
Mathematical Problems : $b Lecture delivered before the International Congress of Mathematicians at Paris in 1900
Hilbert, David
Mathematics
Exactly the corresponding facts are found in space of three dimensions.
The fact of the finiteness of the groups of motions in elliptic
space is an immediate consequence of a fundamental theorem of C.
Jordan,[41] whereby the number of[Pg 31] essentially different kinds of
finite groups of linear substitutions in variables does not
surpass a certain finite limit dependent upon . The groups
of motions with fundamental regions in hyperbolic space have been
investigated by Fricke and Klein in the lectures on the theory of
automorphic functions,[42] and finally Fedorov,[43]
Schoenflies[44]
and lately Rohn[45] have given the proof that there are, in euclidean
space, only a finite number of essentially different kinds of groups
of motions with a fundamental region. Now, while the results and
methods of proof applicable to elliptic and hyperbolic space hold
directly for -dimensional space also, the generalization of the
theorem for euclidean space seems to offer decided difficulties. The
investigation of the following question is therefore desirable: Is
there in -dimensional euclidean space also only a finite number
of essentially different kinds of groups of motions with a fundamental
region?
A fundamental region of each group of motions, together with the
congruent regions arising from the group, evidently fills up space
completely. The question arises: Whether polyhedra also exist which
do not appear as fundamental regions of groups of motions, by means
of which nevertheless by a suitable juxtaposition of congruent copies
a complete filling up of all space is possible. I point out the
following question, related to the preceding one, and important to
number theory and perhaps sometimes useful to physics and chemistry:
How can one arrange most densely in space an infinite number of equal
solids of given form, e. g., spheres with given radii or regular
tetrahedra with given edges (or in prescribed position), that is,
how can one so fit them together that the ratio of the filled to the
unfilled space may be as great as possible?
If we look over the development of the theory of functions in the last
century, we notice above all the fundamental importance of that class
of functions which we now designate as analytic functions—a class
of functions which will probably stand permanently in the center of
mathematical interest.
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