move freely over a surface:
in this case the axiom of Monodromy
is unnecessary,
and the first three axioms suffice to define our group as that of Euclidean
and non-Euclidean motions.
Or free mobility,
within the specified region,
holds only of every point of general position,
while the points of a certain line,
when one point is fixed,
are only able to move on that line,
not on a surface:
when this is the case,
other groups are possible,
and can only be excluded by Helmholtz's
fourth axiom.
Having now stated the purely mathematical results of Lie's investigations,
we may return to philosophical considerations,
by which Helmholtz's
work was mainly motived.
It becomes obvious,
not only that exceptions within a certain region,
but also that limitation to a certain region,
of the axiom of Free Mobility,
are philosophically quite impossible and inconceivable.
How can a certain line,
or a certain surface,
form an impassable barrier in space,
or have any mobility different in kind from that of all other lines or surfaces?
The notion cannot,
in philosophy,
be permitted for a moment,
since it destroys that most fundamental of all the axioms,
the homogeneity of space.
We not only may,
therefore,
but must take Helmholtz's
axiom of Free Mobility in its very strictest sense;
the axiom of Monodromy
thus becomes mathematically,
as well as philosophically,
superfluous.
This is,
from a philosophical standpoint,
the most important of Lie's results.
46.
I have now come to the end of my history of Metageometry.
It has not been my aim to give an exhaustive account of even the important works on the subject—
in the third period,
especially,
the names of Poincaré, Pasch, Cremona, Veronese,
and others who might be mentioned,
would have cried shame upon me,
had I had any such object.
But I have tried to set forth,
as clearly as I could,
the principles at work in the various periods,
the motives and results of successive theories.
We have seen how the philosophical motive,
at first predominant,
has been gradually extruded by the purely mathematical and technical spirit of most recent Geometers.
At first,
to discredit the Transcendental Aesthetic seemed,
to Metageometers,
as important as to advance their science;
but from the works of Cayley, Klein
or Lie,
no reader could gather that Kant
had ever lived.
We have also seen,
however,
that as the interest in philosophy waned,
the interest for philosophy increased:
as the mathematical results shook themselves free from philosophical controversies,
they assumed gradually a stable form,
from which further development,
we may reasonably hope,
will take the form of growth,
rather than transformation.
The same gradual development out of philosophy might,
I believe,
be traced in the infancy of most branches of mathematics;
when philosophical motives cease to operate,
this is,
in general,
a sign that the stage of uncertainty as to premisses is past,
so that the future belongs entirely to mathematical technique.
When this stable stage has been attained,
it is time for Philosophy to borrow of Science,
accepting its final premisses as those imposed by a real necessity of fact or logic.
47.
Now in discussing the systems of Metageometry,
we have found two kinds,
radically distinct and subject to different axioms.
The historically prior kind,
which deals with metrical ideas,
discusses,
to begin with,
the conditions of Free Mobility,
which is essential to all measurement of space.
It finds the analytical expression of these conditions in the existence of a space-constant,
or constant measure of curvature,
which is equivalent to the homogeneity of space.
This is its first axiom.
Its second axiom states that space has a finite integral number of dimensions,
i.
e.
in metrical terms,
that the position of a point,
relative to any other figure in space,
is uniquely determined by a finite number of spatial magnitudes,
called coordinates.
The third axiom of metrical Geometry may be called,
to distinguish it from the corresponding projective axiom,
the axiom of distance.
There exists one relation,
it says,
between any two points,
which can be preserved unaltered in a combined motion of both points,
and which,
in any motion of a system as one rigid body,
is always unaltered.
This relation we call distance.
The above statement of the three essential axioms of metrical Geometry is taken from Helmholtz
as amended by Lie.
Lie's own statement of the axioms,
as quoted above,
has been too much influenced by projective methods to give a historically correct rendering of the spirit of the second period; Helmholtz's
statement,
on the other hand,
requires,
as Lie has shewn,
very considerable modifications.
The above compromise may,
therefore,
I hope be taken as accepting Lie's corrections while retaining Helmholtz's
spirit.
48.
But metrical Geometry,
though it is historically prior,
is logically subsequent to projective Geometry.
For projective Geometry deals directly with that qualitative likeness,
which the judgment of quantitative comparison requires as its basis.
Now the above three axioms of metrical Geometry,
as we shall see in Chapter III.
Section B,
do not presuppose measurement,
but are,
on the contrary,
the conditions presupposed by measurement.
Without these axioms,
which are common to all three spaces,
measurement would be impossible;
with them,
so I shall contend,
measurement is able,
though only empirically,
to decide approximately which of the three spaces is valid of our actual world.
But if these three axioms themselves express,
not results,
but conditions,
of measurement,
must they not be equivalent to the statement of that qualitative likeness on which quantitative comparison depends?
And if so,
must we not expect to find the same axioms,
though perhaps under a different form,
in projective Geometry?
49.
This expectation will not be disappointed.
The above three axioms,
as we shall see hereafter,
are one and all philosophically equivalent to the homogeneity of space,
and this in turn is equivalent to the axioms of projective Geometry.
The axioms of projective Geometry,
in fact,
may be roughly stated thus:
I.
Space is continuous and infinitely divisible;
the zero of extension,
resulting from infinite division,
is called a Point.
All points are qualitatively similar,
and distinguished by the mere fact that they lie outside one another.
II.
Any two points determine a unique figure,
the straight line;
two straight lines,
like two points,
are qualitatively similar,
and distinguished by the mere fact that they are mutually external.
III.
Three points not in one straight line determine a unique figure,
the plane,
and four points not in one plane determine a figure of three dimensions.
This process may,
so far as can be seen à priori,
be continued,
without in any way interfering with the possibility of projective Geometry,
to five or to n
points.
But projective Geometry requires,
as an axiom,
that the process should stop with some positive integral number of points,
after which,
any fresh point is contained in the figure determined by those already given.
If the process stops with (n + 1)
points,
our space is said to have n
dimensions.
These three axioms,
it will be seen,
are the equivalents of the three axioms of metrical Geometry[65],
expressed without reference to quantity.
We shall find them to be deducible,
as before,
from the homogeneity of space,
or,
more generally still,
from the possibility of experiencing externality.
They will therefore appear as à priori,
as essential to the existence of any Geometry and to experience of an external world as such.
50.
That some logical necessity is involved in these axioms might,
I think,
be inferred as probable,
from their historical development alone.
For the systems of Metageometry
have not,
in general,
been set up as more likely to fit facts than the system of Euclid;
with the exception of Zöllner,
for example,
I know of no one who has regarded the fourth dimension as required to explain phenomena.
As regards the space-constant
again,
though a small space-constant
is regarded as empirically possible,
it is not usually regarded as probable;
and the finite space-constants,
with which Metageometry
is equally conversant,
are not usually thought even possible,
as explanations of empirical fact[66].
Thus the motive has been throughout not one of fact,
but one of logic.
Does not this give a strong presumption,
that those axioms which are retained,
are retained because they are logically indispensable?
If this be so,
the axioms common to Euclid
and Metageometry
will be à priori,
while those peculiar to Euclid
will be empirical.
After a criticism of some differing theories of Geometry,
I shall proceed,
in Chapters III.
and IV.,
to the proof and consequences of this thesis,
which will form the remainder of the present work.
FOOTNOTES: [5]
V.
Mémoires de
l'Académie royale des
Sciences de
l'lnstitut de France, T. XII. 1833,
for a full statement of his results,
with references to former writings. [6]
This bolder method,
it appears,
had been suggested,
nearly a century earlier,
by an Italian, Saccheri.
His work,
which seems to have remained completely unknown until Beltrami
rediscovered it in 1889,
is called "Euclides ab
omni naevo vindicatus,
etc."
Mediolani, 1733. (
See Veronese, Grundzüge
der Geometrie, German
translation, Leipzig, 1894,
p. 636.)
His results included spherical as well as hyperbolic space;
but they alarmed him to such an extent that he devoted the last half of his book to disproving them. [7] Klein's
first account of elliptic Geometry,
as a result of Cayley's
projective theory of distance,
appeared in two articles entitled "Ueber
die sogenannte Nicht-Euklidische Geometrie,
I, II,"
Math.
Annalen 4, 6 (1871–2).
It was afterwards independently discovered by Newcomb,
in an article entitled "
Elementary Theorems relating to the geometry of a space of three dimensions,
and of uniform positive curvature in the fourth dimension," Crelle's
Journal für die reine und
angewandte Mathematik,
Vol. 83 (1877).
For an account of the mathematical controversies concerning elliptic Geometry,
see Klein's "Vorlesungen
über Nicht-Euklidische Geometrie," Göttingen 1893,
I.
p. 284 ff.
A bibliography of the relevant literature up to the year 1878
was given by Halsted
in the American Journal of Mathematics, Vols. 1, 2. [8] Veronese (op. cit.
p. 638)
denies the priority of Gauss
in the invention of a non-Euclidean system,
though he admits him to have been the first to regard the axiom of parallels as indemonstrable.
His grounds for the former assertion seem scarcely adequate:
on the evidence against it,
see Klein, Nicht-Euklid,
I.
pp. 171–174. [9]
V.
Briefwechsel mit Schumacher, Bd. II.
p. 268. [10]
f. Helmholtz,
Wiss.
Abh. II.
p. 611. [11] Crelle's
Journal, 1837. [12]
Theorie der Parallellinien, Berlin, 1840.
Republished, Berlin, 1887.
Translated by Halsted, Austin,
Texas, U.
S.
A. 4th
edition, 1892. [13] Frischauf,
Absolute Geometrie,
nach Johann Bolyai, Leipzig, 1872. Halsted,
The Science Absolute of Space,
translated from the Latin, 4th
edition, Austin,
Texas, U.
S.
A. 1896. [14]
Both Lobatchewsky
and Bolyai,
as Veronese
remarks,
start rather from the point-pair than from distance.
See Frischauf,
Absolute Geometrie, Anhang. [15]
Compare Stallo,
Concepts of Modern Physics,
p. 248. [16] Gesammelte Werke,
pp. 255–268. [17]
On the history of this word,
see Stallo,
Concepts of Modern Physics,
p. 258.
It was used by Kant,
and adapted by Herbart
to almost the same meaning as it bears in Riemann. Herbart,
however,
also uses the word Reihenform
to express a similar idea.
See Psychologie
als Wissenschaft,
I. § 100
and II. § 139,
where Riemann's
analogy with colours is also suggested. [18]
Compare Erdmann's "Grössenbegriff
vom Raum." [19]
Compare Veronese, op. cit.
p. 642: "Riemann
ist in seiner Definition des Begriffs Grösse
dunkel."
See also Veronese's
whole following criticism. [20]
Vorträge und Reden,
Vol. II.
p. 18. [21]
Cf. Klein, Nicht-Euklid,
I.
p. 160. [22]
Since we are considering the curvature at a point,
we are only concerned with the first infinitesimal elements of the geodesics that start from such a point. [23]
Disquisitiones generales circa superficies curvas, Werke, Bd. IV. SS. 219–258, 1827. [24]
Nevertheless,
the Geometries of different surfaces of equal curvature are liable to important differences.
For example,
the cylinder is a surface of zero curvature,
but since its lines of curvature in one direction are finite,
its Geometry coincides with that of the plane only for lengths smaller than the circumference of its generating circle (
see Veronese, op. cit.
p. 644).
Two geodesics on a cylinder may meet in many points.
For surfaces of zero curvature on which this is not possible,
the identity with the plane may be allowed to stand.
Otherwise,