49. Analytic Geometry. 49.1
Consider any time-system
: we will term the space of this
time-system '
-space' and its moments '
-moments';
also the points and straight lines of
-space will be termed
'
-points' and '
-lines,' and rects and levels which
lie in
-moments will be termed '
-rects' and
'
-levels.' If
be any event-particle, then
will denote the
-moment which covers
. If
be
any other time-system, there are no
-moments which are also
-moments, and no
-points which are also
-points; but there are
-levels which are also
-levels and
-rects which are also
-rects.
For the two moments
and
intersect in a
common level which will be called
. Then rects lying
in
are both
-rects and
-rects. In
particular through
in the level
pairs of
mutually normal rects exist, and every rect through
and
is a member of one such pair.
49.2 Let
be any arbitrarily chosen event-particle, which we
will term the origin; and let
be the
-point
occupied by
; and let
,
,
be any triad of mutually rectangular
-rects
in the moment
, each containing
. In this notation
,
, etc., do not denote any particular
entities, but the symbols such as
and
are each to be taken as one whole. Let
denote the
matrix containing
and
, with
analogous meanings for
and
; and let
,
and
denote
respectively the levels containing
and
,
and
,
and
. Let
be
any other event-particle occupying the point
, and let
be the
-rects through
respectively parallel to
,
,
.
In the diagram the third dimension of the moments
and
namely the
-dimension, is suppressed, so that these
moments are diagrammatically represented as two-dimensional.
Point-tracks (in this case
-points) are represented by dotted
lines. The diagram has the defect of representing matrices, such as
, by levels, and is thus liable to lead to unfounded
assumptions.
49.3 Lengths on all rects, whether or no they be
-rects, are measurable in terms of one unit length. But
time-lapses between
-moments—or, what is the same thing,
time-lapses along
-points—must be measured in a
time-unit peculiar to the time-system
, since as yet no means
of obtaining congruent time-units in different time-systems has been
disclosed. We will suppose at present that in each time-system there is
a given arbitrarily chosen unit for time-measurement.
49.4 Let the momentary space of
be referred to the
three rectangular
-rects
,
,
as axes of coordinates; and let the momentary space of
be referred to the three rectangular
-rects
,
,
as axes of
coordinates; and let the time-less space of a [the
-space] be
referred to the three rectangular
-lines respectively included
in the matrices
,
,
as axes of coordinates; and let the four-dimensional space of all
particles be referred to the four axes consisting of the three
-rects
,
,
,
and of the
-point
as axes of co-ordinates.
49.5 Let
be any event-particle in the moment
, and let
occupy the
-point
which intersects the moment
in the event-particle
. Let the lapse of time between the moments
and
be
, where
is positive when
is subsequent to
; and let the coordinates
of the
-point
in the
-space be
(
). Then the coordinates of
in the momentary space of
and of
in the momentary
space of
are also
(
). Also the '
-coordinates'
of
in the four-dimensional space of particles are
(
); this fact for
can also be expressed by saying that
occupies the
-point (
)
at the
-time
.
A moment, viewed as a locus of event-particles, is represented
by a linear equation in the four coordinates
(
).
But the converse is not true; namely, not every linear equation
represents a moment. A pair of linear equations represent a level or
a matrix, and three independent linear equations represent a rect or a
point-track or a null-track.
49.6 If
and
be any two time-systems, two
sets of mutually normal axes,
,
and
,
can be found as in the previous subarticle. But these
two sets can evidently be so adjusted that
is
identical with
and
is identical with
, where the two rects
(
) must both lie in the
level
.
Then the matrix normal to this level at
will be denoted by
; it contains through
one
-point
, one
-point
one
-rect
, and one
-rect
. Then any event-particle is referred
to the axes
for the system
, and to the axes
for the system
. Let its
-coordinates be
(
) and its
-coordinates be (
),
where
, and
.
In the diagram, for the sake of simplicity, the particle
is in the matrix
; and its coordinates [as in the
diagram] in the two systems are (
)
and (
), where
(with its proper sign) is
,
(with its proper sign) is
,
(with its proper sign)
is
, and
(with its proper sign) is
.
A pair of sets of four axes for a and allied as described in this
subarticle are called 'mutual axes' for the two systems.
49.7 The formulae for transformation from the
a-coordinates to the
-coordinates, referred to mutual axes, are
obviously of the form
where
are constants dependent on the two systems
and
and
on the two arbitrarily chosen units of time-lapse in
and
, but evidently not dependent on the arbitrarily chosen set of
rectangular rects
and
in the level
.
The corresponding (
)-equations, interchanging
and
, are
The two pairs of (
)-equations, (i) and (ii), must be equivalent.
The conditions are
Only four out of these five conditions are independent.
50. The Principle of Kinematic Symmetry.
50.1 Consider any other time-system
.
The
-point (
) occupied by
(
)
and the
-point occupied by the same event-particle lie on a
matrix
which includes an
-line
(
) of which every
-point is intersected by
. Thus
correlates the
-point
(
) with the
-time
and the neighbouring
-point on
namely
(
),
with the neighbouring
-time
. In this way
makes every set of
-coordinates of a variable
-point to be a function
of
; namely it correlates an
-point
(
) with the velocity
(
), which can
also be written
Analogously the same time-system
correlates a
-point
(
) with the velocity
(
) which can be
written
Now the time-system
indicates a definite transference from an
event-particle (
) to another
event-particle (
)
occupying the same
-point (
),
where any mutually normal
-coordinates are employed. The former
event-particle is that indicated by
(
)
and by (
), and the
latter event-particle by
(
)
and by
(
).
Hence from equations (i) of 49.7
Now
is any time-system. First identify it with
.
Then
.
Hence
, and
is the velocity of the time-system
in the space of
[or, more briefly, the 'velocity of
in
']. Let this
velocity be
; it is evidently along the
-axis in
the space of
, and
Again identify the system
with
. Then
;
and hence
, and
is the velocity of
in
. Let this
velocity be
; it is along the
-axis in the space
of
, and
50.2 We will now introduce what we will term the 'Principle of
Kinematic Symmetry.'
Before enunciating this principle it is necessary to determine a
standard method of choosing the positive directions of the axes
and
in the matrix
and of the axes
and
. By reference to the figure of
subarticle 45.2 it will be seen that, of the four
angular regions into which the rects
and
divide the matrix
, two vertically opposite regions
include no point-tracks passing through
and the remaining two such
regions include point-tracks as well as rects through
. The standard
choice of positive directions for
and
is
such that the two regions bounded one by both positive directions of
these axes, and the other by both negative directions, should include
only rects passing through
.
The positive directions for
and
are
settled by the rule that a positive measure of lapse of time should
indicate subsequence in the time-order to the moment
.
This rule is definite because of the ultimate distinction between
antecedence and subsequence in time, which has not otherwise been made
use of. This standard choice of positive directions along mutual axes
for two time-systems will always be adopted.
50.3 The principle of kinematic symmetry has
two parts, enunciating consequences which flow from the fact that the
time-units in two time-systems
and
are congruent.
The first part may be taken as the definition, or necessary and
sufficient test, of such congruence.
The first part of the principle can be enunciated as the statement that
the measures of relative velocities [i.e. the velocity of
in
and of
in
] are equal and opposite;
namely
The second part is the principle of the symmetry of two time-systems in
respect to transverse velocities; namely, if a velocity
in
, normally transverse to the direction of
in
, is represented by the velocity (
)
in
, where
is along the direction of
in
and
′ is normally transverse to it, then
the same magnitude of velocity
in
, normally transverse
to the direction of
in
, is represented by the
velocity (
) in
, where
is along the direction of
in
,
and
′ is normally transverse to it.
From the first part of the principle, by (ii) and (iii) of
50.1, we deduce
In order to apply the second part of the principle we first identify
with
),
then from (i) and (ii) of 50.1
Again we identify
(
with
), and
by interchanging
and
in the above formulae we find
Hence by the second part of the principle
51. Transitivity of Congruence.
51.1 It follows, from (iii) of
49.7, and from (ii) and (iii) of
50.1, and from (i), (ii), (iii) of
50.3, that equations (i) of
50.1 can be written
We can now express
and
in terms of
and an absolute constant by considering deductions
from the transitivity of congruence.
51.2 Let
be a time-system such
that the level
contains
and
, and let these rects be the axes
and
. Then the matrix
contains
,
,
and
. Thus we have obtained a set of mutual axes for
and
; namely,
(
) and (
),
where
and
now play
the part that
and
sustain for
and
. Thus the velocities of the time-system
in
and
are, by (i) of 51.1,
connected by
We have here assumed the congruence of the time-units in
and
.
Now identify
and
. Then
Hence from (i) of 51.1
Again identify
with
. Then
Hence from (i) of this subarticle
From (ii) and (iii) and (i) of 50.3
51.3 Evidently if
be any other member
of the collinear set of time-systems (
,
), then
Hence if
be a collinear set of time-systems, and
,
,
,
be any four of its members,
and hence, since
, we
obtain
where
is a constant for the collinear set.
Furthermore, if
be a time-system not belonging to
but
related to
and
as explained in 51.2,
51.4 Now let
,
,
be any three
non-collinear time-systems, and construct a diagram to represent
elements in the time-less space of
according to the familiar
method of geometricians.
The points of the diagram symbolise
-points, and the straight
lines of the diagram symbolise
-lines. Let
be any
-point and let
be the direction in
-space
of the velocity
. Then
is the direction in
-space of the velocity (positive or negative) of any member of
the collinear set (
).
Let
be the direction in
-space of the velocity
; by hypothesis
is distinct from
. Let
be the
-line perpendicular to the
-plane
, and let
be a time-system whose velocity in
,
namely
, is along
. Let
denote the
collinear set (
),
′ the collinear set
(
), and
″ the collinear
set (
). Hence from (vi) of 51.3
Hence from (vii) of 51.3
Hence, since
and
, it is easy to prove
that
is the same for any pair of time-systems; in other words,
that
is an absolute constant.
52. The Three Types of Kinematics.
52.1 There are thus three types of kinematics possible, according
as
is positive, negative, or infinite. The formally possible
type where
is zero requires that either or
should be zero; by reference to (i) of
49.7 and to (i) of 51.1 this
supposition is seen to lead to results in such obvious contradiction to
experience as to preclude the necessity for further examination. Let us
name the types retained (according to the familiar habit) the
'hyperbolic,' the 'elliptic' and the 'parabolic' types of kinematics.
52.2 First consider the hyperbolic type and
put
for
. The equations of articles
49 and 51 then become
The equations of transformation, namely (ii), can be expressed
symmetrically as between
and
by means of the scheme
[where
]
| |
, |
, |
, |
 |
 |
, |
0, |
0, |
 |
 |
0, |
1, |
0, |
0 |
 |
0, |
0, |
1, |
0 |
 |
 |
0, |
0, |
 |
52.3 We notice that
The integral
taken throughout the four-dimensional region of the set of event-particles
which analyse [cf. 37.3] an event
will be
called the 'absolute extent' of
. It follows from (i) that the
absolute extent of an event is independent of the time-system in which
its measure is expressed.
Furthermore if
be any function of
(
), it can by (ii) of
52.2 be also expressed as a function of
(
), and then by (i)
or, in more familiar form,
where the limits are taken to include some event.
We may expect important physical properties to be expressible in terms
of such integrals, in particular where
is an invariant form for
the equations of transformation of 52.2, and when
the conditions, which the quantity represented by the integral
satisfies, are also invariant in their expression in different
time-systems.
The formulae of this subarticle hold of each type of kinematics.
52.4 The hyperbolic type of kinematics has issued in the formulae
of the Larmor-Lorentz-Einstein theory of electromagnetic relativity,
namely, the theory by which with a certain amount of interpretation the
electromagnetic equations are invariant for these transformations.
The physical meaning of
is also well known; namely, any velocity
which in any time-system is of magnitude
is of the same magnitude
in every other time-system. No assumption of the existence of a velocity
with this property or of the electromagnetic invariance has entered into
the deduction of the kinematic equations of the hyperbolic type. A
velocity greater than
cannot represent any time-system, and
accordingly its physical significance must be entirely different from
that of a velocity less than
.
52.5 It is easily proved from (ii) of 52.2
that
If the origin
and the event-particle
, i.e.
(
),
be co-momental and
be the time-system whose moment
, contains
, then by (i)
If
and
be sequent and on a point-track, and
be
the time-system whose point
is occupied by
,
then by (i)
Thus there are three ways in which the 'separation' between two
event-particles (
and
) can be estimated; namely, (1) in any
assumed time-system
the
-distance between the
-points occupied by the event-particles measures
-space separation: (2) the lapse of
-time between
the
-moments occupied by the event-particles measures
-time separation: and (3) if the event-particles be co-momental,
measures the 'proper' space separation and there is no 'proper' time
separation; and if the particles be sequent,
measures the 'proper' time separation and there is no
'proper' space separation.
In the framing of physical laws it is essential to consider what measure
of separation is relevant. It is to be noted that there may be
time-systems
(other than
) of special relevance to the
phenomena in question. It is not at all obvious that invariance of form
in respect to all time-systems is a requisite in the complete expression
of such laws; namely, the demand for relativistic equations is only of
limited applicability.
If
and
be on a null-track
Event-particles on the same null-track may be expected to have special
physical relations to each other. Call such event-particles 'co-null.'
52.6 We may conceive a special time-system
associated (by some means) with each event-particle
(
). Thus
is a
function of these four co-ordinates of a particle; or in other words,
(
)
are functions of (
).
A correlation of time-systems to event-particles which is one-many, so
that there is one and only one time-system corresponding to each
event-particle, is called a 'complete kinematic correlation.' The
portion of that correlation which only concerns event-particles at the
time
is called a 'kinematic
-correlation.'
Other portions can be selected by confining the event-particles to
certain regions in the
-space.
If in a certain kinematic correlation the time-system it be correlated to
(
), then
is
called the time-system of
(
) 'proper' to that
correlation. The 'proper' time-system of an event-particle always
refers to a certain kinematic correlation implicitly understood.
Furthermore (
)
is the velocity at (
) due to the
implicitly understood kinematic correlation at the
-time
.
Then,
being the proper time-system at
(
),
Then equations (iii) of 52.2 can be written
The kinematic symmetry as between
and
is now
apparent in the formulae. The first of equations (ii) can be replaced by
52.7 In considering the elliptic type of kinematics put
for
. The equations of article 51 are now
embodied in the scheme
| |
, |
, |
, |
 |
 |
, |
0, |
0, |
 |
 |
0, |
1, |
0, |
0 |
 |
0, |
0, |
1, |
0 |
 |
 |
0, |
0, |
 |
The fundamental distinction between space and time, i.e. between rects
and point-tracks, has failed to find any expression in the formulae for
measurement relations. Accordingly with this type of kinematics, it
would be natural to suppose that the distinction does not exist and that
every rect was a point-track and every point-track a rect. This
conception is logically possible but does not appear to correspond to
the properties of the external world of events as we know it.
Furthermore the electromagnetic equations lose their invariant property.
Altogether there appear to be good reasons for putting aside the
elliptic type of kinematics as inapplicable to nature.
52.8 In the parabolic type of kinematics we put
Hence
Then from (ii) of 51.1 and (ii) of
50.3 and (iii) of 50.1
Thus equations (i) of 49.7 give
These are the formulae for the ordinary Newtonian relativity.
These formulae are well in accordance with common sense and are in fact
the formulae naturally suggested by ordinary experience. To some extent
the hyperbolic formulae lead to unexpected results, though, if
be
a velocity not less than that of light, the divergences from the
deliverances of common sense take place in respect to phenomena which
are not manifest in ordinary experience. But when by refined methods of
observation the divergences between the two types of kinematics should
be apparent to the senses, experiment has, so far, pronounced in favour
of the hyperbolic type. Accordingly it is this type which we consider in
the sequel.
52.9 There is however one objection to the hyperbolic type, as
compared to the parabolic type, which is worth considering. In the
hyperbolic kinematics there is an absolute velocity
with special
properties in nature. The difficulty which is thus occasioned is rather
an offence to philosophic instincts than a logical puzzle. But certainly
our familiar experience, in some way which it is difficult to formulate
in words, leads us to shun the introduction of such absolute physical
quantities. This particular difficulty is largely diminished by noting
that the existence of
with its peculiar properties really means
that the space-units and time-units are comparable; namely, there is a
natural relation between them to be expressed by taking
to be
unity. Either the time-unit would then be inconveniently small or the
space-unit inconveniently large; but this inconvenience does not alter
the fact that congruence between time and space is definable. Always
when a possible definition of congruence is omitted, such absolute
physical quantities occur. The fact that, so far as time and space are
concerned, the existence of a congruence theory seems paradoxical is due
to absence of any phenomena depending on that theory except in very
exceptional circumstances produced by refined observations.