The formation of this concept is achieved by using one of the clocks,
say , as a reference clock which measures and collects two kinds of
data about all the other clocks, say
: Doppler shifts and
instantaneous distance of
from
.
Doppler shift measurements are frequency measurements. The emission
frequencies of all clocks are the same, say
.
Consequently, the frequencies
received and measured by
yield the corresponding Doppler shift factors
The second kind of measurement is the instantaneous separation.
Suppose at some instant of time, say ,
measures the distances
between
and the clocks
.
One way of doing this is to have
operate his transmitter
and receiver as a radar device.
We now say that is equivalent to
, or more briefly
, if
The properties of this equivalence class do not depend on the time at
which makes the distance measurements and hence not on the value
of the ratio
. Indeed, if instead of
that time had
been , say
, then the corresponding distance measurements would
be
, then one would still have a set of equal
ratios
The purpose of an inertial reference frame is for a physicist/observer
to use its recording clocks to measure time and space
displacements. These measurements consist of establishing quantitative
relationships (typically via counting) to a standard which serves as a
unit. For a time measurement the unit is the standard interval between
any two successive ticks of a clock. For a space measurement the unit
is the (logarithm of the) standard Doppler shift factor between any
pair of nearest neighbor clocks. Thus the array of clocks forms a
lattice which is periodic but is expanding uniformly: the recession
velocity between any neighboring pair of clocks is one and the
same. This periodicity is an obvious but tacit stipulation in what is
meant by ``expanding inertial frame''. Because of this property any
one of the recording clocks can play the role of the
reference clock
, which is to say that the equivalence relation,
Eq.(1), is independent of the choice of
.
The two kinds of measurements which gave rise to the equivalence
relation between recording clocks also serve to synchronize their
operations. Every clock synchronizes itself to its nearest neighbor by
setting its own clock reading to the ratio of (i) the nearest neighbor
distance and (ii) the Doppler shift determined velocity. Thus the
common ratio, Eq.(1), is the synchronous time common to
all recording clocks. This common time has an obvious interpretation:
The straight-line extensions into the past of all clock histories
intersect simultaneously in a common point. This is a singular event,
which corresponds to . The common synchronous time of these
clocks is the elapsed proper time since then. However, it is obvious
that this singular event is irrelevant for the definition of the
expanding inertial frame. What is relevant instead is the ability of
the recording clocks to measure Doppler shifts and distances, which
presupposes that
. In fact, these clocks might not even
have existed until they performed their measurements.
Having constructed the spacetime measuring apparatus, we indicate in general terms how to make spacetime measurements of particles and fields.