We must find a mechanism to keep the LCE constant. To do so, we consider whether two out-of-phase MTWs propagating from the opposite directions on a MM originally have HDRE.
We start by analyzing the relativistic kinetic energies of the two out-of-phase waves propagating from the opposite directions on a MM. Two physical quantities that contribute to them are the velocity and RM of each portion which is in wave motion (WM).
4.3. RM Contributing to RKE
The RM in WM is generally the amount obtained by multiplying unit length by mass density. Viewed from a different aspect, the RM in WM corresponds to the coordinate interval (CI) of the wave rather than the length of it.
Firstly, we consider the amount of RM of the wave propagating in the opposite direction of the MM in . Let be its wave. Here we need to take the relativity of simultaneity in SR into account. Suppose that clocks are fixed at certain equal intervals along the and ′ axes respectively. Moreover, we assume that they are synchronized in some way on each axis.
According to the relativity of simultaneity, the clocks at the back of the MM always go by fast compared to those at the front of it. This means that, in
, an event A in the back of the MM occurs earlier than one B in the front of it even if both of them take place in
′ simultaneously. When a wave propagates in the opposite direction of the MM, the
′ coordinate corresponding to the leading end of the wave (LEW) is at the back of the MM compared to that corresponding to the WS. Hence, the time on the former
′ coordinate goes by faster than that on the latter one. Let
and
be the positions of the WS and the LEW at a certain time,
, in
′, respectively. When observing the wave from
, if the position
and time
of the WS coincide with
and
in
′ respectively, then the LEW is not at
. The time on
is not
and
is already past. Therefore, the LEW observed from
has already passed through
and propagates backward on the MM compared to that observed in
′. When observing the LEW from
, it is at
that is positioned farther from
compared with
. Also, at that moment, the clock on
observed in
shows
. Here we can represent the CI by the absolute value. Then the coordinate interval of the portion in WM (CIPWM) observed from
is
, while that in
′ is
. Therefore, we obtain
Moreover, we assume that the portion corresponding to
has a TV
in
′. Converting
in
′ into the corresponding TV,
, in
, from Eq. (3),
since
As indicated above, the LEW in
arrives at
when the TV of the portion becomes
in
′. Hence, the CIPWM with
is
. As a result, we can find that the CIPWM having
in
,
, is larger than one having
in
′,
, i.e.,
Here the term, interval, does not denote the distance between the coordinates of the portion in WM, in other words, the length of the wave. On the other hand, the CI corresponds to RM. Therefore, we can calculate the former using the latter. The RM of the portion having
in
,
, is defined as:
where
is RM per unit CI in
′. Here
in
is determined using
in
′ because the RM corresponding to the CI is depended on the proper
in
′ relative to which the ME is at rest. The RM,
, having
in
′ is equal to a value obtained by multiplying
by
, i.e.,
. Then, since
from inequality (7), we find that
having
in
is larger than
having
in
′. The difference in the RM between the former and the latter results from that of the CI because
is the same value in each frame of reference. Since its difference is proportional to the ratio of the CI, we get
The difference in the CI, in other words, that in the RM between and ′, as indicated above, depends upon the time difference at the coordinates on the ′ axis observed from . This time difference is determined according to the velocity of ′ relative to.
Secondly, we analyze the amount of RM of the wave propagating in the advancing direction of the MM in
. Let
be its wave. In contrast to
, in
, the
′ coordinate corresponding to the LEW is at the front of the MM compared with that corresponding to the WS. Hence, the time on the former
′ coordinate goes by slower than that on the latter
′ coordinate. Then, if the position and time of the WS in
coincide with them of the WS in
′ respectively, then the LEW in
′ propagates forward on the MM compared to that observed from
. In other words, the latter is at the back of the MM compared with the former. This means that the CIPWM in
is smaller than that in
′. Let
and
be the transverse velocities of the portions corresponding to each CIPWM in
′ and
, respectively. The latter velocity is also one obtained by converting
according to the Lorentz transformation. Then the CIPWM having
in
,
, is smaller than
having
in
′, i.e.,
The RM of the portion having
in
,
, is defined as:
Furthermore, since
from inequality (10), we find that
having
in
is smaller than
having
in
′. Again, since its difference is proportional to the ratio of the CI, we obtain
We assume that the magnitudes of velocities of
and
are the same. Thus, those of velocities of
and
are also the same. Then combining expressions (7) and (10) yields
Furthermore, combining expressions (9) and (12), we obtain
Consequently, the RM of a portion of is larger than that of a portion of when each portion has the TV of the same magnitude.
Inequalities (13) and (14) hold true for any CIPWM having the TV of the same magnitude. Therefore, we get
where
and
are the total CIPWM of
and
in
respectively and
is that of one wave in
′. Furthermore, we obtain
where
and
are the total RM of
and
in
respectively and
is that of one wave in
′.
Here we need to bear in mind that we consider and compare only the amount of RM of the portions that are in WM. Total RM including the portions that are not in WM is invariant for the Lorentz transformation.