(Concepts of
simultaneity / Synchronization method / The term ux/c2)
In this
section, Feynman discusses concepts
of simultaneity, a synchronization
method, and the term ux/c2.
1. Concepts of simultaneity:
“…when a man in a space ship thinks the times at two
locations are simultaneous, equal values of t′
in his coordinate system must correspond to different values of t in the other coordinate system! (Feynman et al., 1963, section 15–6 Simultaneity).”
The concept of simultaneity can be distinguished as local simultaneity
and distant simultaneity. In his seminal paper, Einstein (1905) first defines
local simultaneity as “… for example, I say that ‘the train arrives here at seven o’clock,’
that means,
more or
less,
‘The pointing of the
small hand of my
clock to 7 and the arrival
of the train are simultaneous events.” On the other hand, Feynman explains the concept of distant
simultaneity in which an observer (in an inertial frame of reference) thinks
the times at two locations are the same,
but it must correspond to different values of t in another inertial frame. In other words, the impossibility of distant simultaneity is illustrated
by a disagreement among observers from different inertial frames of reference on
the order of events.
It is worthwhile to discuss
the concept of an event in the context of simultaneity. Specifically, an event occurs
at a point in space-time whereby it has a definite place and a definite time (Mermin,
2009). One may expect Feynman to elaborate that the concept of an event is an
idealization just like the concept of a point in space. It is different from a
real event where a lightning strike that has a finite extent. Furthermore,
physicists idealize Einstein’s clocks as infinitely small objects. Importantly,
distant simultaneity is related to
two spatially separated events and it can be shown to be a logically
contradictory concept using Einstein’s postulate of constant speed of light.
2. Synchronization method:
“Let us then suppose that the man in S′ synchronizes his clocks by this
particular method. Let us see whether an observer in system S would agree that the two clocks are
synchronous (Feynman et al., 1963, section 15–6 Simultaneity).”
According to Feynman, one way of synchronizing two clocks in a moving space ship (system S′) is to place a clock each at the front
end and rear end of the ship. Light signals are sent out from the midpoint of
the ship in opposite directions and they arrive at both clocks at the same time
because they move at the same speed. A
man in an inertial frame of reference S
would reason that more time is needed for the light signal to reach the front
clock because the ship was moving forward (or moving away from the light signal).
This is in contrast to the rear clock that was moving toward the light signal
and so the distance between them appears shorter. In summary, the light signal
would reach the rear clock earlier as compared to the front clock and it means
that the two observers would disagree with which event would occur first.
One may hope Feynman to discuss why the synchronization of clocks is
based on the speed of light instead of the speed of sound. There could be further clarifications whether
this method of synchronization is a matter of convention and the possibility of
using sound waves to synchronize clocks. However, it is advantageous to use light signals because they are essentially electromagnetic waves that do
not require a material medium for transmission and the speed of light in vacuum
is independent of its wavelength, amplitude, or direction of propagation (Resnick, 1968). It is worth mentioning that Einstein’s invention of the
theory of special relativity helps to solve problems of Maxwell’s equations. We
should not overlook the obvious fact that Maxwell’s equations describe not only
space and time, but electromagnetic waves.
3. The term ux/c2:
“The most interesting term in that equation is the ux/c2
in the numerator, because that is quite new and unexpected (Feynman et al., 1963, section 15–6 Simultaneity).”
Feynman mentions that the most interesting term in the equation is ux/c2.
The term means that two events that occur at two separated places at the same
time, as seen by Moe in S′ frame, do not
happen at the same time as seen by Joe in S
frame. Feynman calls this circumstance as “failure of simultaneity at a
distance,” but he did not provide a derivation of the term. Interestingly, Morin (2003)
provides derivations of this term in eight different contexts. However, the impossibility
of distant simultaneity can be explained using the term ux/c2. That is,
two events that appear simultaneously to an observer may appear to have a time
difference depending on the relative velocity of another observer (u) and the distance between the two
events (x).
A simple derivation of the term ux/c2 is to compare the time difference
when two light signals reach clock A and clock B in a moving train that is x distance in length and moving at a
speed of u from a ground observer’s (S) perspective (Resnick, 1968). When a
light signal moving to left meets clock A,
at t = tA, we have ctA = (x/2)Ö(1 – u2/c2) – utA. The term utA has a minus sign because
the light signal and the clock A move in the opposite directions. When a light signal
moving to the right meets clock B at t = tB, we have ctB = (x/2)Ö(1 – u2/c2) + utB. The term utB has a plus sign because the light signal and the clock A move in the
same direction.) Comparing the time of two clocks (S frame), the time difference observed is Dt = (x/2)Ö(1–u2/c2)/(c–u)–(x/2)Ö(1–u2/c2)/(c+u) = (ux)[Ö(1–u2/c2)]/(c2–u2). Lastly, taking into account of time dilation, Dt' = DtÖ(1–u2/c2), it can be simplified as Dt' = (ux)(1–u2/c2)/(c2–v2) = ux/c2.
Questions for discussion:
1.
How would you define local simultaneity and distant simultaneity?
2. Why is the synchronization of clocks based on the
speed of light instead of the speed of sound?
3. Does the term ux/c2 mean that it is impossible for a guy and a gal
living separately in two different countries to fall in love simultaneously?
The moral of the lesson: the term ux/c2 implies that the clocks at two locations that appear the same in an inertial frame of reference must correspond to different
values of time in another inertial
frame.
References:
1. Einstein,
A. (1905). On the electrodynamics of moving bodies. Annalen
der Physik, 322(10), 891-921.
2. Feynman, R. P.,
Leighton, R. B., & Sands, M. (1963). The Feynman Lectures on Physics, Vol
I: Mainly mechanics,
radiation, and heat. Reading, MA: Addison-Wesley.
3. Mermin, N. D. (2009). It’s
about time: understanding
Einstein’s relativity. Princeton: Princeton University Press.
4. Morin, D. (2003). Introductory Classical Mechanics.
Cambridge: Cambridge University Press.
5. Resnick, R. (1968). Introduction
to Special Relativity. New York: Wiley.
No comments:
Post a Comment