The Michelson–Morley experiment was an attempt to detect the existence of aether,
a supposed medium permeating space that was thought to be the carrier
of light waves. The experiment was performed between April and July 1887
by Albert A. Michelson and Edward W. Morley at what is now Case Western Reserve University in Cleveland, Ohio, and published in November of the same year. It compared the speed of light in perpendicular directions, in an attempt to detect the relative motion of matter through the stationary luminiferous aether
('aether wind'). The result was negative, in that Michelson and Morley
found no significant difference between the speed of light in the
direction of movement through the presumed aether, and the speed at
right angles. This result is generally considered to be the first strong
evidence against the then-prevalent aether theory, and initiated a line of research that eventually led to special relativity, which rules out a stationary aether. Of this experiment, Einstein
wrote, "If the Michelson–Morley experiment had not brought us into
serious embarrassment, no one would have regarded the relativity theory
as a (halfway) redemption."
Michelson–Morley type experiments have been repeated many times
with steadily increasing sensitivity. These include experiments from
1902 to 1905, and a series of experiments in the 1920s. More recent optical resonator experiments confirmed the absence of any aether wind at the 10−17 level. Together with the Ives–Stilwell and Kennedy–Thorndike experiments, Michelson–Morley type experiments form one of the fundamental tests of special relativity theory.
Detecting the aether
Physics
theories of the late 19th century assumed that just as surface water
waves must have a supporting substance, i.e., a "medium", to move across
(in this case water), and audible sound requires a medium to transmit its wave motions (such as air or water), so light must also require a medium, the "luminiferous aether",
to transmit its wave motions. Because light can travel through a
vacuum, it was assumed that even a vacuum must be filled with aether.
Because the speed of light is so great, and because material bodies pass through the aether
without obvious friction or drag, it was assumed to have a highly
unusual combination of properties. Designing experiments to investigate
these properties was a high priority of 19th century physics.
Earth orbits around the Sun
at a speed of around 30 km/s (18.64 mi/s), or 108,000 km/h
(67,000 mph). The Earth is in motion, so two main possibilities were
considered: (1) The aether is stationary and only partially dragged by Earth (proposed by Augustin-Jean Fresnel in 1818), or (2) the aether is completely dragged by Earth and thus shares its motion at Earth's surface (proposed by Sir George Stokes, 1st Baronet in 1844). In addition, James Clerk Maxwell (1865) recognized the electromagnetic nature of light and developed what are now called Maxwell's equations,
but these equations were still interpreted as describing the motion of
waves through an aether, whose state of motion was unknown. Eventually,
Fresnel's idea of an (almost) stationary aether was preferred because it
appeared to be confirmed by the Fizeau experiment (1851) and the aberration of star light.
According to the stationary and the partially-dragged aether
hypotheses, Earth and the aether are in relative motion, implying that a
so-called "aether wind" (Fig. 2) should exist. Although it would be
possible, in theory, for the Earth's motion to match that of the aether
at one moment in time, it was not possible for the Earth to remain at
rest with respect to the aether at all times, because of the variation
in both the direction and the speed of the motion. At any given point on
the Earth's surface, the magnitude and direction of the wind would vary
with time of day and season. By analyzing the return speed of light in
different directions at various different times, it was thought to be
possible to measure the motion of the Earth relative to the aether. The
expected relative difference in the measured speed of light was quite
small, given that the velocity of the Earth in its orbit around the Sun
has a magnitude of about one hundredth of one percent of the speed of
light.
During the mid-19th century, measurements of aether wind effects of first order, i.e., effects proportional to v/c (v being Earth's velocity, c
the speed of light) were thought to be possible, but no direct
measurement of the speed of light was possible with the accuracy
required. For instance, the Fizeau–Foucault apparatus
could measure the speed of light to perhaps 5% accuracy, which was
quite inadequate for measuring directly a first-order 0.01% change in
the speed of light. A number of physicists therefore attempted to make
measurements of indirect first-order effects not of the speed of light
itself, but of variations in the speed of light (see First order aether-drift experiments). The Hoek experiment, for example, was intended to detect interferometric fringe shifts
due to speed differences of oppositely propagating light waves through
water at rest. The results of such experiments were all negative. This could be explained by using Fresnel's dragging coefficient,
according to which the aether and thus light are partially dragged by
moving matter. Partial aether-dragging would thwart attempts to measure
any first order change in the speed of light. As pointed out by Maxwell
(1878), only experimental arrangements capable of measuring second order
effects would have any hope of detecting aether drift, i.e., effects
proportional to v2/c2. Existing experimental setups, however, were not sensitive enough to measure effects of that size.
1881 and 1887 experiments
Michelson experiment (1881)
Michelson had a solution to the problem of how to construct a device
sufficiently accurate to detect aether flow. In 1877, while teaching at
his alma mater, the United States Naval Academy
in Annapolis, Michelson conducted his first known light speed
experiments as a part of a classroom demonstration. In 1881, he left
active U.S. Naval service while in Germany concluding his studies. In
that year, Michelson used a prototype experimental device to make
several more measurements.
The device he designed, later known as a Michelson interferometer, sent yellow light from a sodium flame (for alignment), or white light (for the actual observations), through a half-silvered mirror
that was used to split it into two beams traveling at right angles to
one another. After leaving the splitter, the beams traveled out to the
ends of long arms where they were reflected back into the middle by
small mirrors. They then recombined on the far side of the splitter in
an eyepiece, producing a pattern of constructive and destructive interference whose transverse displacement would depend on the relative time it takes light to transit the longitudinal vs.
the transverse arms. If the Earth is traveling through an aether
medium, a beam reflecting back and forth parallel to the flow of aether
would take longer than a beam reflecting perpendicular to the aether
because the time gained from traveling downwind is less than that lost
traveling upwind. Michelson expected that the Earth's motion would
produce a fringe shift
equal to 0.04 fringes—that is, of the separation between areas of the
same intensity. He did not observe the expected shift; the greatest
average deviation that he measured (in the northwest direction) was only
0.018 fringes; most of his measurements were much less. His conclusion
was that Fresnel's hypothesis of a stationary aether with partial aether
dragging would have to be rejected, and thus he confirmed Stokes'
hypothesis of complete aether dragging.
However, Alfred Potier (and later Hendrik Lorentz)
pointed out to Michelson that he had made an error of calculation, and
that the expected fringe shift should have been only 0.02 fringes.
Michelson's apparatus was subject to experimental errors far too large
to say anything conclusive about the aether wind. Definitive measurement
of the aether wind would require an experiment with greater accuracy
and better controls than the original. Nevertheless, the prototype was
successful in demonstrating that the basic method was feasible.
Michelson–Morley experiment (1887)
In 1885, Michelson began a collaboration with Edward Morley, spending considerable time and money to confirm with higher accuracy Fizeau's 1851 experiment on Fresnel's drag coefficient, to improve on Michelson's 1881 experiment, and to establish the wavelength of light as a standard of length.
At this time Michelson was professor of physics at the Case School of
Applied Science, and Morley was professor of chemistry at Western
Reserve University (WRU), which shared a campus with the Case School on
the eastern edge of Cleveland. Michelson suffered a nervous breakdown
in September 1885, from which he recovered by October 1885. Morley
ascribed this breakdown to the intense work of Michelson during the
preparation of the experiments. In 1886, Michelson and Morley
successfully confirmed Fresnel's drag coefficient – this result was also
considered as a confirmation of the stationary aether concept.
This result strengthened their hope of finding the aether wind.
Michelson and Morley created an improved version of the Michelson
experiment with more than enough accuracy to detect this hypothetical
effect. The experiment was performed in several periods of concentrated
observations between April and July 1887, in the basement of Adelbert
Dormitory of WRU (later renamed Pierce Hall, demolished in 1962).
As shown in Fig. 5, the light was repeatedly reflected back and
forth along the arms of the interferometer, increasing the path length
to 11 m (36 ft). At this length, the drift would be about 0.4 fringes.
To make that easily detectable, the apparatus was assembled in a closed
room in the basement of the heavy stone dormitory, eliminating most
thermal and vibrational effects. Vibrations were further reduced by
building the apparatus on top of a large block of sandstone (Fig. 1),
about a foot thick and five feet square, which was then floated in a
circular trough of mercury. They estimated that effects of about 0.01
fringe would be detectable.
Michelson and Morley and other early experimentalists using
interferometric techniques in an attempt to measure the properties of
the luminiferous aether, used (partially) monochromatic light only for
initially setting up their equipment, always switching to white light
for the actual measurements. The reason is that measurements were
recorded visually. Purely monochromatic light would result in a uniform
fringe pattern. Lacking modern means of environmental temperature control,
experimentalists struggled with continual fringe drift even when the
interferometer was set up in a basement. Because the fringes would
occasionally disappear due to vibrations caused by passing horse
traffic, distant thunderstorms and the like, an observer could easily
"get lost" when the fringes returned to visibility. The advantages of
white light, which produced a distinctive colored fringe pattern, far
outweighed the difficulties of aligning the apparatus due to its low coherence length. As Dayton Miller
wrote, "White light fringes were chosen for the observations because
they consist of a small group of fringes having a central, sharply
defined black fringe which forms a permanent zero reference mark for all
readings."
Use of partially monochromatic light (yellow sodium light) during
initial alignment enabled the researchers to locate the position of
equal path length, more or less easily, before switching to white light.
The mercury trough allowed the device to turn with close to zero
friction, so that once having given the sandstone block a single push it
would slowly rotate through the entire range of possible angles to the
"aether wind," while measurements were continuously observed by looking
through the eyepiece. The hypothesis of aether drift implies that
because one of the arms would inevitably turn into the direction of the
wind at the same time that another arm was turning perpendicularly to
the wind, an effect should be noticeable even over a period of minutes.
The expectation was that the effect would be graphable as a sine
wave with two peaks and two troughs per rotation of the device. This
result could have been expected because during each full rotation, each
arm would be parallel to the wind twice (facing into and away from the
wind giving identical readings) and perpendicular to the wind twice.
Additionally, due to the Earth's rotation, the wind would be expected to
show periodic changes in direction and magnitude during the course of a
sidereal day.
Because of the motion of the Earth around the Sun, the measured data were also expected to show annual variations.
Most famous "failed" experiment
After all this thought and preparation, the experiment became what has been called the most famous failed experiment in history. Instead of providing insight into the properties of the aether, Michelson and Morley's article in the American Journal of Science
reported the measurement to be as small as one-fortieth of the expected
displacement (Fig. 7), but "since the displacement is proportional to
the square of the velocity" they concluded that the measured velocity
was "probably less than one-sixth" of the expected velocity of the
Earth's motion in orbit and "certainly less than one-fourth."
Although this small "velocity" was measured, it was considered far too
small to be used as evidence of speed relative to the aether, and it was
understood to be within the range of an experimental error that would
allow the speed to actually be zero. For instance, Michelson wrote about the "decidedly negative result" in a letter to Lord Rayleigh in August 1887:
The Experiments on the relative motion of the earth and ether have been completed and the result decidedly negative. The expected deviation of the interference fringes from the zero should have been 0.40 of a fringe – the maximum displacement was 0.02 and the average much less than 0.01 – and then not in the right place. As displacement is proportional to squares of the relative velocities it follows that if the ether does slip past the relative velocity is less than one sixth of the earth’s velocity.
— Albert Abraham Michelson, 1887
From the standpoint of the then current aether models, the experimental results were conflicting. The Fizeau experiment
and its 1886 repetition by Michelson and Morley apparently confirmed
the stationary aether with partial aether dragging, and refuted complete
aether dragging. On the other hand, the much more precise
Michelson–Morley experiment (1887) apparently confirmed complete aether
dragging and refuted the stationary aether.
In addition, the Michelson–Morley null result was further substantiated
by the null results of other second-order experiments of different
kind, namely the Trouton–Noble experiment (1903) and the experiments of Rayleigh and Brace (1902–1904). These problems and their solution led to the development of the Lorentz transformation and special relativity.
After the "failed" experiment Michelson and Morley ceased their
aether drift measurements and started to use their newly developed
technique to establish the wavelength of light as a standard of length.
Light path analysis and consequences
Observer resting in the aether
The beam travel time in the longitudinal direction can be derived as follows: Light is sent from the source and propagates with the speed of light in the aether. It passes through the half-silvered mirror at the origin at . The reflecting mirror is at that moment at distance (the length of the interferometer arm) and is moving with velocity . The beam hits the mirror at time and thus travels the distance . At this time, the mirror has traveled the distance . Thus and consequently the travel time . The same consideration applies to the backward journey, with the sign of reversed, resulting in and . The total travel time is:
Michelson obtained this expression correctly in 1881, however, in transverse direction he obtained the incorrect expression
because he overlooked the increased path length in the rest frame of the aether. This was corrected by Alfred Potier (1882) and Lorentz (1886). The derivation in the transverse direction can be given as follows (analogous to the derivation of time dilation using a light clock): The beam is propagating at the speed of light and hits the mirror at time , traveling the distance . At the same time, the mirror has traveled the distance in the x direction. So in order to hit the mirror, the travel path of the beam is in the y direction (assuming equal-length arms) and in the x
direction. This inclined travel path follows from the transformation
from the interferometer rest frame to the aether rest frame. Therefore,
the Pythagorean theorem gives the actual beam travel distance of . Thus and consequently the travel time , which is the same for the backward journey. The total travel time is:
The time difference between Tℓ and Tt before rotation is given by[A 16]
By multiplying with c, the corresponding length difference before rotation is
and after rotation
Dividing by the wavelength λ, the fringe shift n is found:
Since L ≈ 11 meters and λ≈500 nanometers, the expected fringe shift was n ≈ 0.44.
So the result would be a delay in one of the light beams that could be
detected when the beams were recombined through interference. Any slight
change in the spent time would then be observed as a shift in the
positions of the interference fringes. The negative result led Michelson
to the conclusion that there is no measurable aether drift.
Observer comoving with the interferometer
If
the same situation is described from the view of an observer co-moving
with the interferometer, then the effect of aether wind is similar to
the effect experienced by a swimmer, who tries to move with velocity against a river flowing with velocity .
In the longitudinal direction the swimmer first moves upstream, so his velocity is diminished due to the river flow to . On his way back moving downstream, his velocity is increased to . This gives the beam travel times and as mentioned above.
In the transverse direction, the swimmer has to compensate for
the river flow by moving at a certain angle against the flow direction,
in order to sustain his exact transverse direction of motion and to
reach the other side of the river at the correct location. This
diminishes his speed to , and gives the beam travel time as mentioned above.
Mirror reflection
The
classical analysis predicted a relative phase shift between the
longitudinal and transverse beams which in Michelson and Morley's
apparatus should have been readily measurable. What is not often
appreciated (since there was no means of measuring it), is that motion
through the hypothetical aether should also have caused the two beams to
diverge as they emerged from the interferometer by about 10−8 radians.
For an apparatus in motion, the classical analysis requires that
the beam-splitting mirror be slightly offset from an exact 45° if the
longitudinal and transverse beams are to emerge from the apparatus
exactly superimposed. In the relativistic analysis, Lorentz-contraction
of the beam splitter in the direction of motion causes it to become more
perpendicular by precisely the amount necessary to compensate for the
angle discrepancy of the two beams.
Length contraction and Lorentz transformation
A first step to explaining the Michelson and Morley experiment's null result was found in the FitzGerald–Lorentz contraction hypothesis, now simply called length contraction or Lorentz contraction, first proposed by George FitzGerald (1889) and Hendrik Lorentz (1892). According to this law all objects physically contract by along the line of motion (originally thought to be relative to the aether), being the Lorentz factor. This hypothesis was partly motivated by Oliver Heaviside's
discovery in 1888 that electrostatic fields are contracting in the line
of motion. But since there was no reason at that time to assume that
binding forces in matter are of electric origin, length contraction of
matter in motion with respect to the aether was considered an Ad hoc hypothesis.
If length contraction of is inserted into the above formula for , then the light propagation time in the longitudinal direction becomes equal to that in the transverse direction:
However, length contraction is only a special case of the more
general relation, according to which the transverse length is larger
than the longitudinal length by the ratio . This can be achieved in many ways. If is the moving longitudinal length and the moving transverse length, being the rest lengths, then it is given:
can be arbitrarily chosen, so there are infinitely many combinations to
explain the Michelson–Morley null result. For instance, if the relativistic value of length contraction of occurs, but if then no length contraction but an elongation of occurs. This hypothesis was later extended by Joseph Larmor (1897), Lorentz (1904) and Henri Poincaré (1905), who developed the complete Lorentz transformation including time dilation in order to explain the Trouton–Noble experiment, the Experiments of Rayleigh and Brace, and Kaufmann's experiments. It has the form
It remained to define the value of , which was shown by Lorentz (1904) to be unity. In general, Poincaré (1905) demonstrated that only allows this transformation to form a group, so it is the only choice compatible with the principle of relativity, i.e.,
making the stationary aether undetectable. Given this, length
contraction and time dilation obtain their exact relativistic values.
Special relativity
Albert Einstein formulated the theory of special relativity
by 1905, deriving the Lorentz transformation and thus length
contraction and time dilation from the relativity postulate and the
constancy of the speed of light, thus removing the ad hoc character from the contraction hypothesis. Einstein emphasized the kinematic
foundation of the theory and the modification of the notion of space
and time, with the stationary aether no longer playing any role in his
theory. He also pointed out the group character of the transformation.
Einstein was motivated by Maxwell's theory of electromagnetism (in the form as it was given by Lorentz in 1895) and the lack of evidence for the luminiferous aether.
This allows a more elegant and intuitive explanation of the
Michelson–Morley null result. In a comoving frame the null result is
self-evident, since the apparatus can be considered as at rest in
accordance with the relativity principle, thus the beam travel times are
the same. In a frame relative to which the apparatus is moving, the
same reasoning applies as described above in "Length contraction and
Lorentz transformation", except the word "aether" has to be replaced by
"non-comoving inertial frame". Einstein wrote in 1916:
Although the estimated difference between these two times is exceedingly small, Michelson and Morley performed an experiment involving interference in which this difference should have been clearly detectable. But the experiment gave a negative result — a fact very perplexing to physicists. Lorentz and FitzGerald rescued the theory from this difficulty by assuming that the motion of the body relative to the æther produces a contraction of the body in the direction of motion, the amount of contraction being just sufficient to compensate for the difference in time mentioned above. Comparison with the discussion in Section 11 shows that also from the standpoint of the theory of relativity this solution of the difficulty was the right one. But on the basis of the theory of relativity the method of interpretation is incomparably more satisfactory. According to this theory there is no such thing as a "specially favoured" (unique) co-ordinate system to occasion the introduction of the æther-idea, and hence there can be no æther-drift, nor any experiment with which to demonstrate it. Here the contraction of moving bodies follows from the two fundamental principles of the theory, without the introduction of particular hypotheses; and as the prime factor involved in this contraction we find, not the motion in itself, to which we cannot attach any meaning, but the motion with respect to the body of reference chosen in the particular case in point. Thus for a co-ordinate system moving with the earth the mirror system of Michelson and Morley is not shortened, but it is shortened for a co-ordinate system which is at rest relatively to the sun.
— Albert Einstein, 1916
The extent to which the null result of the Michelson–Morley
experiment influenced Einstein is disputed. Alluding to some statements
of Einstein, many historians argue that it played no significant role in
his path to special relativity, while other statements of Einstein probably suggest that he was influenced by it.
In any case, the null result of the Michelson–Morley experiment helped
the notion of the constancy of the speed of light gain widespread and
rapid acceptance.
It was later shown by Howard Percy Robertson (1949) and others,
that it is possible to derive the Lorentz transformation entirely from
the combination of three experiments. First, the Michelson–Morley
experiment showed that the speed of light is independent of the orientation
of the apparatus, establishing the relationship between longitudinal
(β) and transverse (δ) lengths. Then in 1932, Roy Kennedy and Edward
Thorndike modified the Michelson–Morley experiment by making the path
lengths of the split beam unequal, with one arm being very short. The Kennedy–Thorndike experiment
took place for many months as the Earth moved around the sun. Their
negative result showed that the speed of light is independent of the velocity
of the apparatus in different inertial frames. In addition it
established that besides length changes, corresponding time changes must
also occur, i.e., it established the relationship between longitudinal
lengths (β) and time changes (α). So both experiments do not provide the
individual values of these quantities. This uncertainty corresponds to
the undefined factor as described above. It was clear due to theoretical reasons (the group character
of the Lorentz transformation as required by the relativity principle)
that the individual values of length contraction and time dilation must
assume their exact relativistic form. But a direct measurement of one of
these quantities was still desirable to confirm the theoretical
results. This was achieved by the Ives–Stilwell experiment
(1938), measuring α in accordance with time dilation. Combining this
value for α with the Kennedy–Thorndike null result shows that β must assume the value of relativistic length contraction. Combining β with the Michelson–Morley null result shows that δ must be zero. Therefore, the Lorentz transformation with is an unavoidable consequence of the combination of these three experiments.
Special relativity is generally considered the solution to all negative aether drift (or isotropy
of the speed of light) measurements, including the Michelson–Morley
null result. Many high precision measurements have been conducted as
tests of special relativity and modern searches for Lorentz violation in the photon, electron, nucleon, or neutrino sector, all of them confirming relativity.
Incorrect alternatives
As
mentioned above, Michelson initially believed that his experiment would
confirm Stokes' theory, according to which the aether was fully dragged
in the vicinity of the earth. However, complete aether drag contradicts the observed aberration of light
and was contradicted by other experiments as well. In addition, Lorentz
showed in 1886 that Stokes's attempt to explain aberration is
contradictory.
Furthermore, the assumption that the aether is not carried in the vicinity, but only within matter, was very problematic as shown by the Hammar experiment
(1935). Hammar directed one leg of his interferometer through a heavy
metal pipe plugged with lead. If aether were dragged by mass, it was
theorized that the mass of the sealed metal pipe would have been enough
to cause a visible effect. Once again, no effect was seen, so
aether-drag theories are considered to be disproven.
Walther Ritz's emission theory
(or ballistic theory) was also consistent with the results of the
experiment, not requiring aether. The theory postulates that light has
always the same velocity in respect to the source. However de Sitter
noted that emitter theory predicted several optical effects that were
not seen in observations of binary stars in which the light from the two
stars could be measured in a spectrometer.
If emission theory were correct, the light from the stars should
experience unusual fringe shifting due to the velocity of the stars
being added to the speed of the light, but no such effect could be seen.
It was later shown by J. G. Fox that the original de Sitter experiments were flawed due to extinction, but in 1977 Brecher observed X-rays from binary star systems with similar null results. Also terrestrial tests using particle accelerators have been made that were inconsistent with source dependence of the speed of light. In addition, Emission theory might fail the Ives–Stilwell experiment, but Fox questioned that as well.
Subsequent experiments
Although Michelson and Morley went on to different experiments after
their first publication in 1887, both remained active in the field.
Other versions of the experiment were carried out with increasing
sophistication. Morley was not convinced of his own results, and went on to conduct additional experiments with Dayton Miller from 1902 to 1904. Again, the result was negative within the margins of error.
Miller worked on increasingly larger interferometers, culminating
in one with a 32-meter (105 ft) (effective) arm length that he tried at
various sites, including on top of a mountain at the Mount Wilson Observatory.
To avoid the possibility of the aether wind being blocked by solid
walls, his mountaintop observations used a special shed with thin walls,
mainly of canvas. From noisy, irregular data, he consistently extracted
a small positive signal that varied with each rotation of the device,
with the sidereal day,
and on a yearly basis. His measurements in the 1920s amounted to
approximately 10 km/s (6.2 mi/s) instead of the nearly 30 km/s
(18.6 mi/s) expected from the Earth's orbital motion alone. He remained
convinced this was due to partial entrainment or aether dragging,
though he did not attempt a detailed explanation. He ignored critiques
demonstrating the inconsistency of his results and the refutation by the
Hammar experiment. Miller's findings were considered important at the time, and were discussed by Michelson, Lorentz and others at a meeting reported in 1928.
There was general agreement that more experimentation was needed to
check Miller's results. Miller later built a non-magnetic device to
eliminate magnetostriction, while Michelson built one of non-expanding Invar
to eliminate any remaining thermal effects. Other experimenters from
around the world increased accuracy, eliminated possible side effects,
or both. So far, no one has been able to replicate Miller's results, and
modern experimental accuracies have ruled them out.
Roberts (2006) has pointed out that the primitive data reduction
techniques used by Miller and other early experimenters, including
Michelson and Morley, were capable of creating apparent periodic
signals even when none existed in the actual data. After reanalyzing
Miller's original data using modern techniques of quantitative error
analysis, Roberts found Miller's apparent signals to be statistically
insignificant.
Using a special optical arrangement involving a 1/20 wave step in
one mirror, Roy J. Kennedy (1926) and K.K. Illingworth (1927) (Fig. 8)
converted the task of detecting fringe shifts from the relatively
insensitive one of estimating their lateral displacements to the
considerably more sensitive task of adjusting the light intensity on
both sides of a sharp boundary for equal luminance.
If they observed unequal illumination on either side of the step, such
as in Fig. 8e, they would add or remove calibrated weights from the
interferometer until both sides of the step were once again evenly
illuminated, as in Fig. 8d. The number of weights added or removed
provided a measure of the fringe shift. Different observers could detect
changes as little as 1/300 to 1/1500 of a fringe. Kennedy also carried
out an experiment at Mount Wilson, finding only about 1/10 the drift
measured by Miller and no seasonal effects.
In 1930, Georg Joos
conducted an experiment using an automated interferometer with
21-meter-long (69 ft) arms forged from pressed quartz having very low
thermal coefficient of expansion, that took continuous photographic
strip recordings of the fringes through dozens of revolutions of the
apparatus. Displacements of 1/1000 of a fringe could be measured on the
photographic plates. No periodic fringe displacements were found,
placing an upper limit to the aether wind of 1.5 km/s (0.93 mi/s).
Recent experiments
Optical tests
Optical tests of the isotropy of the speed of light became commonplace. New technologies, including the use of lasers and masers,
have significantly improved measurement precision. (In the following
table, only Essen (1955), Jaseja (1964), and Shamir/Fox (1969) are
experiments of Michelson–Morley type, i.e., comparing two perpendicular beams. The other optical experiments employed different methods.)
Author | Year | Description | Upper bounds |
---|---|---|---|
Louis Essen | 1955 | The frequency of a rotating microwave cavity resonator is compared with that of a quartz clock | ~3 km/s |
Cedarholm et al. | 1958 | Two ammonia masers were mounted on a rotating table, and their beams were directed in opposite directions. | ~30 m/s |
Mössbauer rotor experiments | 1960–68 | In a series of experiments by different researchers, the frequencies of gamma rays were observed using the Mössbauer effect. | ~2.0 cm/s |
Jaseja et al. | 1964 | The frequencies of two He–Ne masers, mounted on a rotating table, were compared. Unlike Cedarholm et al., the masers were placed perpendicular to each other. | ~30 m/s |
Shamir and Fox | 1969 | Both arms of the interferometer were contained in a transparent solid (plexiglas). The light source was a Helium–neon laser. | ~7 km/s |
Trimmer et al. | 1973 | They searched for anisotropies of the speed of light behaving as the first and third of the Legendre polynomials. They used a triangle interferometer, with one portion of the path in glass. (In comparison, the Michelson–Morley type experiments test the second Legendre polynomial) | ~2.5 cm/s |
Recent optical resonator experiments
Over
the last several years, there has been a resurgence in interest in
performing precise Michelson–Morley type experiments using lasers,
masers, cryogenic optical resonators,
etc. This is in large part due to predictions of quantum gravity that
suggest that special relativity may be violated at scales accessible to
experimental study. The first of these highly accurate experiments was
conducted by Brillet & Hall (1979), in which they analyzed a laser
frequency stabilized to a resonance of a rotating optical Fabry–Pérot cavity. They set a limit on the anisotropy of the speed of light resulting from the Earth's motions of Δc/c ≈ 10−15, where Δc is the difference between the speed of light in the x- and y-directions.
As of 2009, optical and microwave resonator experiments have improved this limit to Δc/c ≈ 10−17. In some of them, the devices were rotated or remained stationary, and some were combined with the Kennedy–Thorndike experiment. In particular, Earth's direction and velocity (ca. 368 km/s (229 mi/s)) relative to the CMB rest frame are ordinarily used as references in these searches for anisotropies.
Author | Year | Description | Δc/c |
---|---|---|---|
Wolf et al. | 2003 | The frequency of a stationary cryogenic microwave oscillator, consisting of sapphire crystal operating in a whispering gallery mode, is compared to a hydrogen maser whose frequency was compared to caesium and rubidium atomic fountain clocks. Changes during Earth's rotation have been searched for. Data between 2001–2002 was analyzed. | |
Müller et al. | 2003 | Two optical resonators constructed from crystalline sapphire, controlling the frequencies of two Nd:YAG lasers, are set at right angles within a helium cryostat. A frequency comparator measures the beat frequency of the combined outputs of the two resonators. | |
Wolf et al. | 2004 | See Wolf et al. (2003). An active temperature control was implemented. Data between 2002–2003 was analyzed. | |
Wolf et al. | 2004 | See Wolf et al. (2003). Data between 2002–2004 was analyzed. | |
Antonini et al. | 2005 | Similar to Müller et al. (2003), though the apparatus itself was set into rotation. Data between 2002–2004 was analyzed. | |
Stanwix et al. | 2005 | Similar to Wolf et al. (2003). The frequency of two cryogenic oscillators was compared. In addition, the apparatus was set into rotation. Data between 2004–2005 was analyzed. | |
Herrmann et al. | 2005 | Similar to Müller et al. (2003). The frequencies of two optical Fabry–Pérot resonators cavities are compared – one cavity was continuously rotating while the other one was stationary oriented north–south. Data between 2004–2005 was analyzed. | |
Stanwix et al. | 2006 | See Stanwix et al. (2005). Data between 2004–2006 was analyzed. | |
Müller et al. | 2007 | See Herrmann et al. (2005) and Stanwix et al. (2006). Data of both groups collected between 2004–2006 are combined and further analyzed. Since the experiments are located at difference continents, at Berlin and Perth respectively, the effects of both the rotation of the devices themselves and the rotation of Earth could be studied. | |
Eisele et al. | 2009 | The frequencies of a pair of orthogonal oriented optical standing wave cavities are compared. The cavities were interrogated by a Nd:YAG laser. Data between 2007–2008 was analyzed. | |
Herrmann et al. | 2009 | Similar to Herrmann et al. (2005). The frequencies of a pair of rotating, orthogonal optical Fabry–Pérot resonators are compared. The frequencies of two Nd:YAG lasers are stabilized to resonances of these resonators. |
Other tests of Lorentz invariance
Examples of other experiments not based on the Michelson–Morley
principle, i.e., non-optical isotropy tests achieving an even higher
level of precision, are Clock comparison or Hughes–Drever experiments. In Drever's 1961 experiment, 7Li nuclei in the ground state, which has total angular momentum J = 3/2,
were split into four equally spaced levels by a magnetic field. Each
transition between a pair of adjacent levels should emit a photon of
equal frequency, resulting in a single, sharp spectral line. However,
since the nuclear wave functions for different MJ have
different orientations in space relative to the magnetic field, any
orientation dependence, whether from an aether wind or from a dependence
on the large-scale distribution of mass in space,
would perturb the energy spacings between the four levels, resulting in
an anomalous broadening or splitting of the line. No such broadening
was observed. Modern repeats of this kind of experiment have provided
some of the most accurate confirmations of the principle of Lorentz invariance.