[Physics FAQ] - [Copyright]
By Tom Roberts,
2000.
Original by Siegmar Schleif and others, 1998.
What is the experimental basis of Special Relativity?
Index
1.
Introduction |
|
|
Domain
of Applicability Test
Theories of SR |
2.
Early experiments (Pre-1905) |
|
|
|
|
Roentgen, Eichenwald, Wilson, Rayleigh, Arago, Fizeau, Hoek, Bradley,
Airy. |
3.
Tests of Einstein's Two Postulates |
|
|
|
3.1
Round-Trip Tests of Light Speed Isotropy |
|
|
|
Michelson and Morley, Kennedy and Thorndike, Modern
Laser/Maser Tests, Other. |
|
3,2
One-Way Tests of Light Speed Isotropy |
|
|
|
Cialdea, Krisher, Champeny, Turner & Hill. |
|
3.3
Tests of Light Speed from Moving Sources |
|
|
|
Cosmological Sources: DeSitter, Brecher; Terrestrial Sources:
Alvaeger, Sadeh, .... |
|
3.4
Measurements of the Speed of Light, and Other Limits on it |
|
|
|
NBS Measurements, 1983 Redefinition of the Meter, Limits on Variations
with Frequency, Limits on Photon Mass. |
|
3.5
Tests of the Principle of Relativity and Lorentz Invariance |
|
|
|
Trouton Noble, Other. |
|
3.6
Tests of the Isotropy of Space |
|
|
|
Hughes-Drever, Prestage, Lamoreaux, Chupp, Phillips, Brillet and
Hall. |
4.
Tests of Time Dilation and Transverse Doppler Effect |
|
|
|
|
Ives and Stilwell; Particle Lifetimes, Doppler Shift
Measurements. |
5.
Tests of the Twin Paradox |
|
|
|
|
Haefle and Keating, Vessot et al, Alley, Bailey et al., The Clock
Hypothesis. |
6.
Tests of Relativistic Kinematics |
|
|
|
|
Elastic Scattering, Limiting Velocity c, Relativistic Mass Variations,
Calorimetric Test of SR. |
7.
Other Experiments |
|
|
|
|
Fizeau, Sagnac, Michelson and Gale, g-2 Tests of SR, The Global
Positioning System (GPS), Lunar Laser Ranging, Cosmic Background Radiation
(CMBR), Constancy of Physical Constants, Other. |
8.
Experiments Which Apparently are NOT Consistent with SR/GR |
|
|
|
|
Experimenter's
Bias Publication
Bias |
9.
Acknowledgments |
|
|
1. Introduction
Physics is an experimental
science, and as such the experimental basis for any physical theory is extremely
important. The relationship between theory and experiments in modern
science is a multi-edged sword:
- It is required that the theory not be refuted by any undisputed experiment
within the theory's domain
of applicability.
- It is expected that the theory be confirmed by a number of experiments
that:
- cover a significant fraction of the
theory's domain
of applicability.
- examine a significant
fraction of the theory's predictions.
It is believed that Special Relativity (SR) meets all of these requirements
and expectations. There are literally hundreds of experiments that have
tested SR, with an enormous range and diversity, and the agreement between
theory and experiment is excellent. There is a lot of redundancy in these
experimental tests. There are also a lot of indirect tests of SR which are
not included here. This list of experiments is by no means complete!
Other than their sheer numbers, the most striking thing about these
experimental tests of SR is their remarkable breadth and diversity. An
important aspect of SR is its universality -- it applies to all known physical
phenomena and not just to the electromagnetic phenomena it was originally
invented to explain. In these experiments you will find tests using
electromagnetic and nuclear measurements (including both strong and weak
interactions); gravitational tests are the province of General Relativity, and
are not considered here, see Experimental
Tests of GR.
There are several useful surveys of the experimental basis of SR:
- Y.Z.Zhang, Special Relativity and its Experimental Foundations,
World Scientific (1997).
- G.Holton, "Resource Letter SRT-1 on Special Relativity Theory", Am. J.
Phys., 30 (1962), p462.
- D.I.Blotkhintsev, "Basis for Special Relativity Theory Provided by
Experiments in High Energy Physics", Sov. Phys. Uspekhi, 9 (1966),
p405.
- Newman et al. Phys. Rev. Lett. 40 no. 21 (1978), p1355.
Zhang's book is especially comprehensive.
Textbooks with good summaries of the experimental basis of relativity are:
- M.Born, Einstein's theory of Relativity.
- Bergmann, Introduction to the Theory of Relativity.
- Moller, The Theory of Relativity.
- M. von Laue, Die relativitätstheorie (in German).
Note, however, that SR is not perfect (in agreement with every experiment),
and there are some experiments that are in disagreement with its
predictions. See Experiments
Which Apparently are NOT Consistent with SR where some of these experiments
are referenced and discussed. It is clear that most, if not all, of these
experiments have difficulties that are unrelated to SR. Note also that few
if any standard references or textbooks even mention the possibility that some
experiments might be inconsistent with SR, and there are also aspects of publication
bias in the literature. That being said, as of this writing there are
no reproducible and generally-accepted experiments that are inconsistent with
SR, within its domain
of applicability.
Domain of Applicability
The domain of applicability of a physical theory is the set of physical
situations in which the theory is valid. For SR this is basically
measurements of distance, time, momentum, energy, etc. in inertial frames
(coordinates); calculus can be used to apply SR in accelerated systems, as can
the more advanced mathematics of differential geometry. A more technical
definition is that SR is valid only in flat Lorentz manifolds topologically
equivalent to R4. In particular, any experiment in which the
effects of gravitation are important is outside the domain of SR. Because
SR is the local limit of General Relativity it is possible to compute how large
an error is made when one applies SR to a situation that is approximately but
not exactly inertial, such as the common case of experimental apparatus
supported against gravity on the earth's surface. In many cases (e.g. most
optical and elementary-particle experiments on the rotating earth's surface)
these errors are vastly smaller than the experimental resolution, and SR can be
accurately applied.
Test Theories of SR
A test
theory of SR is a generalization of the Lorentz transforms of SR using
additional parameters. One can then analyze experiments using the test
theory (rather than SR itself) and fit the parameters of the test theory to the
experimental results. If the fitted parameter values differ significantly
from the values corresponding to SR, then the experiment is inconsistent with
SR. But more normally, such fits can show how well a given experiment
confirms or disagrees with SR, and what the experimental accuracy is for doing
so. This gives a general and tractable method of analysis which can be
common to multiple experiments.
Different test theories differ in their assumptions about what form the
transform equations could reasonably take. There are at present four test
theories of SR:
|
Robertson,Rev. of Mod. Phys. 21, p378 (1949). |
|
Edwards, Am. J. Phys. 31 (1963), p482. |
|
Mansouri and Sexl, Gen. Rel. Grav. 8 (1977), p497, p515,
p809. |
|
Zhang, Special Relativity and its Experimental
Foundations. |
Zhang discusses their
interrelationships and presents a unified test theory encompassing the other
three, but with a better and more interpretable parameterization. His
discussion implies that there will be no more test theories of SR that are not
reducible to one of the first three.
Robertson showed that one can unambiguously deduce the Lorentz transform of
SR to an accuracy of ~0.1% from the following three experiments: Michelson and
Morley, Kennedy and Thorndike, Ives and Stilwell. Zhang showed that modern
experiments determine the Lorentz transforms to within a few parts per
million.
These test theories can also be used to examine potential alternate theories
to SR -- such alternate theories predict particular values of the parameters of
the test theory, which can easily be compared to values determined by
experiments analyzed with the test theory. The existing experiments put
rather strong experimental constraints on any alternative theory.
In particular, Zhang showed that these experimental limits essentially require
that any theory based upon the existence of an ether be experimentally
indistinguishable from SR, and have an ether frame which is unobservable (the
only alternative is for a theory to "live in the error bars" of the experiments,
which is quite difficult given the high accuracies achieved by many of these
experiments).
2. Early Experiments (Pre-1905)
The Special Theory of Relativity (SR) is a theory invented in 1905 by
Einstein to explain several experimental results. Since then it has been
found to explain a wide range of experimental results. SR is NOT a
mathematical game or just a hypothesis. SR is a physical theory which has
been well tested many times.
When A. Einstein wrote his famous paper: "The Electrodynamics of Moving
Bodies" in 1905, he already had experimental support for his new theory:
".... Examples of this sort, together with the unsuccessful
attempts to discover any motion of the Earth relatively to the "light medium"
suggest that the phenomena of electrodynamics as well as of mechanics possess
no properties corresponding to the idea of absolute rest. They suggest
rather that, as has already been shown to the first order of small quantities,
the same laws of electrodynamics and optics will be valid for all frames of
reference for which the equations of mechanics hold good..."
What was the experimental support for this claim? There were several
experiments concerning the electrodynamics of moving bodies, which are not very
well known today, but Einstein knew these experiments:
W.C. Roentgen, Annalen der Physik 35 (1888), pg
264. |
|
|
Note that Roentgen describes in this paper an "unsuccessful"
experiment, where he tried to measure the velocity of the Earth through
the ether (a "primitive" version of the Trouton-Noble
experiment). |
A.Eichenwald, Annalen der Physik 11 (1903), pg 1
and. pg 241. |
|
|
Experiments concerning the so called Roentgen convection, with an
electric field (See Sommerfeld Vol. 3, Chapter
4). |
H. A. Wilson, Philosph. Transact. Roy. soc. London
204 (1904), pg 121. H. A. Wilson, M. Wilson, Philosph.
Transact. Roy. soc. London 89 (1913), pg 99. |
|
|
Experiments concerning the so called Roentgen convection, with a
magnetic field (See Sommerfeld Vol. 3, Chapter
4). |
Rayleigh Phil. Mag. (6) 4, pg 678 (1902). Brace Phil.
Mag. (6) 7, pg 317 (1904). |
|
|
Experiments concerning the effect of the motion of the Earth on double
refraction. |
Arago |
|
|
Examined the expected change in focus of a refracting telescope due to
earth's motion around the sun. This is first order in v/c if one
assumes light is fully dragged by the lens. The null result is
consistent with SR |
Fizeau |
|
|
Measured the speed of light in moving materials. The Fresnel
drag coefficient is solidly established by experiments, and is consistent
with SR to within experimental resolutions. |
Hoek |
|
|
Much more accurate version of the basic concept of Arago's experiment,
using a terrestrial source and a square (ring) interferometer with one
side in water and three in air. The null result is consistent with
Arago's result and with Fresnel's drag coefficient, and with
SR. |
Bradley |
|
|
Bradley (1727) discovered that the images of stars move in small
ellipses. This is explained as aberration due to the earth's motion
around the sun. This is inconsistent with a simple model of light as
waves in an aether which is dragged along by the earth; it is consistent
with SR. |
Airy |
|
|
Airy (1871) tested whether stellar aberration remained unchanged if
the telescope was filled with water. It did. |
3. Tests of Einstein's
two Postulates
- The laws by which the states of physical systems undergo change are not
affected, whether these changes of state be referred to the one or the other
of two systems of coordinates in uniform translatory motion.
- Any ray of light moves in the "stationary" system of coordinates with
determined velocity c, whether the ray be emitted by a stationary or by a
moving body.
-- Einstein, Ann. d. Physik 17 (1905); translated by
Perrett and Jeffery; reprinted in: Einstein, Lorentz, Weyl,
Minkowski, The Principle of Relativity, Dover
1952.
"Stationary" was defined in the first paragraph of this section:
Let us take a system of coordinates in which the equations of
Newtonian mechanics hold good. In order to render our presentation more
precise and to distinguish this system of coordinates verbally from others
which will be introduced hereafter, we call it the "stationary system".
--
Ibid.
It is clear that
the word "stationary" is used merely as a label, and implies no "absolute"
aspects at all.
3.1 Round-Trip Tests of Light-Speed
Isotropy
The speed of light is said to be isotropic if it has the same value when
measured in any/every direction.
The Michelson-Morley Experiment (the MMX)
The
Michelson-Morley experiment (MMX) was intended to measure the velocity of the
earth relative to the "lumeniferous aether" which was at the time presumed to
carry electromagnetic phenomena. The failure of it and the other early
experiments to actually observe the earth's motion through the aether became
significant in promoting the acceptance of Einstein's theory of Special
Relativity, as it was appreciated from early on that Einstein's approach (via
symmetry) was more elegant and parsimonious of assumptions than were other
approaches (e.g. those of Maxwell, Hertz, Stokes, Fresnel, Lorentz, Ritz, and
Abraham).
The following table comes from R.S. Shankland et al, Rev. Mod. Phys.
27 no. 2, pp167-178 (1955), which includes references to each
experiment (resolution and the limit on Vaether are from the
original sources). The expected fringe shift is what would be expected
for a rigid ether at rest with respect to the sun and earth's orbital velocity
(~30 km/s).
Name |
Year |
Arm length (meters) |
Fringe shift expected |
Fringe shift measured |
Experimental Resolution |
Upper Limit on Vaether |
Michelson |
1881 |
1.2 |
0.04 |
0.02 |
|
|
Michelson + Morley |
1887 |
11.0 |
0.4 |
< 0.01 |
|
8 km/s |
Morley + Morley |
1902-04 |
32.2 |
1.13 |
0.015 |
|
|
Miller |
1921 |
32.0 |
1.12 |
0.08 |
|
|
Miller |
1923-24 |
32.0 |
1.12 |
0.03 |
|
|
Miller (Sunlight) |
1924 |
32.0 |
1.12 |
0.014 |
|
|
Tomascheck (Starlight) |
1924 |
8.6 |
0.3 |
0.02 |
|
|
Miller |
1925-26 |
32.0 |
1.12 |
0.088 |
|
|
Kennedy (Mt Wilson) |
1926 |
2.0 |
0.07 |
0.002 |
|
|
Illingworth |
1927 |
2.0 |
0.07 |
0.0002 |
0.0006 |
1 km/s |
Piccard + Stahel(Mt Rigi) |
1927 |
2.8 |
0.13 |
0.006 |
|
|
Michelson et al. |
1929 |
25.9 |
0.9 |
0.01 |
|
|
Joos |
1930 |
21.0 |
0.75 |
0.002 |
|
|
A.A. Michelson and E.W. Morley, "On the Relative Motion
of the Earth and the Luminiferous Ether", Am. J.Sci. (3rd series)
34 333-345 (1887). |
|
|
This is the classic paper describing this famous
experiment. |
Shankland, "Michelson-Morley Experiment", American
Journal of Physics 1964, pg 16. |
|
|
This is a general review article. |
G. Joos, Ann. Phys. 7 385 (1930). |
|
|
An excellent repetition of the MMX, in vacuum. |
K.K.Illingworth, Phys. Rev. 30 (1927),
p692. |
|
|
Used a clever technique with a tiny step in one mirror to obtain
significantly improved resolution. |
Shamir and Fox, N. Cim. 62B no. 2 (1969),
p258. |
|
|
A repetition of the MMX with the optical paths in perspex (n = 1.49),
and a laser-based optics sensitive to ~0.00003 fringe. They report a
null result with an upper limit on Vaether of 6.64
km/s. |
See also: Brillet
and Hall.
The Kennedy-Thorndike Experiment
R.J. Kennedy and E.M. Thorndike, "Experimental
Establishment of the Relativity of Time", Phys. Rev. 42 400-418
(1932). |
|
|
This uses an interferometer similar to Michelson's, except that its
arms are of different length, and are not at right angles to each
other. They used a spectacular technique to keep the apparatus
temperature constant to 0.001° C, which gave them sufficient stability to
permit observations during several seasons. They also used
photographs of their fringes (rather than observing them in real time as
in most other interferometer experiments). Their apparatus was fixed
to the earth and could only rotate with it. Their null result is
consistent with SR. |
See also: Hils
and Hall.
Modern Laser / Maser Tests of Light-Speed Isotropy
Cedarholm, Havens, and Townes, Phys. Rev. Lett. 1
(1958), p 342. |
|
|
They used two ammonia-beam masers back-to-back to put a limit of 30
m/s on any "ether drift". |
T.S. Jaseja, A. Javan, J. Murray and C.H. Townes, "Test
of Special Relativity or of the Isotropy of Space by Use of Infrared
Masers", Phys. Rev. 133A 1221-1225 (1964) |
|
|
They mounted two He-Ne microwave masers perpendicularly on a
shock-mounted table and observed the beat frequency between them as the
table was rotated. They put a limit of 30 m/s on the
anisotropy. |
A. Brillet and J.L. Hall, "Improved
Laser Test of the Isotropy of Space", Phys. Rev. Lett. 42 549-552
(1979). |
|
|
This is one of the most accurate limits on any anisotropy in the
round-trip speed of light in a laboratory. They measured the
beat-frequency between a single-mode laser on a rotating table and a
single-mode laser fixed to the earth to put a limit on such an anisotropy
of 3 parts in 1015. Due to the
construction of their rotating laser, this can also be interpreted as a
limit on any anisotropy of space. This is a round-trip experiment
because of their use of a Fabry-Perot etalon to determine the frequency of
the rotating laser. Note that their limit on the round-trip
anisotropy corresponds to a round-trip speed of less than 0.000001 m/s
(!); in terms of the more usual one-way anisotropy it is 30 m/s.
Their residual 17 Hz signal (out of ~1015 Hz) was
interpreted as due to the rotation of the earth in: Aspden, Phys. Lett.
8 no. 9 (1981), pg 411. The experimenters themselves
interpreted it as "unknown", and noted it was fixed w.r.t. their
laboratory and therefore could not be of cosmic
origin. |
Hils and Hall, Phys. Rev. Lett.
64 (1990), p 1697. |
|
|
This is similar to Brillet
and Hall (above), but the lasers are fixed to the earth for better
stability. No variations were found at the level of
2*10-13. As they made observations over a year, this is
not merely a limit on anisotropy, but also a limit on variations in
different inertial frames. Brillet and Hall corresponds roughly to
the Michelson-Morley experiment (no variations of the round-trip speed of
light in different directions, with a time-scale of minutes or seconds);
Hils and Hall corresponds roughly to the Kennedy-Thorndike experiment (no
variations of the round-trip speed of light in different directions or for
the different inertial frames occupied by the earth during a year or
so). |
Other Experiments
Trimmer et al., Phys. Rev. D8, p3321 (1973); Phys.
Rev. D9 p2489 (1974). |
|
|
A triangle interferometer with one leg in glass. They set an
upper limit on the anisotropy of 0.025 m/s. This is about
one-millionth of the earth's orbital velocity and about 1/10,000 of its
rotational velocity. |
Riis et al., Phys. Rev. Lett. 60, p81
(1988). |
|
|
This novel experiment uses a two-photon transition in a Neon atomic
beam to set an upper limit on any anisotropy of 0.3
m/s. |
Silvertooth, J. O. S. A. 62 (1972), p1330. |
|
|
This innovative experiment uses an interferometer with
frequency-doubling crystals, so the fundamental's fringes are due to
signals going all the way around, but the doubled-frequency fringes are
due to signals going only half the way around (converging from opposite
directions onto the detector). Its null result is consistent with
SR. |
3.2 One-Way Tests of Light-Speed
Isotropy
Note that while these experiments clearly use a one-way light path
and find isotropy, they are inherently unable to rule out a large class of
theories in which the one-way speed of light is anisotropic. These
theories share the property that the round-trip speed of light is isotropic in
any inertial frame, but the one-way speed is isotropic only in an ether
frame. In all of these theories the effects of slow clock transport
exactly offset the effects of the anisotropic one-way speed of light (in any
inertial frame), and all are experimentally indistinguishable from SR. All
of these theories predict null results for these experiments. See Test
Theories above, especially Zhang (in which these theories are called
"Edwards frames").
Cialdea, Lett. Nuovo Cimento 4
(1972), p821. |
|
|
Uses two multi-mode lasers mounted on a rotating table to look for
variations in their interference pattern as the table is rotated.
Places an upper limit on any one-way anisotropy of 0.9
m/s. |
Krisher et al., Phys. Rev. D,
42, No. 2, pp. 731-734, (1990). |
|
|
Uses two hydrogen masers fixed to the earth and separated by a 21 km
fiber-optic link to look for variations in the phase between them.
They put an upper limit on the one-way linear anisotropy of 100
m/s. |
Champeny et al, Phys. Lett. 7 (1963), p241.
Champeney, Isaak and Khan, Proc. Physical Soc. 85, p583
(1965). Isaak et al, Phys. Bull. 21 (1970), p255. |
|
|
Uses a rotating Moessbauer absorber and fixed detector to place an
upper limit on any one-way anisotropy of 3 m/s. |
Turner and Hill, Phys. Rev. 134 (1964),
B252. |
|
|
Uses a rotating source and fixed Moessbauer detector to place an upper
limit on any one-way anisotropy of 10 m/s. |
Gagnon, Torr, Kolen, and Chang, Phys. Rev. A38 no.
4 (1988), p1767. |
|
|
A guided-wave test of isotropy. Their null result is consistent
with SR. |
3.3 Tests of Light Speed from Moving
Sources
If the light emitted from a source moving with velocity v toward the
observer has a speed c+kv in the observer's frame, then these experiments place
a limit on k.
Experiments Using Cosmological Sources
Comstock, Phys. Rev. 10 (1910), p267.
DeSitter, Koninklijke Akademie van Wetenschappen, vol 15,
part 2, pg 1297-1298 (1913); DeSitter, Koninklijke Akademie van
Wetenschappen, vol 16, part 1, pg 395--396 (1913).
Zurhellen, Astr. Nachr. 198 (1914), p1. |
|
|
Observations of binary stars. k <
10-6. |
K. Brecher, "Is the Speed of Light Independent of the
Velocity of the Source?", Phys. Rev. Lett. 39 1051-1054, 1236(E)
(1977). |
|
|
Uses observations of binary pulsars to put a limit on the
source-velocity dependence of the speed of light. k <
2*10-9. |
Heckmann, Ann. D'. Astrophys. 23 (1960),
p410. |
|
|
Differential aberration, galaxies versus stars. |
These experiments are all subject to criticism due to extinction effects in
the interstellar gas; see for instance J.G. Fox Am. J. Phys. 30, p297
(1962); AJP 33, 1 (1964). The standard reference for optical
extinction is Born and Wolf, Principles of Optics.
Experiments Using Terrestrial Sources
Beckmann and Mandies, Radio. Sci. 69D (1965),
p623. |
|
|
A moving mirror experiment. |
Alvaeger F.J.M. Farley, J. Kjellman and I Wallin, Physics
Letters 12, 260 (1964). |
|
|
Measured the speed of gamma rays from the decay of fast pi0 (~0.99975
c) to be c with a resolution of 400 parts per million. |
Sadeh, Phys. Rev. Lett. 10 no. 7 (1963),
p271. |
|
|
Measured the speed of the gammas emitted from e+e- annihilation (with
center-of-mass v/c ~ 0.5) to be c within 10%. |
Babcock and Bergmann, Journal Opt. Soc. Amer. Vol.
54, pg 147 (1964). |
|
|
- |
Filipas and Fox, Phys. Rev. 135 no. 4B (1964), p
B1071. |
|
|
Measured the speed of gamma rays from the decay of fast pi0 (~0.2 c)
in an experiment specifically designed to avoid extinction effects.
Their results are in complete disagreement with the assumption c + v, and
are consistent with SR. |
Because of the high energies of the gammas in Alvaeger, extinction is not a
problem for it; Filipas and Fox specifically designed their experiment to avoid
extinction.
3.4 Measurements of the
Speed of Light, and Other Limits on it
In 1983 the international standard for the meter was redefined in terms of
the definition of the second and a defined value for the speed of
light. The defined value was chosen to be as consistent as possible with
the earlier metrological definitions of the meter and the second. Since
then it is not possible to measure the speed of light using the current
metrological standards, but one can still measure any anisotropy in its speed,
or use an earlier definition of the meter if necessary.
Mulligan, Am. J. Phys. 44 no. 10 (1976),
p960. |
|
|
A report on measurements by the NBS. |
Rowley et al, Opt. and Quantum Elect. 8 (1976),
p1. |
|
|
A review article on the set of precision frequency and wavelength
measurements that became the basis for the 1973 value of
c. |
Woods et al, Appl. Optics 17 (1978), p1048;
Rowley, Opt. Comm. 34 (1980), p429. Baird and Whitford,
Opt. Comm. 31 (1979), p363, p367. |
|
|
Measured c = 299792458.8 +- 0.2 meter/s, with 1.2 meter uncertainty
due to realization of the Kr meter standard used. The fact that the
Kr standard for the meter became the limit on accuracy was a major reason
for the 1983 redefinition of the meter in terms of the definition of c and
the definition of the second. |
Goldman, J. O. S. A. 70 (1980), 1640. |
|
|
Discussion of three proposals for a new definition of the meter
(pre-1983). |
Jennings et al, J. Res. N.B.S. 92 (1982),
p11. |
|
|
Review of methods to relate c to the meter, and results for further
measurements checking the 1973 determination of c leading to the 1983
adoption of the new meter standard in terms of the definition of c and the
definition of the second. |
Giacomo, "The New Definition of the Meter", Am. J. Phys.
52 no. 7 (1984), p607. |
|
|
An overview of past definitions of the meter with emphasis on the
guidelines that governed the choice of the new definition in 1983 in terms
of the definition of the second and the definition of the speed of
light. |
Petley, "New Definition of the Metre", Nature 303
(1983), p373. |
|
|
A review article discussing the reasons for the re-definition of the
meter in 1983 in terms of the definition of the second and the definition
of the speed of light. |
Bates, Am. J. Phys. 56 (1986), p682.
Bates, Am. J. Phys. 51 (1983), p1003. |
|
|
A summary of measurements of c. The second paper describes
measuring c by measuring frequency and wavelength and describes a
college-level lab experiment. |
Limits on Velocity Variations with Frequency
Essen and Froome, The Velocity of Light and Radio
Waves (1969). |
|
|
For frequencies between 108 and 1015 Hz the
speed of light is constant within 1 part in
105. |
Brown et al, Phys. Rev. Lett. 30
no. 16 (1973), p763. |
|
|
For visible light and 7 GeV gammas the speed of light differs by at
most 6 parts in 106. The speed of 11 GeV electrons is
within 3 parts in 106 of the speed of visible
light. |
Florman, J. Res. N.B.S. 54 (1955), p355. |
|
|
- |
Schaefer, Phys. Rev. Lett. 82 no. 25 (1999),
p4964. |
|
|
For photons of 30 keV and 200keV the speed of light is the same within
a few parts in 1021. |
Limits on the Photon Mass
Goldhaber and Nieto, "New Geomagnetic Limit on the Mass
of the Photon", Phys. Rev. Lett. 21 no. 8 (1968), p567. |
|
|
A limit of 2.3*10-15 eV. |
Goldhaber and Nieto, "Terrestrial and Extraterrestrial
limits on the Photon Mass", Rev. Mod. Phys. 43 no. 3 (1971),
p277. |
|
|
A review article discussion about various experimental
limits. |
Davis et al, "Limit on the Photon Mass Deduced from
Pioneer-10 Observations of Jupiter's magnetic Fields", Phys. Rev. Lett.
35 no. 21 (1975), p1402. |
|
|
A limit of 6*10-16 eV. |
Lakes, "Experimental limits on the Photon Mass and Cosmic
Magnetic Vector Potential", Phys. Rev. Lett. 80 no. 9 (1998),
p1826. |
|
|
An experimental approach using a toroid Cavendish
balance. |
See also the Particle Data Group's summary
on "Gauge and Higgs Bosons".
3.5 Tests of the Principle of Relativity and
Lorentz Invariance
Einstein's first postulate, the principle of Relativity
(PoR), essentially states that the laws of physics do not vary for different
inertial frames. Most if not all of the tests of his second postulate (the
isotropy experiments above) could also be placed in this section, as could those
in the following section.
The Trouton-Noble Experiment
Trouton and Noble, Phil. Trans. 202 (1903),
p165. |
|
|
This classic experiment looked for a torque induced on a charged
capacitor due to its motion through the ether. Its null result is
consistent with SR. |
Chase, Phys, Rev, 28, pg 378 (1926). |
|
|
Set an upper limit on ether drift of 4 km/s. |
Tomaschek, Ann. d Phys. 78 (1926), p743; 80
(1926), p509. |
|
|
- |
Other Experiments
Coleman and Glashow, "Cosmic ray and Neutrino Tests of
Special Relativity", preprint hep-ph/9703240. |
|
|
Simple observations of the existence of cosmic rays lead to extremely
tight limits on Lorentz non-invariance. These are model dependent,
and depending on choice of model and other assumptions limits as good as
5*10-23 are obtained. |
Coleman and Glashow, "High-Energy Tests of Lorentz
Invariance", preprint hep-ph/9812418. |
|
|
A more general perturbative framework is
developed. |
3.6 Tests of the Isotropy of
Space
Hughes et al, Phys. Rev. lett. 4 no. 1 (1960),
p342. Drever, Philosophical Mag. 6, 683. |
|
|
This extremely-accurate experiment looked for any anisotropy in
nuclear magnetic resonance. Hughes placed an upper limit on such
anisotropy of 10-20. |
Prestage et al., Physics Review Letters 54, 2387
(1985). Lamoreaux et al., Physics Review Letters 57,
3125 (1986). Chupp et al., Phys. Rev. Lett. 63, 1541
(1989). |
|
|
Variations on the Hughes-Drever experiment. |
Phillips, Phys. Rev. Lett. 59 no. 15 (1987),
p1784. |
|
|
A test using a cryogenic torsion pendulum carrying a transversely
polarized magnet. No significant anisotropy was
observed. |
See also Brillet
and Hall.
4. Tests of Time Dilation and
Transverse Doppler Effect
The Doppler effect is the observed variation in frequency of a source when it
is observed by a detector that is moving relative to the source. This
effect is most pronounced when the source is moving directly toward or away from
the detector, and in pre-relativity physics its value was zero for transverse
motion (motion perpendicular to the source-detector line). In SR there is
a non-zero Doppler effect for transverse motion, due to the relative time
dilation of the source as seen by the detector. Measurements of Doppler
shifts for sources moving with velocities approaching c can test the validity of
SR's prediction for such observations, which differs significantly from
classical predictions; the experiments support SR and are in complete
disagreement with non-relativistic predictions.
The Ives and Stilwell Experiment
H.E. Ives and G.R. Stilwell, "An Experimental Study of
the Rate of a Moving Atomic Clock", J. Opt. Soc. Am. 28 215-226
(1938); JOSA 31 369-374 (1941). |
|
|
This classic experiment measured the transverse Doppler effect for
moving atoms. |
Hasselkamp et al, Z. Physik A289 (1989),
p151. |
|
|
A measurement which is truly at 90° in the lab. Agreement with
SR to an accuracy of a few percent. |
Measurements of Particle Lifetimes
Rossi and Hoag, Physical Review 57, pg 461
(1940). Rossi and Hall, Physical Review 59, pg 223
(1941). Rasetti, Physical Review 60, pg 198 (1941).
Redei, Phys. Rev. 162 no. 5 (1967), p1299. |
|
|
Various measurements of the lifetimes of muons. See also: Bailey
et al. |
Durbin, Loar and Havens, Physical Review 88, pg
179 (1952). |
|
|
- |
D. Frisch and J. Smith, "Measurement of the Relativistic
Time Dilation Using Mesons", Am. J. Phys. 31 (1963) 342. |
|
|
Measurements of the lifetimes of pions. An interpretation
was given by: Terell, Nuovo Cimento 16 (1960) pg
457. |
Greenberg et al, Phys. Rev. Lett. 23 no. 21
(1969), p1267. |
|
|
More accurate measurement of pion lifetimes. |
Ayres et al, Phys. Rev. D3 no. 5 (1971),
p1051. |
|
|
Measurements of pion lifetimes, comparison of positive and negative
pions, etc. |
Burrowes et al, Phys. Rev. Lett. 2 (1959),
p117. |
|
|
Measurements of Kaon lifetimes. |
Doppler Shift Measurements
Kaivola et al, Phys. Rev. Lett. 54 no. 4 (1985),
p255. McGowan et al, Phys. Rev. Lett. 70 no. 3 (1993),
p251. |
|
|
They compared the frequency of two lasers, one locked to fast-beam
neon and one locked to the same transition in thermal neon. Kaivola
found agreement with SR's Doppler formula is to within 4*10-5;
McGowan within 2.3*10-6. |
Hay et al, Phys. Rev. Lett. 4 (1960), p165. |
|
|
A Moessbauer absorber on a rotor. |
Kuendig, Phys. Rev. 129 no. 6 (1963),
p2371. |
|
|
A Moessbauer absorber on a rotor was used to verify the transverse
Doppler effect of SR to 1.1%. |
Olin et al, Phys. Rev. D8 no. 6 (1973),
p1633. |
|
|
A nuclear measurement at 0.05 c, in very good agreement with the
prediction of SR. |
5. Tests of the "Twin Paradox"
Haefele and Keating, Nature 227 (1970), pg 270
(Proposal); Science Vol. 177 pg 166--170 (1972)
(Experiment). |
|
|
They flew atomic clocks on commercial airliners around the world in
both directions, and compared the time elapsed on the airborne clocks with
the time elapsed on an earthbound clock (USNO). Their eastbound
clock lost 59 ns on the USNO clock; their westbound clock gained 273 ns;
these agree with GR predictions to well within their experimental
resolution and uncertainties (which total about 25
ns). |
Vessot et al, "A Test of the Equivalence Principle Using
a Space-borne Clock", Gel. Rel. Grav., 10, (1979) 181-204; "Test of
Relativistic Gravitation with a Space borne Hydrogen Maser", Phys. Rev.
Lett. 45 2081-2084. |
|
|
They flew a hydrogen maser in a Scout rocket up into space and back
(not recovered). Gravitational effects are important, as are the
velocity effects of SR. |
C. Alley, "Proper Time Experiments in Gravitational
Fields with Atomic Clocks, Aircraft, and Laser Light Pulses," in Quantum
Optics, Experimental Gravity, and Measurement Theory, eds. Pierre
Meystre and Marlan O. Scully, Proceedings Conf. Bad Windsheim 1981, 1983
Plenum Press New York, ISBN 0-306-41354-X, p363-427. |
|
|
They flew atomic clocks in airplanes which remained localized over
Chesapeake Bay, and also which flew to Greenland and
back. |
Bailey et al., "Measurements of
relativistic time dilatation for positive and negative muons in a circular
orbit," Nature 268 (July 28, 1977) pg 301; Nuclear Physics B
150 pg 1-79 (1979). |
|
|
They stored muons in a storage ring and measured their lifetime.
When combined with measurements of the muon lifetime at rest this becomes
a highly-relativistic twin scenario (v ~ 0.9994 c), for which the stored
muons are the traveling twin and return to a given point in the lab every
few microseconds. Muon lifetime at rest:Meyer et al., Physical
Review 132, pg 2693; Balandin et al. JETP 40, pg 811 (1974);
Bardin et al. Physics Letters 137B, pg 135 (1984). Also a test
of the clock hypotheses (below). |
The Clock Hypothesis
The
clock hypothesis states that the tick rate of a clock when measured in an
inertial frame depends only upon its velocity relative to that frame, and is
independent of its acceleration or higher derivatives. The experiment of
Bailey
et al referenced above stored muons in a magnetic storage ring and measured
their lifetime. While being stored in the ring they were subject to a
proper acceleration of approximately 1018 g (1 g = 9.8
m/s2). The observed agreement between the lifetime of the
stored muons with that of muons with the same energy moving inertially confirms
the clock hypothesis for accelerations of that magnitude.
Sherwin, "Some Recent Experimental Tests of the 'Clock
Paradox'", Phys. Rev. 129 no. 1 (1960), p17. |
|
|
He discusses some Moessbauer experiments that show that the rate of a
clock is independent of acceleration (~1016 g) and depends only
upon velocity. |
6. Tests of Relativistic
Kinematics
Kinematics is basically the study of how energy and momentum
conservation laws constrain and affect physical interactions. The two
basic predictions of SR in this regard are that massive objects will have a
limiting velocity of c (the speed of light), and that their "relativistic mass"
will increase with velocity. This latter property implies that the
Newtonian equations for conservation of energy and momentum will be violated by
enormous factors for objects with velocities approaching c, and that the
corresponding formulas of SR must be used. This has become so obvious in
particle experiments that few experiments test the SR equations, and virtually
all particle experiments rely upon SR in their analysis. The exceptions
are primarily early experiments measuring energy as a function of velocity for
electrons and protons.
Elastic Scattering
Champion, Proc. R. Soc. A136 (1932), p630. |
|
|
Electron-electron elastic scattering |
Foley et al, "Experimental Test of the Pion-Nucleon
Forward Dispersion Relation at High Energies", Phys. Rev. Lett. 19
no. 4 (1967), p193. |
|
|
The dispersion relation basically expresses conservation of
probability, and its validity at different energies is related to
relativistic kinematics. |
Experiments Which Show the Limiting Velocity c
Alspector et al, Phys. Rev. Lett. 36, pg 837
(1976). |
|
|
A comparison of neutrino and muon velocities, at
Fermilab. |
Kalbfleisch et al., Physics Review Letters 43, pg
1361 (1979). |
|
|
A comparison of muon, neutrino, and antineutrino velocities over a
range of energies, at Fermilab. |
Guiragosian et al, Phys. Rev. Lett. 34 no. 6
(1975), p335. |
|
|
Relative velocity measurements of 15 GeV electrons and gammas.
No significant difference was observed within ~2 parts in
107. See also Brown
et al. |
G.L. Greene et al.,"Test of special relativity by a
determination of the Lorentz limiting velocity: Does
E=mc2?" Physical Review D 44 (1991) R2216. |
|
|
An analysis combining the results of several experiments gives the
result that the Lorentz limiting velocity must be equal to the speed of
light to within 12 parts per million. |
Stodolsky, "The Speed of Light and the Speed of
Neutrinos", Phys. Lett. B201 no. 3 (1988), p353. |
|
|
A comparison of neutrino and photon speeds from supernova SN1987A Puts
a limit of about 1 part in 108 on their speed
difference. |
Electron Relativistic Mass Variations
W Kaufmann, "Uber die Konstitution des Elektrons" Ann.
Physik 19 ,495 (1906) ( first historical experiment); W.
Kaufmann, "Uber die Konstitution des Elektrons", Sitzungsberichte der
preussichen Akademie der Wissenschaften, 1915, Part 2. |
|
|
There were several discussions about the conclusions from Kaufmann's
experiments and his data analysis. See for instance: M.
Planck, "Die Kaufmannschen Messungen der Ablenkbarkeit der beta-Strahlen
in ihrer Bedeutung fur die Dynamik der Electron", Verhandlungen der
Deutschen Physikalischen Gesellschaft, 8, 1906. M.
Planck, "Nachtrag zu der Besprechung der Kaufmannschen
Ablenkungsmessungen", Verhandlungen der Deutschen Physikalischen
Gesellschaft, 9, 1907. |
A.H. Bucherer, Phyz. Zeitschr. 9 (1908), pg 755;
Ber. d. deutschen Phys. Ges. 6 (1908), pg 688. A.
Bucherer, "Die experimentelle Bestatigung des Relativitatsprinzips",
Annalen der Physik, 28, 1909. |
|
|
- |
E. Hupka, Ann. Phys. 31 (1910), pg 169. |
|
|
- |
Cl. Schaefer and G. Neumann, Phys. Zeitschr. 14
(1913), pg 1117. |
|
|
- |
Ch.E. Guye and Ch. Lavanchy, Comptes rendus 161
(1915), pg 52. |
|
|
- |
Zahn and Spees, Phys. Rev. 53 (1938), p511. |
|
|
- |
Rogers et al. Physical Review 57 (1940),
p379. |
|
|
Measurement of m/e and v for three beta-particles (electrons) from
Radium. Supports the Lorentz model over the Abraham model by >10
sigma. |
Meyer et al. Helv. Physica Acta 36 , pg 981
(1963). |
|
|
- |
W. Bertozzi, Am. J. Phys. 32, 551 (1964). |
|
|
Measurements of speed vs energy for 0.5--15 MeV
electrons. |
Geller and Kollarits, Am. J. Phys. 40 (1972),
p1125. |
|
|
- |
Proton Relativistic Mass Variations
Zrelov, Tiapkin, Farago Soviet Physics JETP, Vol.
34, pg 384 (1958) |
|
|
- |
Calorimetric Test of Special Relativity
D.R. Walz, H.P. Noyes and R.L. Carezani, Physical Review
A29 (1984), pg 2110. |
|
|
The beam power at SLAC is measured using temperature rise in a
calorimeter, for electrons of ~17 and 20 GeV/c and beam currents up to ~15
microamperes. Their results confirm SR with a resolution of about
30%, and are "many orders of magnitude larger than predicted by the theory
of autodynamics", of which Carezani is the author (and also member of this
experimental group). |
7. Other Experiments
The Fizeau
Experiment
Fizeau measured the speed of light in moving mediums,
most notably moving water. Fresnel proposed a "drag coefficient" which
putatively described how strongly a moving material medium "dragged" the
ether. SR predicts no ether but does predict that the speed of light in a
moving medium differs from the speed in the medium at rest, by an amount
consistent (to within experimental resolutions) with these experiments and with
the Fresnel drag coefficient.
Michelson-Morley, Am. J. Sci. 31, 377 (1886). |
|
|
This is a repetition of Fizeau's experiment, NOT the original MMX
experiment! |
Zeeman: Proc. Royal Soc. Amsterdam 17, pg 445
(1914); Proc. Royal Soc. Amsterdam 18, pg 398 (1915); Amst. Versl.
23, pg 245 (1914); Amst. Versl. 24, pg 18 (1915). |
|
|
A critical review of Zeeman's experiments is in: Lerche, American
Journal of Physics Vol. 45, pg 1154 (1977). |
Macek et al, "Measurement of Fresnel Drag with the Ring
Laser", J. Appl. Phys. 35 (1964), p2556. |
|
|
A more accurate, modern repetition. Includes a moving solid, liquid,
and gas. |
Bilger et al, Phys. Rev. A5 (1972) p591. |
|
|
- |
James and Sternberg, Nature 197 (1963),
p1192. |
|
|
Measurements with a glass plate moving perpendicular to the light
path. |
The Sagnac Experiment
Sagnac constructed a ring
interferometer and measured its fringe shifts as it is rotated.
Sagnac, C.R.A.S 157 (1913), p708, p1410; J. Phys.
Radium, 5th Ser. 4 (1914), p177. |
|
|
The classic papers by Sagnac. |
Post, "Sagnac Effect", Rev. Mod. Phys., 39 no. 2,
pg 475 (1967). |
|
|
A review article. This is probably the most useful reference on
ring interferometers and the Sagnac effect. |
Anderson et al, Am. J. Phys. 62 no. 11 (1994),
p975. |
|
|
A more recent review, and description of a much more accurate ring
interferometer. |
Hasselbach and Nicklaus, Phys. Rev. A 48 no. 1
(1993), p143. |
|
|
The Sagnac effect using electrons. |
Allan et al, Science, 228 (1985), p69. |
|
|
They observed the Sagnac effect using GPS satellite signals observed
simultaneously at multiple locations around the world. |
Anandan, "Sagnac Effect in Relativistic and
Nonrelativistic Physics", Phys. Rev. D24 no. 2 (1981), p338.
Gron, "Relativistic description of a Rotating Disk", AJP 43
no. 10 (1975), p869. Rizzi and Tartaglia, "Speed of Light on
Rotating Platforms", preprint gr-qc/9805089.
Mainwaring and Stedman, "Accelerated Clock Principles in Special
Relativity", Phys. Rev. A47 no. 5 (1993), p3611.
Berenda, "The Problem of the Rotating Disk", Phys. Rev. 62
(1942), p280. |
|
|
Various additional papers on the analysis of rotating
systems. |
Ashtekar and Magnon, "The Sagnac Effect in General
Relativity", J. Math. Phys. 16 no. 2 (1975), p341. |
|
|
A discussion using GR. |
The Michelson and Gale Experiment
Michelson and Gale, Nature 115 (1925), p566;
Astrophys. J. 61 (1925), p137. |
|
|
This is essentially the Sagnac experiment, but on a much larger
scale. They constructed a ring interferometer fixed on the ground
with a size of 0.2 mi by 0.4 mi (about 320 m by 640 m). They did
indeed detect the rotation of the earth. |
g-2 Experiments as a Test of Special Relativity
Newman et al, Phys. Rev. Lett. 40 no. 21 (1978),
p1355. |
|
|
A discussion of the basic technique of using measurements of the
anomalous magnetic moment of electrons and muons as a test of SR, and an
analysis of some low-energy electron data. |
F. Combley et al., Physical Review Letters 42
(1979), pg 1383. |
|
|
Electron and muon measurements. |
P.S. Cooper et al,. Physical Review Letters 42
(1979), pg 1386. |
|
|
Electron measurements up to 12 GeV. |
Farley et al, Nuovo Cimento Vol 45, pg 281
(1966). Farley et al, Nature 217, pg 17 (1968).
Bailey et al, Nuovo Cimento 9A, pg 369 (1972).
Bailey et al, Phys. Lett. 68B no. 2 (1977), p191. |
|
|
Measurements of the anomalous magnetic moment of
muons. |
The Global Positioning System (GPS)
Allan et al, IEEE Trans. Inst. and Meas., IM-32
no. 2 (1985), p118. |
|
|
They discuss in detail how time and frequency comparisons among the
various standards organizations of the world can be performed with an
accuracy of about 1 part in 1014, using GPS
satellites. |
Ashby and Allan, "Coordinate time On and Near Earth",
Phys. Rev. Lett. 53 no. 19 (1984), p1858. |
|
|
They discuss how the GPS coordinate system is used on and near
earth. They also describe two different comparisons between USNO and
the Paris Observatory. |
Petit and Wolf, "Relativistic Theory for Picosecond Time
Transfer in the Vicinity of earth", Astron. and Astrophys. 286
(1994), p971. |
|
|
- |
Saburi et al, "High-Precision Time Comparison via
Satellite and Observed Discrepancy of Synchronization", IEEE Trans. Inst.
Meas. IM-25 no. 4 (1976), p473. |
|
|
The "discrepancy" they mention is merely the Sagnac effect, and
observations agree with predictions. |
Lunar Laser Ranging
Bender et al, Science 182 (1973), p229. |
|
|
The corner reflectors placed on the moon by the Apollo astronauts are
used to verify GR with a net accuracy of 15 cm in the
telescope-to-reflector distance. |
Mueller et al, Ap. J. 382 (1991), p L101. |
|
|
- |
Williams et al, Phys. Rev. Lett. 36 no. 11 (1976),
p551. Williams et al, Phys. Rev. D53 no. 12 (1996),
p6730. |
|
|
- |
Dickey et al, Science 265 (1994), p482. |
|
|
- |
Cosmic Microwave Background Radiation (CMBR)
Smoot et al, Phys. Rev. Lett. 39 no. 14 (1977),
p898. |
|
|
Detected an anisotropy in the CMBR, and determined it is primarily a
dipole anisotropy which would be zero in a frame moving at 390 +- 60 km/s
w.r.t. the earth. |
Mather et al, Ap. J. 420 (1994), p439. |
|
|
Measurement of the CMBR by the COBE satellite's FIRAS
instrument. |
Bennett et al, Physics Today (Nov. 1997), p32. |
|
|
Microkelvin variations in the CMBR are described. Note that
these are after the dipole is subtracted out (i.e. these variations are
measured in the "zero-dipole frame" of the CMBR moving about 370 km/s wrt
the earth). |
Songalla et al, Nature 371 (1994), p43. |
|
|
They present a measurement of the CMBR for a distant object with z =
1.776. |
Ge et al, Ap. J. 474 (1997), p67. |
|
|
They present a measurement of the CMBR for a distant object with z =
1.9731. |
The Constancy of Physical Constants
Tubbs and Wolfe, "Evidence for large-Scale Uniformity of
Physical Laws", Ap. J. 236 (1980), pL105. |
|
|
Uniformity to 1 part in 104 is shown, subsequent to an
epoch corresponding to less than 5% of the current age of the
universe. |
Potekhin and Varshalovich, "Non-Variability of the
Fine-Structure Constant over cosmological Time Scales", Astron. Astrophys.
Suppl. Ser. 104 (1994), p89. |
|
|
Quasar spectra with redshifts z ~ 0.2--3.7 are used to put a limit on
the rate of change of alpha of about 4*10-14 per
year. |
The Neutrality of Molecules
Dylla and King, Phys. Rev. A7 (1973) p1224. |
|
|
The charge on sulfur hexafluoride is less than 2*10-19
times the charge on an electron. |
Other experiments that I'm not sure how to classify (and haven't
seen)
Otting, Physik. Zeitschr. 40 , 681 (1939).
Mandelberg and Witten, Journal Opt. Soc. Amer. 52, pg 529
(1962).
Zeitschrift fuer Physik A 342, pg 455
(1992).
8. Experiments Which
Apparently are NOT Consistent with SR/GR
It is clear that most if not all of these experiments have difficulties which
are unrelated to SR. In some cases the inconsistent experiment has been
carefully repeated and been shown to be in error (e.g. Miller, Kantor); in
others the experimental result is so outrageous that any serious attempt to
reproduce it is unlikely (e.g. Esclangon); in still other cases there are great
uncertainties and/or unknowns involved (e.g. Mirabel, Nodland), and some are so
recent that no consensus has yet developed (e.g. Nodland, Anderson). In
any case, no reproducible and generally-accepted experiment is inconsistent with
SR, within its domain
of applicability. Yes in the case of a few anomalous experiments there
is an aspect of this being a self-fulfilling prophecy (being inconsistent with
SR may be considered to be an indication that the experiment is not
acceptable). Note also that few if any standard references or textbooks
even mention the possibility that some experiments might be inconsistent with
SR, and there are also aspects of publication
bias in the literature -- some of these papers appear in obscure
journals. Some of those papers exhibit various levels of incompetence,
which explains their authors' difficulty in being published in mainstream
peer-reviewed journals; the presence of major peer-reviewed journals here
indicates it is not impossible for an anomalous experiment to get published in
them.
All that being said, I repeat: as of this writing there are no reproducible
and generally-accepted experiments that are inconsistent with SR, within its domain
of applicability.
Esclangon, C.R.A.S. 185 no. 26 (1927),
p1593. |
|
|
He observed a systematic variation in the position of an optical
image, correlated with sidereal time. This result is inconsistent
not only with SR, but is also inconsistent with the hypothesis that space
is Euclidean and light travels in straight lines (on earth).
His "signal" is actually composed of points that are an average of
several thousand measurements each, and the magnitude of the signal is
about 25 times smaller than the resolution of the individual
measurements. See Experimenter's
Bias below. |
Miller, Rev. Mod. Phys. 5 (1933), p203. |
|
|
This is a laborious repetition of the Michelson-Morley experiment
(MMX), with observations taken over a decade. He reports a net ether
drift of about 10 km/s, and describes the variation in velocity and
direction in terms of the motions of the sun and the earth combined with a
net ether drift.
This experiment was re-analyzed in: R.S. Shankland, S.W. McCuskey,
F.C. Leone and G. Kuerti, "New Analysis of the Interferometric
Observations of Dayton C. Miller", Rev. Mod. Phys. 27 167-178
(1955). They re-examined Miller's original data logs and explained his
non-null result as partly due to statistical fluctuations and partly due
to local temperature conditions. Their re-analysis is consistent
with a null result at all epochs during a year. They gave no
justification for any correlation with sidereal time such as Miller
reported.
Miller's "signal" is actually composed of points that are an average of
several hundred measurements each, and the magnitude of the signal is more
than 10 times smaller than the resolution with which the measurements were
recorded. See Experimenter's
Bias below. |
Kantor, J. O. S. A. 52 (1962),978. |
|
|
Criticized in: Burcev, Phys. Lett. 5 no. 1 (1963), p44.
Repeated by: Babcock and Bergman, J.O.S.A. 54 (1964),
p147. Repeated by: Rotz, Phys. Lett. 7 no. 4 (1963),
p252. The consensus is now that Kantor's non-null result was due
to his rotating mirrors dragging the air; repetitions in vacuum yield a
null result consistent with SR. |
Silvertooth and Jacobs, Applied Optics 22 no. 9
(1983), p1274. Silvertooth, Specl. Sci. and Tech. 10 no.
1 (1986), p3. Silvertooth and Whitney, Physics Essays 5
no. 1 (1992), p82. |
|
|
This is a series of experiments using variations on a novel
interferometer in which Silvertooth claims to have observed the
ether. The first paper is simply a description of the special
phototube and its usage in measuring Wiener fringes. The second and
third present different variations of Silvertooth's basic
double-interferometer; both claim to observe the ether.
I believe there have been discussions of this in Physics Essays
following the third paper, but I have no access to them.
The experiments are marred by two clear instrumentation effects: there
is almost certainly feedback into the laser in at least the first paper
(and quite probably in the others), and the multi-mode lasers employed
could mimic the effect seen due to the interrelationships among the
different modes. Also the analysis presented is downright wrong --
the anisotropy in the speed of light postulated in the 2nd and 3rd papers
is completely unable to account for their observations (two different
erroneous analyses are presented in the last two papers, making the same
elementary mistake both times: not considering the entire light
path). |
Kolen and Torr, Found. Phys. 12 no. 4 (1982),
p401. Torr and Kolen, NBS Special Publication 617 (1984),
p675-679. |
|
|
This is an experiment using two atomic clocks separated by 500 m which
looks for sidereal variations in the phase between them. The first
paper is merely a proposal, while the second presents results that are
reported to show a non-null result (but other reports indicate consistency
with a null result). That second paper is not available to me as of
this writing. This experiment is quite similar to those of Krisher
et al and Cialdea
referenced above (both of whom reported null results). |
Pearson et al, "Superluminal Expansion of Quasar 3C273".
Nature 290 (1981), p365. Mirabel and Rodriguez, "A
Superluminal Source in the Galaxy", Nature 371 no. 1 (1994),
p46. |
|
|
As of this writing it's not clear to me whether or not these
observations are consistent with SR, GR and/or current cosmological
models.
Note, however, that the simple observation of a visibly-superluminal
expansion or motion of a distant object does not necessarily imply that
anything actually exceeds c locally. See for instance: Gabuzda,
Am. J. Phys. 55 no. 3 (1987), p214. If a high-gamma
(subluminal) object is moving at a small angle wrt our line-of-sight it
can appear to be going faster than light, but is not. This is
different from any uncertainties in distance
scales. |
Nodland and Ralston, "Indication of Anisotropy in
Electromagnetic Propagation over Cosmological Distances", Phys. Rev. Lett.
78 no. 16 (1997), p3043; preprint astro-ph/9704196. |
|
|
As of this writing it's not clear to me whether or not this
observation is consistent with SR, GR and/or current cosmological
models. |
Anderson et al, "Indication from Pioneer 10/11, Galileo,
and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range
Acceleration", preprint gr-qc/9808081. |
|
|
This has been the subject of an ongoing debate in the recent preprint
archives. See also: gr-qc/9809070, gr-qc/9906112, gr-qc/9809075, gr-qc/9810015, gr-qc/9906112, gr-qc/9906113, gr-qc/9907363, gr-qc/9904150.There are
probably additional preprints on this subject. While I see no clear
consensus, there are prosaic explanations offered (anisotropic heat
radiation from the spacecraft). |
Experimenter's Bias
Experimenter's bias is a phenomenon caused by the inability of human
participants in an experiment to remain completely objective, in which the human
experimenter directly influences the experiment's outcome based upon his or her
personal desires or expectations. It is most commonly a concern in medical
and sociological experiments, in which "single-blind" and "double-blind"
protocols are usually required. But some physical experiments in which a
human observer is required to round-off measurements can also be subject to
it. In the experiments here the conditions for this are basically the
combination of a signal smaller than the actual measurement resolution and an
over-averaging of the data used to extract the "signal" from the
measurements.
In principle, if a measurement has a resolution of R, then if the
experimenter averages N independent measurements the average will
have a resolution of R/sqrt(N) (this is the central limit theorem of
statistics). This is an important experimental technique used to reduce
the impact of randomness on an experiment's outcome. But note that this
requires that the measurements be statistically independent, and
there are several reasons why that may not be true -- if so then the average may
not actually be a better measurement but may merely reflect the correlations
among the individual measurements and their non-independent nature.
The most common cause of non-independence is systematic errors (errors
affecting all measurements equally, causing the different measurements to be
highly correlated, so the average is no better than any single
measurement). But another cause can be due to the inability of a human
observer to round off measurements in a truly random manner. If an
experiment is searching for a sidereal variation of some measurement, and if the
measurement is rounded-off by a human who knows the sidereal time of the
measurement, and if hundreds of measurements are averaged to extract a "signal"
which is smaller than the apparatus' actual resolution, then it should be clear
that this "signal" can come from the non-random round-off, and not from the
apparatus itself. In such cases a single-blind experimental protocol is
required; if the human observer does not know the sidereal time of the
measurements, then even though the round-off is non-random it cannot introduce a
spurious sidereal variation.
Note that modern electronic and/or computerized data acquisition techniques
have greatly reduced the likelihood of such bias, but it can still be introduced
by a poorly-designed analysis technique. Experimenter's bias was not well
recognized until the 1950's and 60's, and then it was primarily in medical
experiments and studies. Its effects on experiments in the physical
sciences have not always been fully recognized. Several experiments
referenced above were clearly affected by it.
Publication Bias
There
are two very different aspects of publication bias:
- Unpopular or unexpected results may not be published because either the
original experimenters or some journal referees have misgivings or
reservations about the results, based on the results themselves and not any
independent evaluation of experimental procedures or technique.
- Expected experimental results may not be published because either
the original experimenters or some journal referees do not consider them
interesting enough to merit publication.
In both cases the
experimental record in the literature does not fully and accurately reflect the
actual experiments that have been performed. Both of these effects clearly
affect the literature on experimental tests of SR. This second aspect is
one reason why this list of experiments is incomplete; there have probably been
many hundreds of unpublished experiments that agree with SR.
Note that this does not include papers that are rejected for other
reasons, such as: inappropriate subject or style, major internal
inconsistencies, or downright incompetence on the part of authors or
experimenters. Such rejections are not bias, they are the proper
functioning of a peer-reviewed journal.
9. Acknowledgments
My interest in the experimental basis of SR has been piqued by many
discussions in the newsgroup sci.physics.relativity about how well SR has or has
not been confirmed or refuted. One effect of this is that I have assembled
a rather large collection of papers on experimental tests of SR; this FAQ page
is in some sense an index to this collection. Most of the descriptions
above are my summaries direct from primary sources. In some cases the
original paper was unavailable to me and I have relied on secondary sources
(primarily the previous version of this FAQ page, and the books by Zhang, by
Born, and by von Laue).
I wish to thank the previous authors of this FAQ, most notably Siegmar
Schleif whose original list of references provided a fertile source of papers
for my collection (and also the original source of this page several years
ago). While the previous authors may have difficulty finding their
original words in this revision, they will note that I have not deleted a single
reference while adding many. I also wish to thank Nathan Urban, who as
"keeper of the FAQ" has provided invaluable assistance and numerous
suggestions.
Tom Roberts tjroberts@lucent.com [Top]