Aether drag hypothesis
In the 19th century, the theory of the luminiferous aether as the hypothetical medium for the propagation of light was widely discussed. An important part of this discussion was the question concerning the state of motion of Earth with respect to this medium. The aether drag hypothesis dealt with the question of whether or not the luminiferous aether is dragged by or entrained within moving matter. According to the first variant no relative motion exists between Earth and aether; according to the second one, relative motion exists and thus the speed of light should depend on the speed of this motion ("aether wind"), which should be measurable by instruments at rest on Earth's surface. Specific aether models were invented by Augustin-Jean Fresnel who in 1818 proposed that the aether is partially entrained by matter. The other one was proposed by George Stokes in 1845, in which the aether is completely entrained within or in the vicinity of matter.
While Fresnel's almost stationary theory was apparently confirmed by the Fizeau experiment (1851), Stokes' theory was apparently confirmed by the Michelson–Morley experiment (1881, 1887). This contradictory situation was resolved by the works of Hendrik Antoon Lorentz (1895, 1904) whose Lorentz ether theory banished any form of aether dragging, and finally with the work of Albert Einstein (1905) whose theory of special relativity does not contain the aether as a mechanical medium at all. 
Partial aether dragging
In 1810, François Arago realised that variations in the refractive index of a substance predicted by the corpuscular theory would provide a useful method for measuring the velocity of light. These predictions arose because the refractive index of a substance such as glass depends on the ratio of the velocities of light in air and in the glass. Arago attempted to measure the extent to which corpuscles of light would be refracted by a glass prism at the front of a telescope. He expected that there would be a range of different angles of refraction due to the variety of different velocities of the stars and the motion of the earth at different times of the day and year. Contrary to this expectation he found that there was no difference in refraction between stars, between times of day or between seasons. All Arago observed was ordinary stellar aberration.
In 1818, Augustin-Jean Fresnel examined Arago's results using a wave theory of light. He realised that even if light were transmitted as waves the refractive index of the glass-air interface should have varied as the glass moved through the aether to strike the incoming waves at different velocities when the earth rotated and the seasons changed. Fresnel proposed that the glass prism would carry some of the aether along with it so that "..the aether is in excess inside the prism". He realised that the velocity of propagation of waves depends on the density of the medium so proposed that the velocity of light in the prism would need to be adjusted by an amount of 'drag'. The velocity of light in the glass without any adjustment is given by:
The drag adjustment is given by:
Where is the aether density in the environment, is the aether density in the glass and is the velocity of the prism with respect to the aether.
The factor can be written as because the refractive index, n, would be dependent on the density of the aether. This is known as the Fresnel drag coefficient. The velocity of light in the glass is then given by:
This correction was successful in explaining the null result of Arago's experiment. It introduces the concept of a largely stationary aether that is dragged by substances such as glass but not by air. Its success favoured the wave theory of light over the previous corpuscular theory.
Problems of partial aether dragging
Fresnel's dragging coefficient was directly confirmed by the Fizeau experiment and its repetitions. In general, with the aid of this coefficient the negative result of all optical aether drift experiments sensitive enough to detect first order effects (such as the experiments of Arago, Fizeau, Hoek, Airy, Mascart) can be explained. The notion of an (almost) stationary aether is also consistent with stellar aberration. However, this theory is considered to be refuted for the following reasons:
- It was already known in the 19th century, that partial aether dragging requires the relative velocity of aether and matter to be different for light of different colours – which is evidently not the case.
- Fresnel's theory of an (almost) stationary aether predicts positive results by experiments which are sensitive enough to detect second order effects. However, experiments such as the Michelson–Morley experiment and the Trouton–Noble experiment, gave negative results within their margin of error and are therefore considered refutations of Fresnel's aether.
- In the Hammar experiment, conducted by Gustaf Wilhelm Hammar in 1935, a common-path interferometer was used. Massive lead blocks were installed on both sides of only one leg of the interferometer. This arrangement should cause different amounts of aether drag and therefore produce a positive result. However, the result was again negative.
Complete aether dragging
For George Stokes (1845) the model of an aether which is totally unaffected or only partially affected by moving matter was unnatural and unconvincing, so he assumed that the aether is completely dragged within and in the vicinity of matter, partially dragged at larger distances, and stays at rest in free space. Also Heinrich Rudolf Hertz (1890) incorporated a complete aether drag model within his elaboration of Maxwell's theory of electromagnetism, to bring it into accord with the Galilean principle of relativity. That is, if it is assumed that the aether is at rest within matter in one reference frame, the Galilean transformation gives the result that matter and (entrained) aether travel with the same speed in another frame of reference.
Problems of complete aether dragging
Complete aether dragging can explain the negative outcome of all aether drift experiments (like the Michelson–Morley experiment). However, this theory is considered to be wrong for the following reasons:
- The Fizeau experiment (1851) indicated only a partial entrainment of light.
- The Sagnac effect shows that two rays of light, emanated from the same light source in different directions on a rotating platform, require different times to come back to the light source. However, if the aether is completely dragged by the platform this effect should not occur at all.
- Oliver Lodge conducted experiments in the 1890s, seeking evidence that the propagation of light is influenced by being in the proximity of large rotating masses, and found no such influence.
- It is inconsistent with the phenomenon of stellar aberration. In stellar aberration the position of a star when viewed with a telescope swings each side of a central position by about 20.5 seconds of arc every six months. This amount of swing is the amount expected when considering the speed of earth's travel in its orbit. In 1871 Airy demonstrated that stellar aberration occurs even when a telescope is filled with water. It seems that if the aether drag hypothesis were true then stellar aberration would not occur because the light would be travelling in the aether which would be moving along with the telescope. Consider a bucket on a train about to enter a tunnel, and a drop of water drips from the tunnel entrance into the bucket at the very center. The drop will not hit the center at the bottom of the bucket. The bucket is analogous to the tube of a telescope, the drop is a photon and the train is the earth. If aether is dragged then the droplet would be traveling with the train when it is dropped and would hit the center of bucket at the bottom. The amount of stellar aberration, , is given by:
- The speed at which the earth goes round the sun, v = 30 km/s, and the speed of light is c = 299,792,458 m/s which gives = 20.5 seconds of arc every six months. This amount of aberration is observed and this contradicts the complete aether drag hypothesis.
Stokes' responses to those problems
Stokes already in 1845 introduced some additional assumptions in order to bring his theory into accord with experimental results. To explain aberration, he assumed that his incompressible aether is irrotational as well, which would give, in connection with his specific model of aether drag, the correct law of aberration. To reproduce Fresnel's dragging coefficient (and therefore to explain the Fizeau experiment) he argued that the aether is completely dragged within a medium – i.e. the aether gets condensed when it enters the medium and rarefied when it leaves it again, which modifies the speed of the aether as well as that of light and leads to the same expression as Fresnel's.
Even though Stokes' aberration theory was considered viable for some time, it had to be given up because Lorentz argued in 1886, that when the aether is incompressible as in Stokes' theory, and if the aether has the same normal component of velocity as the earth, it would not have the same tangential component of velocity, so all conditions posed by Stokes cannot be fulfilled at the same time.
Gravitational aether drag
Another version of Stokes' model was proposed by Theodor des Coudres and Wilhelm Wien (1900). They assumed that aether dragging is proportional to the gravitational mass. That is, the aether is completely dragged by the earth, and only partially dragged by smaller objects on earth. And to save Stokes's explanation of aberration, Max Planck (1899) argued in a letter to Lorentz, that the aether might not be incompressible, but condensed by gravitation in the vicinity of earth, and this would give the conditions needed for the theory of Stokes ("Stokes-Planck theory"). When compared with the experiments above, this model can explain the positive results of the experiments of Fizeau and Sagnac, because the small mass of those instruments can only partially (or not at all) drag the aether, and for the same reason it explains the negative result of Lodge's experiments. It is also compatible with Hammar's and Michelson–Morley experiment, as the aether is completely dragged by the large mass of earth.
However, this theory was directly refuted by the Michelson–Gale–Pearson experiment (1925). The great difference of this experiment against the usual Sagnac experiments is the fact that the rotation of earth itself was measured. If the aether is completely dragged by the Earth's gravitational field, a negative result has to be expected - but the result was positive.
And from a theoretical side it was noted by Hendrik Antoon Lorentz, that the Stokes-Planck hypothesis requires that the speed of light is not affected by a density increase of 50,000 times of the aether. So Lorentz and Planck himself rejected this hypothesis as improbable.
Lorentz and Einstein
Since Lorentz was forced to abandon Stokes' hypothesis, he chose Fresnel's model as a starting point. He was able to reproduce Fresnel's dragging coefficient in 1892, though in Lorentz's theory it represents a modification of the propagation of light waves, not the result of any aether entrainment. Therefore, Lorentz's aether is fully stationary or immobile. However, this leads to the same problem that already afflicted Fresnel's model: it stood in contradiction with the Michelson–Morley experiment. Therefore, George Francis FitzGerald (1889) and Lorentz (1892) introduced length contraction, that is, all bodies contract in the line of motion by the factor . In addition, in Lorentz's theory the Galilean transformation was replaced by the Lorentz transformation.
However, the accumulation of hypotheses to rescue the stationary aether concept was considered to be very artificial. So it was Albert Einstein (1905), who recognized that it is only required to assume the principle of relativity and the constancy of the speed of light in all inertial frames of reference, in order to develop the theory of special relativity and to derive the complete Lorentz transformation. All this was done without using the stationary aether concept.
As shown by Max von Laue (1907), special relativity predicts the result of the Fizeau experiment from the velocity addition theorem without any need for an aether. If is the velocity of light relative to the Fizeau apparatus and is the velocity of light relative to the water and is the velocity of the water:
which, if v/c is small can be expanded using the binomial expansion to become:
Allais aether hypothesis
Maurice Allais proposed in 1959 an aether hypothesis involving a wind velocity of about 8 km/s, much lower than the standard value of 30 km/s supported by scientists of the nineteenth century, and compatible with the Michelson–Morley and the Dayton Miller experiments, as well as his own experiments regarding the controversial Allais effect unpredictable by general relativity. Despite advocating for the need of another theory of gravity, his hypothesis didn't gain significant traction amongst mainstream scientists.
In modern physics (which is based on the theory of relativity and quantum mechanics), the aether as a "material substance" with a "state of motion" no longer plays any role. So questions concerning a possible "aether drag" are no longer considered meaningful by the scientific community. However, frame-dragging as predicted by general relativity, in which rotating masses distort the spacetime metric, causing a precession of the orbit of nearby particles, does exist. But this effect is orders of magnitude weaker than any "aether drag" discussed in this article.
- History of special relativity
- Tests of special relativity
- Tests of general relativity
Bibliography and references
- Whittaker, Edmund Taylor (1910), A History of the theories of aether and electricity (1. ed.), Dublin: Longman, Green and Co.
- Jannsen, Michel; Stachel, John (2008), The Optics and Electrodynamics of Moving Bodies (PDF)
- Rafael Ferraro; Daniel M Sforza (2005), "Arago (1810): the first experimental result against the ether", Eur. J. Phys., 26 (1): 195–204, arXiv:physics/0412055, Bibcode:2005EJPh...26..195F, doi:10.1088/0143-0807/26/1/020, S2CID 119528074
- Arago, A. (1810–1853), "Mémoire sur la vitesse de la lumière, lu à la prémière classe de l'Institut, le 10 décembre 1810", Comptes Rendus de l'Académie des Sciences, 36: 38–49
- Fresnel, A. (1818), "Lettre de M. Fresnel à M. Arago sur l'influence du mouvement terrestre dans quelques phénomènes d'optique", Annales de Chimie et de Physique, 9: 57–66 (Sep. 1818), 286–7 (Nov. 1818); reprinted in H. de Senarmont, E. Verdet, and L. Fresnel (eds.), Oeuvres complètes d'Augustin Fresnel, vol. 2 (1868), pp. 627–36; translated as "Letter from Augustin Fresnel to François Arago, on the influence of the movement of the earth on some phenomena of optics" in K.F. Schaffner, Nineteenth-Century Aether Theories, Pergamon, 1972, pp. 125–35, doi:10.1016/B978-0-08-015674-3.50011-7; also translated by R.R. Traill as "Letter from Augustin Fresnel to François Arago concerning the influence of terrestrial movement on several optical phenomena", General Science Journal, 23 January 2006 (8 pp.).
- G. W. Hammar (1935), "The Velocity of Light Within a Massive Enclosure", Physical Review, 48 (5): 462–463, Bibcode:1935PhRv...48..462H, doi:10.1103/PhysRev.48.462.2
- Stokes, George Gabriel (1845), doi:10.1080/14786444508645215 , Philosophical Magazine, 27 (177): 9–15,
- Stokes, George Gabriel (1846), doi:10.1080/14786444608645365 , Philosophical Magazine, 28 (185): 76–81,
- Stokes, George Gabriel (1846), doi:10.1080/14786444608562589 , Philosophical Magazine, 29 (191): 6–10,
- Stokes, George Gabriel (1848), doi:10.1080/14786444808645996 , Philosophical Magazine, 32: 343–349,
- Georg Joos: Lehrbuch der theoretischen Physik. 12. edition, 1959, page 448
- Lodge, Oliver J. (1893), "Aberration Problems", Philosophical Transactions of the Royal Society A, 184: 727–804, Bibcode:1893RSPTA.184..727L, doi:10.1098/rsta.1893.0015
- Lodge, Oliver J. (1897), Philosophical Transactions of the Royal Society A, 189: 149–166, Bibcode:1897RSPTA.189..149L, doi:10.1098/rsta.1897.0006 ,
- Lorentz, Hendrik Antoon (1886), "De l'influence du mouvement de la terre sur les phénomènes lumineux", Archives Néerlandaises des Sciences Exactes et Naturelles, 21: 103–176
- Wien, Wilhelm (1898), , Annalen der Physik, 301 (3): I–XVIII.
- Lorentz, H.A. (1899), "Stoke's Theory of Aberration in the Supposition of a Variable Density of the Aether", Proceedings of the Royal Society, 1: 443–448, Bibcode:1898KNAB....1..443L, archived from the original on 2008-04-04
- Lorentz, Hendrik Antoon (1904), , Proceedings of the Royal Netherlands Academy of Arts and Sciences, 6: 809–831
- Einstein, Albert (1905), "On the Electrodynamics of Moving Bodies", Annalen der Physik, 322 (10): 891–921, Bibcode:1905AnP...322..891E, doi:10.1002/andp.19053221004.
- Laue, Max von (1907), "Die Mitführung des Lichtes durch bewegte Körper nach dem Relativitätsprinzip" [The Entrainment of Light by Moving Bodies in Accordance with the Principle of Relativity], Annalen der Physik (in German), 23 (10): 989–990, Bibcode:1907AnP...328..989L, doi:10.1002/andp.19073281015
- Miller, Dayton C. (July 1933). "The Ether-Drift experiment and the determination of the absolute motion of the Earth" (PDF). Reviews of Modern Physics. 5 (3): 203–254. Bibcode:1933RvMP....5..203M. doi:10.1103/RevModPhys.5.203.
- Allais, M. (September 1959). "Should the Laws of Gravitation Be reconsidered? Part I – Abnormalities in the Motion of a Paraconical Pendulum on an Anisotropic Support" (PDF). Aero/Space Engineering: 46–52. Archived from the original (PDF) on 2015-07-20. Retrieved 2017-03-30.
- Allais, M. (October 1959). "Should the Laws of Gravitation Be reconsidered? Part II – Experiments in Connection with the Abnormalities Noted in the Motion of the Paraconical Pendulum With an Anisotropic Support" (PDF). Aero/Space Engineering: 51–55. Archived from the original (PDF) on 2016-06-22. Retrieved 2017-03-30.
- Deloly, Jean-Bernard. "The re-examination of Miller's interferometric observations and of Esclangon's observations". Maurice Allais Foundation.
- Wikibooks: Special Relativity
- Resnick, Robert, Basic Concepts in Relativity and Early Quantum Theory, 1972, John Wiley and Sons Inc.
- Mathpages: Stokes’ Mistake