The Michelson-Morley Experiment and the Dimensions of Moving Bodies

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The Michelson-Morley Experiment and the Dimensions of Moving Bodies  (1921) 
by Hendrik Lorentz
Nature, Volume 106, Issue 2677, pp. 793-795, Source

The Michelson-Morley Experiment and the Dimensions of Moving Bodies.

By Prof. H. A. Lorentz, For.Mem.R.S.

AS doubts have sometimes been expressed concerning the interpretation of Prof. Michelson's celebrated experiment, some remarks on the subject will perhaps not be out of place here. I shall try to show, by what seems to me an unimpeachable mode of reasoning, that, if we adopt Fresnel's theory of a stationary æther, supposing also that a material system can have a uniform translation with constant velocity v without changing its dimensions, we must surely expect the result that was predicted by Maxwell.

Let us introduce a system of rectangular axes of co-ordinates fixed to the material system, the axis of x being in the direction of the motion. Then, with respect to these axes, the æther will flow with the velocity -v. The progress of waves of light, relatively to them, may be traced by means of Huygens's principle; for this purpose it suffices to know the form and position of the elementary waves. For the sake of generality I shall suppose the propagation to take place in a material medium of refractive index \mu, so that, if c is the velocity of light in the æther, the velocity in the medium when at rest would be c/\mu. The elementary wave formed in the time dt around a point P will be a sphere of radius (c/\mu)dt, of which the centre P' does not, however, coincide with P, the line PP' being in the direction opposite to that of OX. and having the length \left(v/\mu^{2}\right)dt (Fresnel's coefficient).

If Q is any point on the surface of the sphere, PQ can be considered as an element of a ray of light, and w=PQ/dt will be the velocity of the ray. Confining ourselves to terms of the second order, i.e. of the order v^{2}/c^{2}, and denoting by \delta the angle between the ray and OX, we have

\frac{1}{w}=\frac{\mu}{c}+\frac{v}{c^{2}}\cos\delta+\frac{v^{2}}{2\mu c^{3}}\left(1+\cos^{2}\delta\right) (1)

Now, let A and B be points having fixed positions in the material system. The course s of a ray of light passing from A to B will be determined by the condition that the integral

\int\frac{ds}{w} (2)

is a minimum. Using the above value of 1/w, it is easily shown that, if quantities of the second order are neglected, the course of the ray is not affected by the translation v, so that, if L_{0} is the path of the ray in the case v = 0, and L the real path, these lines will be distant from each other to an amount of the second order only. Hence, if in the case of a translation v we calculate by means of (1) the integral (2), both for L and L_{0}, the two values will differ by no more than a quantity of the fourth order; indeed, since the integral is a minimum for L, the difference must be of the second order with respect to the distances between L and L_{0}, and these distances are already of the second order of magnitude.

It is seen in this way that, so long as we neglect terms of an order higher than the second, we may replace

\int\limits _{L}\frac{ds}{w} by \int\limits _{L_{0}}\frac{ds}{w'}

an argument that must not be overlooked in the theory of the experiment. On the ground of it we shall commit no error if, in determining the paths L_{1} and L_{2} of two rays that start from a point A, and are made to interfere at a point B, we take no account of the motion of the apparatus. The change in the difference of phase produced by the translation will be given by the difference between the values which the integral

\int\frac{v^{2}}{2\mu c^{3}}\left(1+\cos^{2}\delta\right)ds

takes for the lines L_{1} and L_{2} so determined. If, along the first of them, \cos^{2}\delta=1, and along the second \cos^{2}\delta=0, and \mu=1, the change will be the same as would be produced by a lengthening of L_{1} in the ratio of 1 to 1+v^{2}/2c^{2}. As no displacement of the fringes has been observed, we are led to the well-known hypothesis of a contraction of moving bodies in the direction of translation, in the ratio of 1 to 1-v^{2}/2c^{2}.

We could now try to extend the above considerations to cases in which v/c, though always below 1, is no longer a small fraction. This would require somewhat lengthy calculations, into which, however, we need not enter here, because we know by the theory of relativity that the true value of the coefficient of contraction is \sqrt{1-v^{2}/2c^{2}}. I may remark here that there can be no question about the reality of this change of length. Suppose that, in studying the phenomena, we use a system of rectangular co-ordinates x_{1},x_{2},x_{3}, and a time t, and that in this system the velocity of light is c in all directions. Further, let there be two rods, I. and II., exactly equal to each other, and both placed in the direction of x_{1}, I. at rest in the system of co-ordinates, and II. moving in the direction of its length with a velocity v. Then, certainly, if the length of a rod is measured by the differences of the values which the coordinate x_{1} has at the two ends at one and the same instant t, II. will be shorter than I., just as it would be if it were kept at a lower temperature. I need scarcely add that if, by the ordinary transformation of the theory of relativity, we pass to new co-ordinates x_{1}',x_{2}',x_{3}',t' in such a manner that in this system the rod II. is at rest, and if now we measure the lengths by the difference between the values of x_{1}' which correspond to a definite value of t', I. will be found to be the shorter of the two.

The question arises as to how far the dimensions of a solid body will be changed when its parts have unequal velocities, when, for example, it has a rotation about a fixed axis. It is clear that in such a case the different parts of the body will, by their interaction, hinder each other in their tendency to contract to the amount determined by \sqrt{1-v^{2}/c^{2}}. The problem can be solved by the ordinary theory of elasticity, provided only that this theory be first adapted to the principle of relativity. Indeed, we can still use Hamilton's principle: —

\delta\int_{t_{1}}^{t_{2}}dt\int(T-U)dS=0 (3)

(dS, element of volume; T, kinetic, and U, potential, energy, both per unit of volume), if, by some slight modifications, the integral is made to be independent of the particular choice of co-ordinates. That this can be done, even in the general theory of relativity (theory of gravitation), is due to the possibility of expressing the length of a line-element in the four-dimensional space x_{1},x_{2},x_{3},x_{4}\ \left(x_{4}=t\right) in "natural units" — i.e. in such a manner that the number obtained for it is the same whatever be the co-ordinates chosen — and of measuring angles in a similar way. As is well known, the length ds of a line-element is given by the formula : —

ds^{2}=\sum(ab)g_{ab}dx_{a}dx_{b} (4)

where the ten quantities g_{ab}\ \left(g_{ab}=g_{ba}\right) are the gravitation potentials, and the angle \delta between two elements is determined by

\cos\delta ds\ d's=\sum(ab)g_{ab}dx_{a}d'x_{b} (5)

In the sums, each of the indices a and b is to be given the values 1, 2, 3, 4. When the value 4 is excluded, as will be the case in some of the following formulae, a Greek letter will be used for the index.

We can also find an invariant value l for the distance between two material particles P and P' infinitely near each other. To this effect we have to consider the word-lines L and L' of these particles in the space x_{1},x_{2},x_{3},x_{4}. Let Q be the point of L corresponding to the chosen time x_{4}, and Q' a point of L' such that QQ' is at right angles to L. Then the length of QQ', determined by means of (4), will be the value required. Similarly, if P'' is a third particle, infinitely near P and P', and Q'' the point of its word-line so situated that QQ'' is perpendicular to L, the angle P'PP'' will be taken to be the angle between the elements QQ' and QQ'' determined according to (5).

As to the co-ordinates x_{1},x_{2},x_{3},x_{4}, it may be recalled that, in a field free from gravitation, they may be chosen in such a manner (x_{1},x_{2},x_{3} being at right angles to each other) that the velocity of light has the constant magnitude c; the potentials g_{ab} will in this case have the values

g_{11}=g_{22}=g_{33}=-1,\ g_{44}=c^{2},\ g_{ab}=0\, for a\ne b\,

These may be called the normal values of the potentials, and a system of co-ordinates for which they hold a normal system.

Let us now consider a solid body M, and let us first conceive it to be placed in a normal system of co-ordinates (S_{0}), and to be at rest in that system, free from all external forces. The body may then be said to be in its natural state, and its particles may be distinguished from each other by their co-ordinates \xi,\eta,\zeta with respect to three rectangular axes fixed in the body. In all that follows, these quantities will be constant, and so will be the mass \rho d\xi d\eta d\zeta of an element, \rho being the density in the natural state.

We shall now suppose the body to be placed in a system of co-ordinates x_{1},x_{2},x_{3},x_{4}\ (S), not necessarily normal, and to have some kind of motion in that system. It is this motion, in which x_{1},x_{2},x_{3} will be definite functions of \xi,\eta,\zeta, and x_{4}, which we want to determine by means of Hamilton's principle properly modified.

In order to get the new U, I shall introduce the dilatations \xi_{\xi},\eta_{\eta},\zeta, and shearing strains \xi_{\eta},\eta_{\zeta},\zeta, with respect to the axes \xi,\eta,\zeta. These quantities are defined as follows: —

Let P, P' be the particles \xi,\eta,\zeta, and \xi+d\xi,\eta,\zeta, and let l be their distance in the state considered (system S), and l_{0} their distance in the natural state (system S_{0}), these distances being both determined in the manner specified in what precedes. Then

\xi^{\xi}=\left(l-l_{0}\right)/l_{0}\,

Again, if P'' is the particle \xi,\eta+d\eta,\zeta, and if the angle P'PP'', calculated as stated before, has in the two cases the values \delta and \delta_{0}\left(=\tfrac{1}{2}\pi\right), we shall have

\xi^{\eta}=\delta_{0}-\delta

The six deformations \xi_{\xi}\dots will be considered as infinitely small. In the problem we have in view, they are of the order of magnitude v^{2}/c^{2}, so that our final result will be correct to that order.

If we put

U=A\left(\xi_{\xi}^{2}+\eta_{\eta}^{2}+\zeta_{\zeta}^{2}\right)+\frac{1}{2}B\left(\xi_{\xi}+\eta_{\eta}+\zeta_{\zeta}\right)^{2}+\frac{1}{2}A\left(\xi_{\eta}^{2}+\eta_{\zeta}^{2}+\zeta_{\xi}^{2}\right) (6)

the well-known expression for the potential energy of an isotropic elastic body, U will be invariant for any change of co-ordinates.

As to the kinetic energy T, it is to be replaced by an expression containing \rho\tfrac{ds}{dt}. Finally, we must write, instead of (3),

\delta\int_{t_{1}}^{t_{2}}\int\left(-c\rho-\frac{1}{c}U\right)\frac{ds}{dt}dt\ d\xi\ d\eta\ d\zeta=0

We have still to add the formula; that are found by working out the above definitions of \xi_{\xi},\xi_{\eta}, etc. viz.:—

\xi_{\xi}=-\frac{1}{2}\sum(\alpha\beta)g_{\alpha\beta}\frac{\partial x_{\alpha}}{\partial\xi}\frac{\partial x_{\beta}}{\partial\xi}+\frac{\left[\sum(\alpha\beta)g_{\alpha\beta}v_{\beta}\frac{\partial x_{\alpha}}{\partial\xi}\right]^{2}}{2\sum(ab)g_{ab}v_{a}v_{b}}-\frac{1}{2}

\xi_{\eta}=-\sum(\alpha\beta)g_{\alpha\beta}\frac{\partial x_{\alpha}}{\partial\xi}\frac{\partial x_{\beta}}{\partial\eta}+\frac{\sum(\alpha\beta)g_{\alpha\beta}v_{\beta}\frac{\partial x_{\alpha}}{\partial\xi}\cdot\sum(\alpha\beta)g_{\alpha\beta}v_{\beta}\frac{\partial x_{\alpha}}{\partial\eta}}{\sum(ab)g_{ab}v_{a}v_{b}}

(v_{1},v_{2},v_{3} are the components of the velocity, and v_{4}=1).

In our problem the body is supposed to move in a normal system of co-ordinates. By this our formula; simplify to[1]

\delta\int_{t_{1}}^{t_{2}}\int\left(-c^{2}\rho-U\right)\left(1-\frac{v^{2}}{c^{2}}\right)^{\frac{1}{2}}dt\ d\xi\ d\eta\ d\zeta=0,

\xi_{\xi}=\frac{1}{2}\sum(\alpha)\left(\frac{\partial x_{\alpha}}{\partial\xi}\right)^{2}+\frac{\left[\sum(\alpha)v_{a}\frac{\partial x_{\alpha}}{\partial\xi}\right]^{2}}{2\left(c^{2}-v^{2}\right)}-\frac{1}{2},

\xi_{\eta}=\sum(\alpha)\frac{\partial x_{\alpha}}{\partial\xi}\frac{\partial x_{\alpha}}{\partial\eta}+\frac{\sum(\alpha)v_{\alpha}\frac{\partial x_{\alpha}}{\partial\xi}\cdot\sum(\alpha)v_{a}\frac{\partial x_{\alpha}}{\partial\eta}}{c^{2}-v^{2}},

(7)

When applied to a revolving body, these equations will enable us to determine the deformation that is produced, wholly independently of the theory of relativity, by centrifugal force, a deformation that will in reality far surpass the changes we want to consider. To get free from it we can consider the ideal case of a "rigid" body — i.e. a body for which the moduli of elasticity A and B in (6) are infinitely great. The centrifugal force will then have no effect on the dimensions, but the changes required by the theory of relativity will subsist. The assumption has also the advantage of simplifying the calculations ; indeed, since U becomes infinitely great, the term -c^{2}\rho in (7) may be omitted.

I have worked out the case of a thin circular disc rotating with constant speed about an axis passing through its centre, at right angles to its plane. The result is that, if v is the velocity at the rim, the radius will be shortened in the ratio of 1 to 1-\tfrac{1}{8}\tfrac{v^{2}}{c^{2}}. The circumference changing to the same extent, its decrease is seen to be exactly one-fourth of that of a rod moving with the same velocity in the direction of its length. That there would be a smaller contraction was to be expected; indeed, the case can be compared to what takes place when a hot metal band is fitted tightly around a wheel and then left to cool.

At first sight our problem seems to lead to a paradox. Let there be two equal discs A and B, mounted on the same axis, A revolving and B at rest. Then A will be smaller than B, and it must certainly appear so (the discs being supposed to be quite near each other) to any observer, whatever be the system of co-ordinates he chooses to use. However, we can introduce a system of co-ordinates S' revolving with the disc A; with respect to these it will be B that rotates, and so one might think that now this latter disc would be the smaller of the two. The conclusion would be wrong because the system S' would not be a normal one. If we leave S for it, we must at the same time change the potentials g_{ab}, and if this is done the fundamental equation will certainly again lead to the result that A is smaller than B.


  1. If in (7) we replace \left(1-v^{2}/c^{2}\right)^{\frac{1}{2}} by 1-v^{2}/2c^{2}, omitting the constant term -c^{2}\rho and neglecting U\cdot v^{2}/2c^{2}, we are led back to the ordinary formula (3).
This work is in the public domain in the United States because it was published before January 1, 1923.

The author died in 1928, so this work is also in the public domain in countries and areas where the copyright term is the author's life plus 80 years or less. This work may also be in the public domain in countries and areas with longer native copyright terms that apply the rule of the shorter term to foreign works.