The conservation laws of nonrelativistic and relativistic systems are reviewed and some simple illustrations are provided for the restrictive nature of the relativistic conservation law involving the center of energy compared to the nonrelativistic conservation law for the center of mass. Extension of the nonrelativistic interaction of particles through a potential to a system that is Lorentz-invariant through order v2c2 is found to require new velocity- and acceleration-dependent forces that are suggestive of a field theory where the no-interaction theorem of Currie, Jordan, and Sudershan does not hold.

1.
This belief is encouraged by mechanics texts that write one-particle “relativistic Lagrangians” with an arbitrary potential function V(r) rather than applying external forces to a relativistic particle. See, for example, Refs. 2 and 3.
2.
H.
Goldstein
,
C.
Poole
, and
J.
Safko
,
Classical Mechanics
, 3rd ed. (
Addison-Wesley
,
New York
,
2002
), p.
313
.
3.
J. V.
Jose
and
E. J.
Saletan
,
Classical Dynamics: A Contemporary Approach
(
Cambridge U. P.
,
Cambridge
,
1998
), p.
210
.
4.
D. G.
Currie
,
T. F.
Jordan
, and
E. C. G.
Sudarshan
, “
Relativistic invariance and Hamiltonian theories of interacting particles
,”
Rev. Mod. Phys.
34
,
350
375
(
1963
).
5.
See Ref. 2, pp.
324
and
353
.
6.
S.
Coleman
and
J. H.
Van Vleck
, “
Origin of ‘hidden momentum forces’ on magnets
,”
Phys. Rev.
171
,
1370
1375
(
1968
).
7.
T. H.
Boyer
, “
Illustrations of the relativistic conservation law for the center of energy
,”
Am. J. Phys.
73
,
953
961
(
2005
).
8.
The terminology for “mass” used here corresponds to the usage of
E. F.
Taylor
and
J. A.
Wheeler
,
Spacetime Physics
, 2nd ed. (
Freeman
,
San Francisco
,
2001
), pp.
244
251
, which apparently corresponds to the currently preferred terminology. The word “mass” is now taken to be synonymous with what used to be termed “rest mass,” and many historical uses of the term “mass” are now considered less appropriate. This refinement in terminology requires that the mass of an object is a measure of its energy content only in its center-of-momentum frame. The term “center of mass,” taken to mean what we have termed “center of energy,” is no longer the appropriate terminology. This older terminology appears, for example, in the first edition of
E. F.
Taylor
and
J. A.
Wheeler
,
Spacetime Physics
(
Freeman
,
San Francisco
,
1966
), p.
143
, and in
L. D.
Landau
and
E. M.
Lifshitz
,
Classical Theory of Fields
, 4th ed. (
Pergamon
,
New York
,
1985
), p.
168
. The refined terminology also changes the answers (but not the physics) of various text book problems, such as Epstein and Hewitt’s problem of the streetcar and the motorcycle
[
L. C.
Epstein
and
P. G.
Hewitt
,
Thinking Physics
(
Insight Press
,
San Francisco
,
1981
), pp.
460
461
].
9.
There have been numerical calculations of the energy distributions for colliding particles in a box with reflecting walls. It turns out that a nonrelativistic particle takes on the Maxwell velocity distribution, and the relativistic particle takes on the Jüttner distribution [
F.
Jüttner
, “
Das Maxwellsche Gesetz der Geschwindigkeitsverteilung in der Relativtheorie
,”
Ann. Phys.
34
,
856
882
(
1911
)] in the rest frame of the box, T. H. Boyer (unpublished).
10.
However, this failure is pointed out emphatically by
F.
Rohrlich
,
Classical Charged Particles
(
Addison-Wesley
,
Reading, MA
,
1965
), p.
210
.
11.
This parallel-plate example has been discussed in more detail in Ref. 7 and in
T. H.
Boyer
, “
Relativistic mechanics and a special role for the Coulomb potential
,” arXiv:0810.0434.
12.
Approximately Lorentz-invariant Lagrangians of this form appear in
P.
Havas
and
J.
Stachel
, “
Invariances of approximately relativistic Lagrangians and the center-of-mass theorem. I
,”
Phys. Rev.
185
,
1636
1647
(
1969
), Eq. (46), and
F. J.
Kennedy
, “
Approximately relativistic interactions
,”
Am. J. Phys.
40
,
63
74
(
1972
), Eq. (27). See also
H. W.
Woodcock
and
P.
Havas
, “
Approximately relativistic Lagrangians for classical interacting point particles
,”
Phys. Rev. D
6
,
3422
3444
(
1972
).
13.
See Ref. 2, Secs. 7.9–7.10 and Ref. 3, pp.
209
212
.
14.
See, for example,
R. W.
Brehme
, “
The relativistic Lagrangian
,”
Am. J. Phys.
39
,
275
280
(
1971
).
15.
J. D.
Jackson
,
Classical Electrodynamics
3rd ed. (
Wiley
,
New York
,
1999
), pp.
596
598
. The Darwin Lagrangian is given in Eq. 12.82.
16.
The expressions for the electric and magnetic fields agree with those given by
L.
Page
and
N. I.
Adams
, “
Action and reaction between moving charges
,”
Am. J. Phys.
13
,
141
147
(
1945
).
17.
See Ref. 2, p.
316
, and Ref. 10, pp.
179
181
, where the harmonic oscillator potential is used.
18.
See, for example,
T. H.
Boyer
, “
Blackbody radiation, conformal symmetry, and the mismatch between classical mechanics and electromagnetism
,”
J. Phys. A
38
,
1807
1821
(
2005
), and
T. H.
Boyer
Connecting blackbody radiation, relativity, and discrete charge in classical electrodynamics
,”
Found. Phys.
37
,
999
1026
(
2007
).
19.
The mistaken idea of Lorentz-invariant behavior as a description of nature involving only the use of relativistic mechanical momentum appears in the analysis of blackbody radiation by
R.
Blanco
,
L.
Pesquera
, and
E.
Santos
, “
Equilibrium between radiation and matter for classical relativistic multiperiodic systems. Derivation of Maxwell-Boltzmann distribution from Rayleigh-Jeans spectrum
,”
Phys. Rev. D
27
,
1254
1287
(
1983
), and
R.
Blanco
,
L.
Pesquera
, and
E.
Santos
, “
Equilibrium between radiation and matter for classical relativistic multiperiodic systems. II. Study of radiative equilibrium with Rayleigh-Jeans radiation
,”
Phys. Rev. D
29
,
2240
2254
(
1984
).
AAPT members receive access to the American Journal of Physics and The Physics Teacher as a member benefit. To learn more about this member benefit and becoming an AAPT member, visit the Joining AAPT page.