Abstract
Directly interacting particles are considered in the multitime formalism of predictive relativistic mechanics. When the equations of motion leave a phase-space volume invariant, it turns out that the phase average of any first integral, covariantly defined as a flux across a 7n-dimensional surface, is conserved. The Hamiltonian case is discussed, a class of simple models is exhibited, and a tentative definition of equilibrium is proposed.
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A start to covariant theory was given by A. Lichnerowicz and R. Marriot,Compt. Rend. Acad. Sci. (Paris) 210, 759 (1940).
R. Hakim,J. Math. Phys. 8, 1315 (1967).
W. Israel and H. E. Kandrup,Ann. Phys. (N.Y.) 152, 30–84 (1984). These authors have explicity stated that the gravitational forces at work between “particles” should be modeled by direct interactions, and they cared to considern-dimensional world sheets in an 8n-dimensional phase space.
J. A. Wheeler and R. P. Feynman,Rev Mod. Phys. 17, 157 (1945).
H. Van Dam and E. P. Wigner,Phys. Rev. B 138, 1576 (1965).
Relativistic Action at a distance. Classical and Quantum Aspects, Llosa, ed. (Lecture Notes in Physics162) (Springer, New York, 1982).
Ph. Droz-Vincent,Lett Nuovo Cimento 1, 839 (1969);Phys. Scri. 2, 129 (1970).
Ph. Droz-Vincent,Rep Math Phys. 8, 79 (1975);Ann. Inst. H. Poincaré A 32, 317 (1980).
This scheme could be extended to second-order derivatives in order to take radiation into account along the lines of R. Hakim,J. Math. Phys. 8, 1379 (1967).
Along the lines of R. N. Hill and E. H. Kerner,Phys. Rev. Lett. 17, 1156 (1966), L. Bel has proposed an alternative version of predictive mechanics which is not manifestly covariant (although relativistically invariant) and will not be discussed here:Ann. Inst. Henri Poincaré A 12, 307 (1970);14, 189 (1971). In contrast, H. P. Künzle has considered a generalization of the covariant formalism:J. Math. Phys. 15, 1033 (1974). This extension is tremendously complicated for our purpose.
R. Lapiedra and E. Santos,Phys. Rev. D 23, 2181–2188 (1981).
L. P. Horwitz and C. Piron,Helv. Phys. Acta 46, 316 (1973).
L. P. Horwitz, W. C. Schieve, and C. Piron,Ann. Phys. 137, 306 (1981), L. P. Horwitz, S. Shashoua, and W. C. Schieve,Physica A 161, 300 (1989). L. Burakovsky and L. P. Horwitz,Physica A 201, 666 (1993).
P. G. Bergmann,Phys. Rev. 84 1026 (1951).
R. Abraham and J. E. Marsden,Foundations of Mechanics, 2nd edn. (Addison-Wesley, Reading, 1978), Chap. 2, exercise 2.4B, p. 121.
For the two-body case see, for instance, R. Arens,Nuovo Cimento B 21, 395 (1974). Here, the formula with two wedges is a short-hand notation for a pseudo-vector in space-time.
Ph. Droz-Vincent, Contribution toDifferential Geometry and Relativity, M. Cahen and M. Flato, eds. Reidel, Dordrecht, 1976).
Ph. Droz-Vincent,Ann. Inst. Henri Poincaré A 27, 407 (1977).
L. Lusanna,Nuovo Cimento A 64, 65–88 (1981).
I. T. Todorov, JINR Report, E2-10125, Dubna (1976); see also contribution to Ref. 6. V.V. Molotkov and I. T. Todorov,Commun. Math. Phys. 79, 111 (1981).
U. Ben-Ya'acov, “Irreversibility in relativistic statistical mechanics,”Mod. Phys. Lett. B 8, 1847–1860 (1994).
W. Hunziker,Commun. Math. Phys. 8, 282 (1968). This author assumes a Hamiltonian formalism; this technical assumption is not conceptually required, though it seems to be necessary in order to derive the results.
Ph. Droz-Vincent,Nuovo Cimento A 58, 365 (1980).
L. P. Horwitz and F. Rohrlich,Phys. Rev. D 24, 1528 (1981).
D. G. Currie, T. F. Jordan and E. C. G. Sudarshan,Rev. Mod. Phys. 35, 350, 1030 (1963), H. Leutwyler,Nuovo Cimento 37, 556 (1965).
Ph. Droz-Vincent,Found. Phys. 25, 67 (1995).
L. Bel and X. Fustero, “Mécanique relativiste prédictive des systèmes deN particules,”Ann. Inst. Henri Poincaré A 25, 411–436 (1976).
In relativistic mechanics HJ coordinates have been considered first in the two-body problem, with asymptotic conditions in time by L. Bel and J. Martin,Ann. Inst. Henri Poincaré A 22, 173–199 (1975) Later we advocated the use of HJ coordinates for the explicit construction of two-body (see Ref. 18) andn-body interactions: Ph. Droz-Vincent,C. R. Acad Sci. (Paris) 299 II, 139 (1984). Construction of relativistic interactions by a map to free motion was also considered without Hamiltonians by R. Arens, contributions in Ref. 6, p. 1.
X. Barcons and R. Lapiedra,Phys. Rev. 28, 3030 (1983).
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Invited paper, dedicated to Prof. Lawrence P. Horwitz on the occasion of his 65th birthday, October 14, 1995.
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Droz-Vincent, P. Direct interactions in relativistic statistical mechanics. Found Phys 27, 363–387 (1997). https://doi.org/10.1007/BF02550162
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DOI: https://doi.org/10.1007/BF02550162