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Phase-space symmetries of a relativistic plasma

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Il Nuovo Cimento B (1965-1970)

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References

  1. B. Kursunoglu:Symmetries of a relativistic plasma, to appear in theProc. of the Relativistic Plasma Symposium (New York).

  2. Let us recall that the name «symmetry» is used in elementary-particle physics for denoting a group of transformations able to characterize a physical system.

  3. The no-interaction theorem states that a finite number of classical particles cannot be represented by a theory including interactions if the theory is invariant under the inhomogeneous Lorent group. See, for instance:D. G. Currie, T. F. Jordan andE. C. G. Sudarshan:Rev. Mod. Phys.,35, 350 (1963);H. Leutwyler:Nuovo Cimento,37, 556 (1965);R. N. Hill:Journ. Math. Phys.,8, 201 (1967).

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  12. See ref. (11), pp. 281–291.

  13. For investigation on theSU 3,1 group see, for instance,R. M. Santilli:Nuovo Cimento,51 A, 89 (1967).

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Author notes

  1. R. M. Santilli

    Present address: the Istituto di Fisica dell’Università, Torino

Authors and Affiliations

  1. Center for Theoretical Studies, University of Miami, Coral Gables, Fla.

    R. M. Santilli

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  1. R. M. Santilli
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Additional information

Supported by Air Force Office of Scientific Research Contract no. 1268-67 and National Aero nautics and Space Administration Contract no. NASA NGR 10-007-010.

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Santilli, R.M. Phase-space symmetries of a relativistic plasma. Nuovo Cimento B (1965-1970) 56, 323–326 (1968). https://doi.org/10.1007/BF02710158

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