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// Workers AI · dad joke modeWhat did no-interaction theorem say to its date? You don't interact with me.

From Wikipedia, the free encyclopedia

In classical mechanics, the no-interaction theorem is a no-go theorem that shows that a system of many interacting particles cannot exist when special relativity is taken into account. It concludes that the only allowed configuration is that of a system of free particles only. The theorem is important for modern physics, as it suggest the necessity of introducing fields to describe interactions between particles. This theorem excludes the possibility of action at a distance. The modern understanding of the fundamental interactions (gravity, electromagnetism and nuclear forces) is that objects can interact by locally perturbing the fields in which each interaction propagates.

Various formulations of the theorem exist. The earliest version was given by Douglas G. Currie, Thomas F. Jordan and E. C. George Sudarshan in 1963,[1] extended by John T. Cannon and Jordan in 1964,[2] and generalized by Heinrich Leutwyler in 1965.[3] An alternative formulation was given by Hendrik van Dam and Eugene Wigner[4] in 1966.[5][6][7]

Assumptions

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Consider a system with a finite number N of particles described by special relativity using Lagrangian or Hamiltonian mechanics. The no-interaction theorem states that, aside from contact forces, there can be no direct interaction between any two particles in a form that is manifestly invariant under Lorentz transformations (covariant).[6][8] The theorem can be explicitly shown using three postulates:

  1. Conservation of total linear momentum: the total four-momentum at a given time is expressed as , where is the four-momentum of particle . The postulate assumes that at any time.
  2. No coincidence: there are no two distinct particles and with proper times such that .
  3. Asymptotically straight world lines: for large times, , .

which leads to the momentum of individual particles being constant (no interactions) at any time. The third postulate implies that the total momentum transforms under Lorentz transformations.[9]

More advanced proofs rely on group theoretical arguments.[10][9]

Case of two identical particles

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The no-interaction theorem indicates that two classical particles of mass cannot interact. If is the four-velocity of particle 1 and the four-velocity of particle 2, the total momentum is[7]In another frame, the four-momentum transforms asfor some Lorentz boost .

Van Dam and Wigner prove by contradiction that momentum is not conserved unless the particles come into contact.[7] Supposing particle 1 is at point P at time and also at point P at time (following its world line), and particle 2 is at point Q at and at Q' at , the transformation of the total momentum is given by but as the four-velocity at point P also transforms as and at point Q asas is arbitrary we conclude that meaning that the velocity of particle 2 remains constant when moving from Q to Q'. This result implies that the momentum of each particle remains constant, which is only possible if the particles did not interact.

References

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  1. Currie, D. G.; Jordan, T. F.; Sudarshan, E. C. G. (1963-04-01). "Relativistic Invariance and Hamiltonian Theories of Interacting Particles". Reviews of Modern Physics. 35 (2): 350–375. doi:10.1103/RevModPhys.35.350. ISSN 0034-6861. Archived from the original on 2026-02-08.
  2. Cannon, John T.; Jordan, Thomas F. (1964-03-01). "A No-Interaction Theorem in Classical Relativistic Hamiltonian Particle Dynamics". Journal of Mathematical Physics. 5 (3): 299–307. doi:10.1063/1.1704121. ISSN 0022-2488.
  3. Leutwyler, H. (1965-05-01). "A no-interaction theorem in classical relativistic Hamiltonian particle mechanics". Il Nuovo Cimento (1955-1965). 37 (2): 556–567. doi:10.1007/BF02749856. ISSN 1827-6121.
  4. Van Dam, H.; Wigner, E. P. (1965-06-21). "Classical Relativistic Mechanics of Interacting Point Particles". Physical Review. 138 (6B): B1576–B1582. doi:10.1103/PhysRev.138.B1576. ISSN 0031-899X. Archived from the original on 2024-07-12.
  5. Marmo, G.; Samuel, J.; Simoni, A.; Zaccaria, F. (1988-10-01). "No-interaction theorem for classical relativistic particles with Grassmann internal coordinates". Il Nuovo Cimento A (1965-1970). 100 (4): 447–461. doi:10.1007/BF02789492. ISSN 1826-9869.
  6. 1 2 Williams, Anthony G. (2022-08-04). Introduction to Quantum Field Theory: Classical Mechanics to Gauge Field Theories. Cambridge University Press. ISBN 978-1-108-60087-3.
  7. 1 2 3 Ohanian, Hans C. (1976). Gravitation and spacetime. Internet Archive. New York : Norton. ISBN 978-0-393-09198-4.{{cite book}}: CS1 maint: publisher location (link)
  8. Goldstein, Herbert; Poole, Charles P.; Safko, John L. (2002). Classical Mechanics. Addison Wesley. ISBN 978-0-201-65702-9.
  9. 1 2 Mann, Ronald A. (2013-10-22). The Classical Dynamics of Particles: Galilean and Lorentz Relativity. Academic Press. ISBN 978-1-4832-6201-7.
  10. Esposito, Giampiero; Marmo, Giuseppe; Sudarshan, George (2004-03-11). From Classical to Quantum Mechanics: An Introduction to the Formalism, Foundations and Applications. Cambridge University Press. ISBN 978-1-139-45054-6.