Soviet Physics Journal

, Volume 28, Issue 10, pp 773–776

Conditions for the appearance of gravitational ultrarelativistic spin-orbital interaction

Authors

  • R. M. Plyatsko
    • Institute for Applied Problems in Mechanics and Mathematics
  • A. L. Vynar
    • Institute for Applied Problems in Mechanics and Mathematics
  • Ya. N. Pelekh
    • Institute for Applied Problems in Mechanics and Mathematics
Elementary-Particle Physics and Field Theory

DOI: 10.1007/BF00897946

Cite this article as:
Plyatsko, R.M., Vynar, A.L. & Pelekh, Y.N. Soviet Physics Journal (1985) 28: 773. doi:10.1007/BF00897946

Abstract

A qualitative analysis of the energy and momentum integrals for the Mathisson-Papapetrou equations in a Schwarzschild field is employed to determine the conditions under which all solutions of the exact Mathisson-Papapetrou equations corresponding to fixed initial coordinate and velocity values differ significantly from the solution of the abbreviated equations normally used for the same initial data. Numerical computer calculations provide additional indication of a difference in the world lines of the exact Mathisson-Papapetrou equations from solutions of the geodesic equations at ultrarelativistic velocity values. For high energy particles entering into the composition of cosmic rays one can expect appearance of gravitational ultrarelativistic spin-orbital interaction upon motion of such particles in the field of a neutron star.

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Copyright information

© Plenum Publishing Corporation 1986