Gravitational acceleration of relativistic particles at finite temperature

Details Gravitational acceleration of relativistic particles at finite temperature Gravitational acceleration of relativistic particles at finite temperature

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..36..617g&link_type=abstract

Physical Review D (Particles and Fields), Volume 36, Issue 2, 15 July 1987, pp.617-619

Physics

3

Scientific paper

Starting from the explicit expression of a generalized energy-momentum tensor, representing the effective source of gravity at finite temperature, it is shown that, in the case of a weak, static field and in the low-temperature limit, the thermal corrections to the gravitational acceleration of a relativistic test particle do not depend on its kinetic energy, and that the only effect is a constant, mass-dependent shift of the gravitational to inertial mass ratio, just as in the case, previously discussed, of nonrelativistic test bodies.

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