On the finite-temperature quantum electrodynamics of gravitational acceleration

Details On the finite-temperature quantum electrodynamics of gravitational acceleration On the finite-temperature quantum electrodynamics of gravitational acceleration

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..40.4096b&link_type=abstract

Physical Review D (Particles and Fields), Volume 40, Issue 12, 15 December 1989, pp.4096-4099

Physics

Condensed Matter

Statistical Mechanics

3

Specific Calculations, Other Topics In General Relativity And Gravitation, Quantum Statistical Mechanics

Scientific paper

The temperature-dependent quantum-electrodynamic corrections to the Helmholtz free energy F of a particle at rest, and to its inertial mass minert, are the same: ΔF=Δminert=πe2(kT)2/3m. By contrast, the correction to the total energy U=F+TS is ΔU=-ΔF. Donoghue, Holstein, and Robinett have pointed out that if (as the equivalence principle appears to imply) weight is proportional to total energy, then the gravitational acceleration of a particle inside a blackbody cavity becomes g(m+ΔU)/(m+ΔF)~=g(1-2ΔF/m)

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