Radiative transfer theory for vacuum fluctuations

dc.creatorMishchenko, E. G.
dc.creatorBeenakker, C. W. J.
dc.date1999-07-06
dc.date1999-10-01
dc.date.accessioned2026-07-07T03:13:50Z
dc.date.available2026-07-07T03:13:50Z
dc.descriptionA semiclassical kinetic theory is presented for the fluctuating photon flux emitted by a disordered medium in thermal equilibrium. The kinetic equation is the optical analog of the Boltzmann-Langevin equation for electrons. Vacuum fluctuations of the electromagnetic field provide a new source of fluctuations in the photon flux, over and above the fluctuations due to scattering. The kinetic theory in the diffusion approximation is applied to the super-Poissonian noise due to photon bunching and to the excess noise due to beating of incident radiation with the vacuum fluctuations.
dc.description4 pages, 2 figures, revised version according to referee's comments
dc.identifierhttps://arxiv.org/abs/cond-mat/9907080
dc.identifierhttp://arxiv.org/abs/cond-mat/9907080
dc.identifierPhys. Rev. Lett. 83, 5475 (1999)
dc.identifierdoi:10.1103/PhysRevLett.83.5475
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/29454
dc.subjectMesoscale and Nanoscale Physics
dc.subjectQuantum Physics
dc.titleRadiative transfer theory for vacuum fluctuations
dc.typetext

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