A study on black-body radiation: classical and binary photons

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dc.creatorVarro, Sandor
dc.date2006-11-01
dc.date.accessioned2026-07-07T07:40:11Z
dc.date.available2026-07-07T07:40:11Z
dc.descriptionThe present study gives a detailed analysis of the black-body radiation based on classical random variables. It is shown that the energy of a mode of a chaotic radiation field (Gauss variable) can be uniquely decomposed into a sum of a discrete variable (Planck variable having the Planck-Bose distribution) and a continuous dark variable (with a truncated exponential distribution of finite support). The Planck variable is decomposed, on one hand, into a sum of binary variables representing the binary photons of energies 2^s*h*nu with s=0,1,2,etc. In this way the black-body radiation can be viewed as a mixture of thermodinamically independent fermion gases. The Planck variable can also be decomposed into a sum of independent Poisson components representing the classical photo-molecules of energies m*h*nu with m=1,2,3,etc. These classical photons have only particle-like fluctuations, on the other hand, the binary photons have wave-particle fluctuations of fermionic character.
dc.description20 pages
dc.identifierhttps://arxiv.org/abs/quant-ph/0611010
dc.identifierhttp://arxiv.org/abs/quant-ph/0611010
dc.identifierActa Physica Hungarica B, Vol. 26, pp 365-389 (2006)
dc.identifierdoi:10.1556/APH.26.2006.3-4.18
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121702
dc.subjectQuantum Physics
dc.titleA study on black-body radiation: classical and binary photons
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