This paper investigates the axiom that the photon’s probability distribution is a Gaussian distribution. The Airy disc empirical evidence shows that the best fit, if not exact, distribution is a modified Gamma mΓ distribution (whose parameters are ) in the plane orthogonal to the motion of the photon. This modified Gamma distribution is then used to reconstruct the probability distributions along the hypotenuse from the pinhole, arc from the pinhole, and a line parallel to photon motion. This reconstruction shows that the photon’s probability distribution is not a Gaussian function. However, under certain conditions, the distribution can appear to be Normal, thereby accounting for the success of quantum mechanics. This modified Gamma distribution changes with the shape of objects around it and thus explains how the observer alters the observation. This property therefore places additional constraints to quantum entanglement experiments. This paper shows that photon interaction is a multi‐phenomena effect consisting of the probability to interact the probabilistic function and the ability to interact the electromagnetic function. Splitting the probability function from the electromagnetic function enables the investigation of the photon behavior from a purely probabilistic perspective. The Probabilistic Interaction Hypothesis is proposed as a consistent method for handling the two different phenomena, the probability function and the ability to interact thus redefining radiation shielding, stealth or cloaking, and invisibility as different effects of a single phenomenon of the photon probability distribution. Sub wavelength photon behavior is successfully modeled as a multi‐phenomena behavior. The Probabilistic Interaction Hypothesis provides a good fit to Otoshi’s (1972) microwave shielding, Schurig et al. (2006) microwave cloaking, and Oulton et al. (2008) sub wavelength confinement; thereby providing a strong case that the photon probability distribution is a modified Gamma mΓ distribution and not a Gaussian distribution.
Non‐Gaussian Photon Probability Distribution
SPACE, PROPULSION & ENERGY SCIENCES INTERNATIONAL FORMUM SPESIF‐2010: 14th Conference on Thermophysics Applications in Microgravity 7th Symposium on New Frontiers in Space Propulsion Sciences 2nd Symposium on Astrosociology 1st Symposium on High Frequency Gravitational Waves ; 2010 ; Huntsville (Alabama)
AIP Conference Proceedings ; 1208 , 1 ; 261-273
28.01.2010
13 pages
Aufsatz (Konferenz)
Elektronische Ressource
Englisch
Gaussian Probability Distribution Plots
AIAA | 1988
|Non-Gaussian Collision Probability (AAS 13-908)
British Library Conference Proceedings | 2014
|Collision Probability with Gaussian Mixture Orbit Uncertainty
Online Contents | 2014
|