Non-Gaussian Photon Probability Distribution
Description
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 α = r, βr/√(u)) 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 Pi, the probabilistic function and the ability to interact Ai, the electromagnetic function. Splitting the probability function Pi from the electromagnetic function Ai enables the investigation of the photon behavior from a purely probabilistic Pi perspective. The Probabilistic Interaction Hypothesis is proposed as a consistent method for handling the two different phenomena, the probability function Pi and the ability to interact Ai, thus redefining radiation shielding, stealth or cloaking, and invisibility as different effects of a single phenomenon Pi 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.
Additional details
Identifiers
- DOI
- 10.1063/1.3326254;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1208
- Journal Issue
- 1
- Journal Page Range
- p. 261-273
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 14. conference on thermophysics applications in microgravity; 7. symposium on new frontiers in space propulsion sciences; 2. symposium on astrosociology; 1. symposium on high frequency gravitational waves
- Acronym
- SPESIF-2010
- Dates
- 24-26 Feb 2009
- Place
- Huntsville, AL (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41101392
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DISTRIBUTION; GAUSS FUNCTION; MICROWAVE RADIATION; PARTICLE INTERACTIONS; PHOTONS; PROBABILISTIC ESTIMATION; PROBABILITY; QUANTUM ENTANGLEMENT; QUANTUM GROUPS; QUANTUM MECHANICS; SHIELDING; WAVELENGTHS
- Descriptors DEC
- BOSONS; CALCULATION METHODS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FUNCTIONS; INTERACTIONS; MASSLESS PARTICLES; MECHANICS; RADIATIONS; SYMMETRY GROUPS
Optional Information
- Notes
- (c) 2010 American Institute of Physics