Polarized light propagation and scattering in random media

2001 ◽  
Author(s):  
Arnold D. Kim ◽  
Sermsak Jaruwatanadilok ◽  
Akira Ishimaru ◽  
Yasuo Kuga
Keyword(s):  
Random Media ◽  
Light Propagation ◽  
Polarized Light

scholarly journals On spacetime structure and electrodynamics

2016 ◽  
Vol 25 (11) ◽  
pp. 1603001
Author(s):  
Wei-Tou Ni
Keyword(s):  
Constitutive Relation ◽  
Degrees Of Freedom ◽  
Light Propagation ◽  
Wave Packets ◽  
Polarization State ◽  
Polarized Light ◽  
Continuous Media ◽  
Weak Field ◽  
Degree Of Freedom ◽  
Intermediate Boson

Electrodynamics is the most tested fundamental physical theory. Relativity arose from the completion of Maxwell–Lorentz electrodynamics. Introducing the metric [Formula: see text] as gravitational potential in 1913, versed in general (coordinate-)covariant formalism in 1914 and shortly after the completion of general relativity, Einstein put the Maxwell equations in general covariant form with only the constitutive relation between the excitation and the field dependent on and connected by the metric in 1916. Further clarification and developments by Weyl in 1918, Murnaghan in 1921, Kottler in 1922 and Cartan in 1923 together with the corresponding developments in electrodynamics of continuous media by Bateman in 1910, Tamm in 1924, Laue in 1952 and Post in 1962 established the premetric formalism of electrodynamics. Since almost all phenomena electrodynamics deal with have energy scales much lower than the Higgs mass energy and intermediate boson energy, electrodynamics of continuous media should be applicable and the constitutive relation of spacetime/vacuum should be local and linear. What is the key characteristic of the spacetime/vacuum? It is the Weak Equivalence Principle I (WEP I) for photons/wave packets of light which states that the spacetime trajectory of light in a gravitational field depends only on its initial position and direction of propagation, and does not depend on its frequency (energy) and polarization, i.e. nonbirefringence of light propagation in spacetime/vacuum. With this principle it is proved by the author in 1981 in the weak field limit, and by Lammerzahl and Hehl in 2004 together with Favaro and Bergamin in 2011 without assuming the weak-field condition that the constitutive tensor must be of the core metric form with only two additional degrees of freedom — the pseudoscalar (Abelian axion or EM axion) degree of freedom and the scalar (dilaton) degree of freedom (i.e. metric with axion and dilaton). In this paper, we review this connection and the ultrahigh precision empirical tests of nonbirefringence together with present status of tests of cosmic Abelian axion and dilaton. If the stronger version of WEP is assumed, i.e. WEP II for photons (wave packets of light) which states in addition to WEP I also that the polarization state of the light would not change (e.g. no polarization rotation for linear polarized light) and no amplification/attenuation of light, then no Abelian (EM) axion and no dilaton, and we have a pure metric theory.

Some features of light propagation in statistically anisotropic random media

2000 ◽  
Author(s):  
Alexander I. Saichev ◽  
Vladimir G. Gavrilenko ◽  
Evgeniya Z. Gribova ◽  
Andrey V. Aistov
Keyword(s):  
Random Media ◽  
Light Propagation

Cloud-based online application for imitation of polarized light propagation in turbid scattering media

2020 ◽  
Author(s):  
Alexander Doronin ◽  
Hee Ryung Lee ◽  
Igor Meglinski ◽  
Alexander Bykov ◽  
Tatiana Novikova
Keyword(s):  
Light Propagation ◽  
Polarized Light ◽  
Scattering Media ◽  
Online Application
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