Definitions of the degree of polarization of a light beam

Author(s):  
Asma Al-Qasimi ◽  
Daniel James ◽  
Olga Korotkova ◽  
Emil Wolf
Author(s):  
Mayukh Lahiri ◽  
Armin Hochrainer ◽  
Gabriela B. Lemos ◽  
Radek Lapkiewicz ◽  
Anton Zeilinger

1997 ◽  
Vol 502 ◽  
Author(s):  
R. W. Collins ◽  
Joungchel Lee ◽  
P. I. Rovira ◽  
Ilsin An

ABSTRACTA multichannel spectroscopic ellipsometer based on the rotating-compensator principle was developed and applied to characterize nanocrystalline diamond thin film growth processes by plasma-enhanced chemical vapor deposition (PECVD). With the newly-designed instrument, a time resolution of 32 ms is possible for spectra (1.5˜4.0 eV) in the Stokes vector of the light beam reflected from the surface of the growing film. Several advantages of the rotating-compensator over the simpler rotating-polarizer multichannel ellipsometer design are demonstrated here for diamond thin film growth. These include the ability to: (i) resolve the sign ambiguity in the p–s wave phase-shift difference Δ, (ii) obtain accurate Δ values for low ellipticity polarization states, and (iii) deduce spectra in the degree of polarization of the light beam reflected from the film/substrate. The degree of polarization has been applied to characterize the time evolution of light scattering during the nucleation of the diamond, as well as the time evolution of thickness non-uniformity over the probed area of the growing film. In this paper, a brief description of calibration and data reduction for the new instrument is also provided.


2017 ◽  
Vol 42 (15) ◽  
pp. 2898 ◽  
Author(s):  
Noé Ortega-Quijano ◽  
Julien Fade ◽  
François Parnet ◽  
Mehdi Alouini

2016 ◽  
Vol 30 (06) ◽  
pp. 1650055 ◽  
Author(s):  
Namrata Shukla ◽  
Ranjana Prakash

We study polarization squeezing of a light beam initially in the coherent state using the nonlinear interaction Hamiltonian [Formula: see text]. For the degree of polarization squeezing, we use a definition written in the final form by the authors and also used in earlier papers. We find that the polarization squeezing can be very high and the degree of polarization squeezing can be less than unity by a very small amount. We achieve the polarization squeezing even for very low beam intensity under some conditions involving phase angles in the polarization modes.


Crystals ◽  
2019 ◽  
Vol 9 (8) ◽  
pp. 387 ◽  
Author(s):  
Paweł Marć ◽  
Noureddine Bennis ◽  
Anna Spadło ◽  
Aleksandra Kalbarczyk ◽  
Rafał Węgłowski ◽  
...  

Polarization is a very useful parameter of a light beam in many optical measurements. Improvement of holographic systems requires optical elements which need a diffused and depolarized light beam. This paper describes a simple monochromatic depolarizer based on a pure vertically aligned liquid crystal without pretilt. In this work we present an extended description of depolarizer by analyzing its electro-optic properties measured in spatial and time domains with the use of crossed polarizers and polarimetric configurations. Crossed polarizers set-up provides information on spatial and temporal changes of microscopic textures while polarimetric measurement allows to measure voltage and time dependence of degree of polarization. Three different thicknesses, i.e., 5 μm, 10 μm and 15 μm have been manufactured in order to analyze another degree of freedom for this type of depolarizer device based on a liquid crystals’ material. Consideration of the light scattering capability of the cell is reported.


2007 ◽  
Vol 32 (9) ◽  
pp. 1015 ◽  
Author(s):  
Asma Al-Qasimi ◽  
Olga Korotkova ◽  
Daniel James ◽  
Emil Wolf

1977 ◽  
Vol 8 (6) ◽  
pp. 373-384 ◽  
Author(s):  
J Badoz ◽  
M Billardon ◽  
J C Canit ◽  
M F Russel

1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.


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