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Optical polarization

About: Optical polarization is a research topic. Over the lifetime, 13992 publications have been published within this topic receiving 244284 citations.


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Journal ArticleDOI
TL;DR: Mesures obtenues avec le polarimetre de l'observatoire de Meudon, appliquees sur des surfaces, including echantillons de roches et de poudres, des meteorites, des echantillon lunaires and des corps planetaires without atmosphere as discussed by the authors.
Abstract: Mesures obtenues avec le polarimetre de l'observatoire de Meudon, appliquees sur des surfaces incluant des echantillons de roches et de poudres, des meteorites, des echantillons lunaires et des corps planetaires sans atmosphere

68 citations

Proceedings ArticleDOI
20 Jun 2005
TL;DR: This work employs a polarization raytracing method to compute both the path of the light and its polarization state, and proposes an iterative computation method that estimates the surface shape of the transparent object by minimizing the difference between the polarization data rendered by the polarization ray Tracing method and the polarized data obtained from a real object.
Abstract: We propose a novel method for estimating the surface shapes of transparent objects by analyzing the polarization state of the light. Existing methods do not fully consider the reflection, refraction, and transmission of the light occurring inside a transparent object. We employ a polarization raytracing method to compute both the path of the light and its polarization state. Our proposed iterative computation method estimates the surface shape of the transparent object by minimizing the difference between the polarization data rendered by the polarization raytracing method and the polarization data obtained from a real object.

68 citations

Journal ArticleDOI
TL;DR: In this article, numerical hydrodynamics simulations are presented of X-ray heated winds believed to form the "mirrors" which reflect light from obscured Seyfert galaxy nuclei into our line of sight.
Abstract: Numerical hydrodynamics simulations are presented of X-ray heated winds believed to form the 'mirrors' which reflect light from obscured Seyfert galaxy nuclei into our line of sight. Above a likely range of parameters, it is shown that steady state flows are created when a cool torus surrounds an AGN. Some of the mass evaporated off the inner edge of the torus is captured by the central gravitational well, while the rest is driven off in a warm wind. When the central gravity is strong relative to the radiative heating rate, i.e., L/L(E) is small, nearly all the injected matter is captured. When the gravity is weaker, a given combination of heating rate and injected pressure leads to a maximum mass loss rate; when the rate at which mass is injected exceeds this amount, the excess is captured. The dividing line between these two cases comes at L/L(E) = about 0.08.

68 citations

Journal ArticleDOI
TL;DR: In this article, a complex set of optical phenomena linked to the spin dynamics of exciton polaritons in semiconductor microcavities are addressed, including pump energy, pumping intensity and polarization.
Abstract: In this chapter we address a complex set of optical phenomena linked to the spin dynamics of exciton polaritons in semiconductor microcavities. When optically created, polaritons inherit the spin and dipole moment from the exciting light. Their state can be fully characterized by a so-called pseudospin accounting for both spin and dipole moment orientation. However, from the very beginning of their life in a microcavity, polaritons start changing their pseudospin state under effect of effective magnetic fields of different nature and due to scattering with acoustic phonons, defects, and other polaritons. This makes pseudospin dynamics of exciton polaritons rich and complex. It manifests itself in non-trivial changes in polarization of light emitted by the cavity versus time, pumping energy, pumping intensity and polarization. During the first years of theoretical research on exciton-polariton relaxation the polarization has been simply neglected. Later it has been understood that the energy and momentum-relaxation of exciton polaritons are spin-dependent. It is typically the case in the regime of stimulated scattering when the spin polarizations of initial and final polariton state have a huge effect on the scattering rate between these states. It appeared that critical conditions for polariton Bose-condensation are also polarization-dependent. In particular, the stimulation threshold (i.e. the pumping power needed to have a population exceeding 1 at the ground state of the lower polariton branch) has been experimentally shown to be lower under linear than under circular pumping. These experimental observations have stimulated the theoretical research toward understanding of mutually dependent polarization- and energy-relaxation mechanisms in microcavities. The authors of this chapter have been working on theoretical description of different specific effects of polariton spin-dynamics in microcavities for years. Here we attempted to put together all fragments and to formulate a general approach to the problem that would allow then to consider a variety of particular cases. We start from reminding the main spin-relaxation mechanisms known for free carriers and excitons. We then overview the most essential experimental results in this field before to present our original formalism which allowed us to interpret the key experimental findings. We are going to discuss only the strong coupling regime leaving aside all polarization effects in VCSELs.

68 citations

Journal ArticleDOI
TL;DR: D density functional theory calculations of the N- V- system are conducted and for the first time a quantitatively accurate picture of the optical transition energy, excited-state lifetime, and optical polarization anisotropy is produced taking into account all possible transitions within all contributing energy bands.
Abstract: Despite tremendous activity in employing the $N\ensuremath{-}{V}^{\ensuremath{-}}$ center in a host of quantum technology applications, the electronic and optical properties of the system are still not theoretically well understood. We have conducted density functional theory calculations of the $N\ensuremath{-}{V}^{\ensuremath{-}}$ system which show convergence at the $3\ifmmode\times\else\texttimes\fi{}3\ifmmode\times\else\texttimes\fi{}3$ supercell level and for the first time produce a quantitatively accurate picture of the optical transition energy, excited-state lifetime, and optical polarization anisotropy taking into account all possible transitions within all contributing energy bands. These calculations were augmented by a group theoretical analysis, in sum providing a new ab initio understanding of this important solid-state quantum system.

68 citations


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Performance
Metrics
No. of papers in the topic in previous years
YearPapers
20221
2021404
2020359
2019318
2018470
2017504