Faraday rotation in a disordered medium
نویسندگان
چکیده
The Faraday rotation angle is calculated in a diffusive regime on a three-dimensional disordered slab. It is shown that tan is (i) an oscillating function of the magnetic field or the medium’s internal properties, and (ii) proportional to the ratio of the inelastic mean-free path lin to the mean-free path l, that is, to the average number of photon scatterings. The maximum rotation is achieved at frequencies when the photon’s elastic mean-free path is minimal. We have obtained the rotation angle of backscattered light taking into account the maximally crossed diagrams. The latter leads to an ellipticity in the backscattered wave that can serve as a precursor of weak localization. The critical strength of the magnetic field is Bc ∼ gc ∼ λ/l beyond which rotation in the backscattered wave disappears. The traversal time of an electromagnetic wave through the slab is estimated in a diffusive regime. The disorder enhanced the traversal time by an additional factor lin/l in comparison with a free light propagation time. Comparison with the experimental data is carried out.
منابع مشابه
خواص نوری- مغناطیسی و ضرایب اپتیکی لایههای نازک منگنز-کبالت
Having precise hysterics loop of thin ferroelectric and ferromagnetic layers for optical switching and optical storages are important. A hysterieses loop can be achieved from a phenomenon call the magneto-optic effect. The magneto-optic effect is the rotation of a linear polarized electromagnetic wave propagated through a ferromagnetic medium. When light is transmitted through a layer of magnet...
متن کاملDetermination of Linear Polarization and Faraday Rotation of Pulsar Signals from Spectral Intensity Modulation
Most of the known pulsars are sources of highly linearly polarized radiation. Faraday rotation in the intervening medium rotates the plane of the linear polarization as the signals propagate through the medium. The Rotation Measure (RM), which quantifies the amount of such rotation as a function of wavelength, is useful in studying the properties of the medium and in recovering the intrinsic po...
متن کاملAntisymmetry in the Faraday Rotation Sky Caused by a Nearby Magnetized Bubble
Rotation measures of pulsars and extragalactic point sources have been known to reveal largescale antisymmetries in the Faraday rotation sky with respect to the Galactic plane and halo that have been interpreted as signatures of the mean magnetic field in the Galactic halo. We describe Faraday rotation measurements of the diffuse Galactic polarized radio emission over a large region in the nort...
متن کاملGraphene-based photonic crystal to steer giant Faraday rotation
Related Articles All-optical tuning of a quantum dot in a coupled cavity system Appl. Phys. Lett. 100, 231107 (2012) Cherenkov high-order harmonic generation by multistep cascading in χ(2) nonlinear photonic crystal Appl. Phys. Lett. 100, 221103 (2012) Partially disordered photonic-crystal thin films for enhanced and robust photovoltaics Appl. Phys. Lett. 100, 181110 (2012) Control of absorptio...
متن کاملCharacteristics of the Galactic magneto-ionized ISM from Faraday rotation
Faraday rotation measurements of polarized extragalactic sources probe the Galactic magnetized, ionized interstellar medium. Rotation measures of these sources behind the inner Galactic plane are used to explore characteristics of the structure in the spiral arms and in interarm regions. Structure in the spiral arms has a characteristic outer scale of a few parsecs only, whereas interarm region...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2013