scholarly journals Perturbative Quantum Analysis and Classical Limit of the Electron Scattering by a Solenoidal Magnetic Field

2009 ◽  
Author(s):  
Gabriela Murguía ◽  
Matías Moreno ◽  
Manuel Torres
Keyword(s):  
Magnetic Field ◽  
Electron Scattering ◽  
Classical Limit ◽  
Quantum Analysis ◽  
Perturbative Quantum

Electron scattering from gas phase cis-diamminedichloroplatinum(II): Quantum analysis of resonance dynamics

2013 ◽  
Vol 138 (20) ◽  
pp. 204308 ◽  
Author(s):  
Ralph Carey ◽  
Robert R. Lucchese ◽  
F. A. Gianturco
Keyword(s):  
Gas Phase ◽  
Electron Scattering ◽  
Quantum Analysis

Electron Scattering Spectroscopy by High Magnetic Field in Mid-Infrared Quantum Cascade Lasers

2007 ◽  
Author(s):  
Aude Leuliet ◽  
Aaron Wade ◽  
Angela Vasanelli ◽  
Georgy Fedorov ◽  
Dmitry Smirnov ◽  
...  
Keyword(s):  
Magnetic Field ◽  
High Magnetic Field ◽  
Electron Scattering ◽  
Quantum Cascade Lasers ◽  
Mid Infrared ◽  
Quantum Cascade ◽  
Cascade Lasers

scholarly journals Modelling the photometric variability of magnetic massive stars with the Analytical Dynamical Magnetosphere model

2019 ◽  
Author(s):  
M S Munoz ◽  
G A Wade ◽  
Y Nazé ◽  
J Puls ◽  
S Bagnulo ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Electron Scattering ◽  
Massive Star ◽  
Massive Stars ◽  
Mass Density ◽  
Magellanic Clouds ◽  
Light Curves ◽  
Photometric Variability ◽  
P Type ◽  
The Magnetic Field

Abstract In this paper, we investigate the photometric variability of magnetic O-type stars. Such stars possess oblique, predominantly dipolar magnetic fields that confine their winds roughly axisymmetrically about the magnetic equator, thus forming a magnetosphere. We interpret their photometric variability as phase-dependent magnetospheric occultations. For massive star winds dominated by electron scattering opacity in the optical and NIR, we can compute synthetic light curves from simply knowing the magnetosphere’s mass density distribution. We exploit the newly-developed Analytical Dynamical Magnetosphere model (ADM) in order to obtain the predicted circumstellar density structures of magnetic O-type stars. The simplicity in our light curve synthesis model allows us to readily conduct a parameter space study. For validation purposes, we first apply our algorithm to HD 191612, the prototypical Of?p star. Next, we attempt to model the photometric variability of the Of?p-type stars identified in the Magellanic Clouds using OGLE photometry. We evaluate the compatibility of the ADM predictions with the observed photometric variations, and discuss the magnetic field properties that are implied by our modelling.

Cyclotron resonance in the extreme anomalous relaxation region

1964 ◽  
Vol 278 (1373) ◽  
pp. 256-273 ◽  
Keyword(s):  
Magnetic Field ◽  
Electron Scattering ◽  
Cyclotron Resonance ◽  
Surface Resistance ◽  
Electron Gas ◽  
Degenerate Semiconductors ◽  
Line Shapes ◽  
Infra Red ◽  
Anomalous Relaxation ◽  
The Magnetic Field

A reformulation of the theory of cyclotron resonance in metals as a variational problem is combined with the exact solution of the Boltzmann equation and used to calculate the surface resistance of an isotropic electron gas, in the extremeanom alous relaxation region, as a function of an applied magnetic field parallel to the surface of the medium . The line shapes obtained depend strongly on the diffuse or specular nature of the electron scattering a t the surface and also on the longitudinal or transverse orientation of the magnetic field relative to the current. The effect should be observable in degenerate semiconductors and semimetals a t infra-red frequencies.

scholarly journals Energy and momentum losses in the process of neutrino scattering on plasma electrons in the presence of a magnetic field

Open Physics ◽  
2003 ◽  
Vol 1 (1) ◽  
Author(s):  
Nickolay Mikheev ◽  
Elena Narynskaya
Keyword(s):  
Magnetic Field ◽  
External Magnetic Field ◽  
Electron Scattering ◽  
Volume Density ◽  
Neutrino Energy ◽  
Magnetized Plasma ◽  
Neutrino Scattering ◽  
Energy And Momentum

AbstractThe neutrino-electron scattering in a dense degenerate magnetized plasma under the conditions μ 2 > 2eB ≫ μE is investigated. The volume density of the neutrino energy and momentum losses due to this process are calculated. The results we have obtained demonstrate that plasma in the presence of an external magnetic field is more transparent for neutrino than for non-magnetized plasma. It is shown that neutrino scattering under conditions considered does not lead to the neutrino force acting on plasma.

Sign in / Sign up

Export Citation Format

Share Document