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The relativistic kinetic equations describing time evolution and space dependence of the density matrices of polarized photons and electrons interacting via Compton scattering are deduced from the quantum Liouville equation. The induced…

天体物理学 · 物理学 2009-11-07 Dmitrij I. Nagirner , Juri Poutanen

Accounting for all the relativistic effects, we have developed the fully nonlinear gauge-invariant formalism for describing the cosmological observables and presented the second-order perturbative expressions associated with light…

宇宙学与河外天体物理 · 物理学 2022-10-03 Matteo Magi , Jaiyul Yoo

We provide a linear analysis on normal modes of the spin Boltzmann equation proposed in \cite{Weickgenannt:2021cuo}, where the non-diagonal or polarized part of the transition rate is neglected to ensure the Hermitian property of linearized…

高能物理 - 唯象学 · 物理学 2022-08-17 Jin Hu

The angular distribution of the emitted electrons, following the two--photon ionization of the hydrogen--like ions, is studied within the framework of second order perturbation theory \textit{and} the Dirac equation. Using a density matrix…

原子物理 · 物理学 2007-05-23 Peter Koval , Stephan Fritzsche , Andrey Surzhykov

We study the electron as a system composed by an electron and a photon, using lowest order perturbation theory. We derive the leading-twist transverse-momentum-dependent distribution functions for both the electron and photon in the dressed…

高能物理 - 唯象学 · 物理学 2016-01-20 Alessandro Bacchetta , Luca Mantovani , Barbara Pasquini

A novel covariant formalism for the treatment of the transfer and Compton scattering of partially polarized light is presented. This was initially developed to aid in the computation of relativistic corrections to the polarization generated…

天体物理学 · 物理学 2016-08-30 Jamie Portsmouth , Edmund Bertschinger

This paper presents an overview of the radiative transfer problem of calculating the spectral line intensity and polarization that emerges from a (generally magnetized) astrophysical plasma composed of atoms and molecules whose excitation…

太阳与恒星天体物理 · 物理学 2015-05-14 J. Trujillo Bueno

After an introduction to the problem of cosmological structure formation, we develop gauge invariant cosmological perturbation theory. We derive the first order perturbation equations of Einstein's equations and energy momentum…

天体物理学 · 物理学 2010-12-09 Ruth Durrer

We consider a system of non-interacting charged particles moving in two dimensions among fixed hard scatterers, and acted upon by a perpendicular magnetic field. Recollisions between charged particles and scatterers are unavoidable in this…

凝聚态物理 · 物理学 2007-05-23 A. V. Bobylev , Alex Hansen , J. Piasecki , E. H. Hauge

This is the second of two papers in which we study real and virtual photon-proton scattering in a nonperturbative framework. In the first paper we have identified the leading contributions to this process at high energies and have derived…

高能物理 - 唯象学 · 物理学 2008-11-26 Carlo Ewerz , Otto Nachtmann

Consider the linear Boltzmann equation of radiative transfer in a half-space, with constant scattering coefficient $\sigma$. Assume that, on the boundary of the half-space, the radiation intensity satisfies the Lambert (i.e. diffuse)…

偏微分方程分析 · 数学 2018-09-18 Claude Bardos , François Golse , Iván Moyano

We present the results of a study of the gauge dependence of spacetime perturbations. In particular, we consider gauge invariance in general, we give a generating formula for gauge transformations to an arbitrary order n, and explicit…

广义相对论与量子宇宙学 · 物理学 2007-05-23 M. Bruni , S. Matarrese , S. Mollerach , S. Sonego

The paper considers existence results of solution for a linear coupled system of Boltzmann transport equations and related inverse problem. The system models the evolution of three species of particles, photons, electrons and positrons.…

偏微分方程分析 · 数学 2019-12-02 Jouko Tervo

Higher (2nd)-order Wigner distribution function in quantum phase space for entangled bi-modal coherent states, a representative of higher (2nd)-order optical-polarization, is introduced by generalizing kernel (transiting) operator in…

量子物理 · 物理学 2012-04-04 Ravi S. Singh , Sunil P. Singh , Lallan Yadava , Gyaneshwar K. Gupta

The linear polarization signals produced by scattering processes in strong resonance lines are rich in information on the magnetic and thermal structure of the chromosphere and transition region of the Sun and of other stars. A correct…

太阳与恒星天体物理 · 物理学 2015-06-19 Luca Belluzzi , Javier Trujillo Bueno

An economic technique for calculation of polarized bremsstrahlung process is proposed, assuming typical atomic momentum transfer $q\ll m$. The adopted approach is based on the natural reduction of the matrix element to the form…

高能物理 - 唯象学 · 物理学 2008-06-23 Miccola V. Bondarenco

We present a formalism for analyzing a full-sky temperature and polarization map of the cosmic microwave background. Temperature maps are analyzed by expanding over the set of spherical harmonics to give multipole moments of the two-point…

天体物理学 · 物理学 2009-10-28 Marc Kamionkowski , Arthur Kosowsky , Albert Stebbins

We review the general construction of distribution functions for gases of fermions and bosons (photons), emphasizing the similarities and differences between both cases. The central object which describes polarization for photons is a…

宇宙学与河外天体物理 · 物理学 2020-10-06 Cyril Pitrou

The two-photon decay in hydrogen-like ions is investigated within the framework of second order perturbation theory and Dirac's relativistic equation. Special attention is paid to the angular correlation of the emitted photons as well as to…

原子物理 · 物理学 2014-10-23 P. Amaro , F. Fratini , S. Fritzsche , P. Indelicato , J. P. Santos , A. Surzhykov

Collisionless Boltzmann equation is used to describe the intensity correlations in partially saturated and fully saturated regimes in terms of photon distribution function in the phase space. Explicit expression for fourth moment of the…

量子物理 · 物理学 2022-07-13 Roman Baskov