Radiative Corrections in a Strong Magnetic Field

Radiative Transition of Massless Neutrino in Strong Magnetic Field

Radiative transition of massless neutrino νl → νl + γ (l = e, μ, τ) in a strong magnetic field is investigated in the framework of the Standard Model. The process probability and the mean values of the neutrino energy and momentum loss are presented. Possible astrophysical manifestation of the process considered is analysed. Talk given at the XXXII Rencontres de Moriond on Electroweak interacti...

Strong-field Radiative Scattering

Strong radiative corrections to Wbb̄ production in pp̄ collisions

Structure and radiative transitions of the hydrogen atom moving in a strong magnetic field

The discrete specmm of the hydrogen atom moving acmss a stmng magnetic field (E = 7 x 10"-7 x IO'* G) is studied by expanding wavefunctions over a complete onhogonal basis, whose single term pmvides a correct description of an mmic state at large pseudomomenta K of the h'ansverse motion. Wavefunctions, energies, atomic sires and oscillator strengths of radiative transitions a~ calculated and an...

Coulomb Scattering in a Strong Magnetic Field

The presence of a strong magnetic eld intrinsically changes the orbit of electrons in their Coulomb interactions with ions for a range of parameters. The characteristic scale for the orbit modi cation is r0 = (Zme=4 0B) where Ze is the ion charge, me the electron mass and B the magnetic eld strength. The scale length is comparable to the interparticle spacing when n 1=3 e r0 = (!pe=!ce) 2=3(Z=4...