Engineering topics
Publications and source records attributed to Ginzburg, V. L..
Gamma ray emissions from young supernova remnants are discussed and calculated. The positron annihilation line is also calculated. Decay of charged pions in remnants cause generation of high energy neutrinos. This emission of neutrinos is reviewed. The CR origin and gamma emission from Magellanic clouds help to establish the intensity gradient in the galaxy. This gamma astronomical data is briefly discussed.
Cosmic ray (CR) propagation in the Galaxy and generally in the cosmic plasma is usually considered in the diffusion approximation. The diffusion is regarded to result from CR scattering due to their interaction with a magnetic and an electric field. In most cases the fields are assumed to be given. Meanwhile, in the Galaxy the CR energy density w sub cr is similar to I eV/cm, i.e., it is comparable with the energy densities of the magnetic field and turbulent motions in the interstellar gas. Therefore, for the Galaxy it becomes necessary to take into account the influence of CR on the gas dynamics and on the magnetic fields in this gas. The simplest way to this is to use the hydrodynamic approximation, but this is possible only on scales greatly exceeding the CR free path lambda before scattering and only for times larger than lambda/v approx. equals lambda/c. One should thus obtain corresponding MHD equations and establish the limits of their applicability.
The assumption that cosmic rays originate from metagalactic sources is investigated. Gamma ray astronomy and its application to studying nuclear components of cosmic rays far from the earth, estimating energy density of cosmic rays, and determining magnetic field strength is also examined.
A theory on the origin of cosmic rays is presented. Specifically, magellanic clouds and the galactic center were investigated as possible cosmic ray sources.
Particle motions, reabsorption mechanism, and related problems of synchrotron radiation theory
Uniform and metagalactic cosmic ray models - halo, disk, and nonstationary galactic models
Radio galactic emission and cosmic X-radiation
Coherent radio emission mechanism in quasars and remains of supernovae
Bremsstrahlung nature of X-ray emission from discrete sources
Magnetic fields of collapsing masses and nature of supernovae
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