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We use recently calculated next-to-next-to-leading order (NNLO) anomalous dimension coefficients for the moments of the F2 structure function in eN scattering, together with the corresponding two-loop Wilson coefficients, to obtain improved QCD predictions for non-singlet structure function. The Jacobi polynomial method is used to parameterize parton distribution up to NNLO. Target mass corrections is also consider in our calculations. [ABSTRACT FROM AUTHOR]

Proton and neutron data as well as photon data are necessary in various intermediate energy applications. To meet these requirements, many groups in the world continue some activities concerning nuclear data evaluation in the energy range above 20 MeV, which is the upper limit of conventional general-purpose evaluated nuclear data files. In this paper, reviewed is brief history of intermediate energy nuclear data development as well as Pearlstein’s contribution for it. Present status of world evaluated nuclear data files in the intermediate energy region is reported as well as evaluation methodology and sample results of evaluation and integral benchmark tests by using the case of JENDL High Energy File as an example. © 2005 American Institute of Physics [ABSTRACT FROM AUTHOR]

The Coulomb equilibration time scale among various particle species behind a fast collisionless shock can be much larger than the dynamical time scale in a supernova remnant or CME. Ultraviolet and optical emission line profiles can be used to measure proton, electron and ion temperatures. Particles are fairly close to thermal equilibrium behind a relatively slow (350 km/s) shock, but very far from equilibrium in faster (2000–3000 km/s) shocks. © 2005 American Institute of Physics [ABSTRACT FROM AUTHOR]