The main stages in the evolution of a neutron star, from its birth as a proto-neutron star, to its old age as a cold, catalyzed configuration, are described. A proto-neutron star is formed in the aftermath of a successful supernova explosion and its evolution is dominated by neutrino diffusion. Its neutrino signal is a valuable diagnostic of its internal structure and composition. During its tr...

Crystallization and preliminary neutron-diffraction measurements of wild-type variant Val58-->Ile of the Escherichia coli trp repressor are reported. A vapor-diffusion chamber suitable for initial protein-solution Volumes in the range 0.2-0.5 ml was used to grow cube-shaped crystals with edge dimensions in the range 0.8-1.4 mm. Neutron Laue measurements to a nominal resolution of 2.1 A were rec...

Recent analysis of the isospin diffusion data from heavy-ion collisions based on an isospinand momentum-dependent transport model with in-medium nucleon-nucleon cross sections has led to the extraction of a value of L = 88±25 MeV for the slope of the nuclear symmetry energy at saturation density. This imposes stringent constraints on both the parameters in the Skyrme effective interactions and ...

Background: To evaluate the effects of hyperthermia (HT) on the frequency of chromosomal aberrations induced by a low dose of neutron or γ-rays in human peripheral blood lymphocytes. Materials and Methods: Blood samples were exposed to HT (41.5°C for 30 and 60min, 43°C for 15 and 30min), 10 cGy neutron or γ-rays, HT + neutron/γ, and neutron/γ + HT. After standard cell culture, harvestin...

Background: Neutron contamination is produced in electron beams of linac when tooth or dental materials are located in the path of beam. Objective: This study aims to determine the neutron dose contamination from different dental restoration materials in electron mode of a linac. Material and Methods: In this experimental study, the neutron dose contamination was calculated in the p...

We review the recent progress in application of microscopic many-body theory, based on realistic twoand threenucleon interactions, to nuclei and neutron star matter. Modern models of nuclear interactions are discussed along with quantum Monte Carlo methods used to calculate nuclear and nucleon matter properties. Essentially exact Green’s function Monte Carlo calculations have been successfully ...

The neutron energy spectra have been calculated in the fuel region, inner and outer irradiation sites of the zero power research reactor using the MCNP-4C code and the combination of the WIMS-D/4 transport code for generation of group constants and the three-dimensional CITATION diffusion code for core analysis calculations. The neutron energy spectrum has been divided into three regions and co...