R. Bodemann

TL;DR: In this paper, a consistent database covering presently ca 550 nuclear reactions and containing nearly 15,000 individual cross sections of which about 10000 are reported here for the first time, providing a basis for model calculations of the production of cosmogenic nuclides in extraterrestrial matter by solar and galactic cosmic ray protons.

TL;DR: In this paper, the authors measured the depth and size dependence of cosmogenic nuclides in ordinary chondrites for preatmospheric radii between 8.5 cm and about 100 cm, and the observed depth profiles and the dependence of the center production rates on meteoroid size were well reproduced by model calculations based on Monte Carlo calculations of the intra and internuclear cascade of galactic protons in meteoritic matter and on experimental and theoretical excitation functions of the underlying nuclear reactions.

TL;DR: In a series of irradiation experiments at the cyclotron of the Svedberg Laboratory/University of Uppsala sixteen different target elements were investigated for proton energies up to 100 MeV in order to determine such thin-target excitation functions as mentioned in this paper.

TL;DR: In this article, cross sections for the production of Be from O, Mg, Al, Si, Mn, Fe and Ni and 26Al were measured using accelerator mass spectrometry, and Monte Carlo calculations on the basis of an intranuclear-cascade/evaporation model using the HERMES code system.

TL;DR: In this paper, a detailed hybrid model analysis was performed using the code ALICE LIVERMORE 87, which in contrast to earlier formulations of the model takes into account experimental mass data, multiple preequilibrium nucleon emission and non-integer initial exciton numbers.