Titlebook: Spallation Nuclear Reactions and their Applications; B. S. P. Shen,M. Merker Book 1976 D. Reidel Publishing Company, Dordrecht, Holland 19

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,Spallation Reactions: Experimental Results, 1967–75,calculations with experiment. The following chapter in this volume by H. Bertini (1976) continues that effort; here we concentrate on describing experimental results obtained subsequent to 1967 and discuss their significance.

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Book 1976a. I Since that time, a number of devel­ opments have given renewed impetus to the study of spallation reactions. Among these are the successful acceleration of high­ energy heavy ions in the laboratory and their potential use in cancer radiotherapy, the availability of returned lunar rocks containi

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Spallation Reactions: Calculations,a will probably yield the most accurate predictions for these reactions in general. However, if the products in question have binding energies appreciably different from their isotopic neighbors and if the cross section is ∼ 30 mb or larger, then the intranuclear-cascade-evaporation approach is prob

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Semiempirical Cross Sections, and Applications to Nuclear Interactions of Cosmic Rays,ed, of high-energy reactions. Here we present parameters that are updated on the basis of recent experimental data. These calculations have been employed in the analysis of cosmic-ray data when measured values are unavailable. (About half of the cosmic rays heavier than helium have undergone spallat

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The Application of Nuclear Cross Section Measurements to Spallation Reactions in Cosmic Rays,actions*. These studies have been going on for several decades, essentially ever since the availability of particle accelerators made it possible to produce such reactions artificially. As in many areas, however, one finds that what scientists are able to do in the laboratory, nature has managed to

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The Light Element Formation: A Signature of High Energy Nuclear Astrophysics,r to be synthetized by high energy processes occurring either during the interaction of galactic cosmic rays with the interstellar medium or in supernovae envelopes. These formation processes are discussed. It is emphasized that the most coherent scenario regarding the formation of the light element