Neutrons and Related Gamma Ray Problems / Neutronen und Verwandte Gammastrahlprobleme

Neutrons and Related Gamma Ray Problems / Neutronen und Verwandte Gammastrahlprobleme

Author: Edoardo Amaldi

Publisher: Springer Science & Business Media

Published: 2012-12-06

Total Pages: 874

ISBN-13: 364245920X

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661 tures, such as occurs in stellar atmospheres and in thermonuc1ear processes, will not be considered 1. Because photoelectric absorption predominates completely at low photon energies, and penetration theory is elementary under these conditions, attention is directed in this artic1e to photon energies above ""20 kev. On the high energy side, this artic1e does not cover the cascade shower processes which are dealt 2 with in cosmic ray studies • In this connection it is recalled that the cascade shower process, which involves electrons and positrons besides X rays, becomes predominant above 10 Mev in heavy elements, and above 100 Mev in light ones. Theories developed for the study of cascade showers in cosmic rays rely on assumptions about the prob ability of interactions with matter which are adequate only at energies of the order of 1 Gev or more. Below this energy there is a gap in which penetration phenomena are qualitatively known and understood but have not yet been calculated in detail. A few detailed experimental studies which have been made at energies up to 300 Mev will be reviewed in this article.


Energy and Angular Distribution of Neutrons and Gamma Rays

Energy and Angular Distribution of Neutrons and Gamma Rays

Author: J. H. Thorngate

Publisher:

Published: 1969

Total Pages: 80

ISBN-13:

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Where possible, these data have been compared with data from previous field experiments. In every case, they were compared with calculations which approximated the experiment. Agreement in both cases is generally good, and this strengthens confidence in calculated results.


Fission Neutrons

Fission Neutrons

Author: Nikolay Kornilov

Publisher: Springer

Published: 2014-07-25

Total Pages: 135

ISBN-13: 3319071335

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Although the fission of heavy nuclei was discovered over 75 years ago, many problems and questions still remain to be addressed and answered. The reader will be presented with an old, but persistent problem of this field: The contradiction between Prompt Fission Neutron (PFN) spectra measured with differential (microscopic) experiments and integral (macroscopic and benchmark) experiments (the Micro-Macro problem). The difference in average energy is rather small ~3% but it is stable and we cannot explain the difference due to experimental uncertainties. Can we measure the PFN spectrum with high accuracy? How may we compare results of different experiments to provide better accuracy? Are our traditional theoretical models correct? What can be done to solve the Micro-Macro problem in future? These questions are discussed in this monograph for the reader. The current work will be of interest to graduate students and researchers, particularly those working in nuclear and neutron physics.