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Book Gamma ray Production Due to Neutron Interactions with Tungsten for Incident Neutron Energies Between 1 0 and 20 MeV

Download or read book Gamma ray Production Due to Neutron Interactions with Tungsten for Incident Neutron Energies Between 1 0 and 20 MeV written by J. K. Dickens and published by . This book was released on 1973 with total page 48 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Gamma ray Production Due to Neutron Interactions with Iron for Incident Neutron Energies Between 0 8 and 20 MeV

Download or read book Gamma ray Production Due to Neutron Interactions with Iron for Incident Neutron Energies Between 0 8 and 20 MeV written by J. K. Dickens and published by . This book was released on 1972 with total page 64 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Gamma ray Production Due to Neutron Interactions with Silver for Incident Neutron Energies Between 0 3 and 20 MeV

Download or read book Gamma ray Production Due to Neutron Interactions with Silver for Incident Neutron Energies Between 0 3 and 20 MeV written by and published by . This book was released on 1975 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Numerical values of differential cross sections for gamma rays produced by neutron reactions with silver have been obtained for neutron energies between 0.3 and 20 MeV for theta/sub gamma/ = 125$sup 0$. The d$sup 2$sigma/d$omega$dE values were obtained using a NaI spectrometer. These data are presented as gamma- ray production group cross-section values of d$sup 2$sigma/d$omega$dE for 0.3 less than or equal to E/sub gamma/ less than or equal to 10.5 MeV, with gamma-ray intervals ranging from 15 keV for E/sub gamma/ less than or equal to 0.4 MeV to 160 keV for E/sub gamma/ approximately 9 MeV. Neutron energy intervals varied from 0.10 MeV for E/sub n/ between 0.3 and 0.4 MeV to 3 MeV for E/sub n/ between 14 and 20 MeV. (auth).

Book Gamma ray Production Due to Neutron Interactions with Zinc Tabulated Differential Cross Sections for 31 Gamma Rays for Incident Neutron Energies Between 0 9 and 6 MeV

Download or read book Gamma ray Production Due to Neutron Interactions with Zinc Tabulated Differential Cross Sections for 31 Gamma Rays for Incident Neutron Energies Between 0 9 and 6 MeV written by and published by . This book was released on 1974 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Numerical values of differential cross section for gamma rays produced by neutron interactions with zinc were measured for neutron energies between 0.9 and 6 MeV for sigma = 120 deg. The d sigma /d omega data were obtained using a 35 cm/sup 3/ Ge(Li) detector. The data consist of cross section values for 31 gamma rays having E/sub gamma / between 300 and =780 keV. Neutron energy intervals varied between a minimum of ~50 keV at E/sub n/, ~ 900 keV and a maximum of ~1.5 MeV for E/sub n/ ~ 5.8 MeV. (auth).

Book Fast Neutron Scattering from the 182 184 and 186 Isotopes of Tungsten

Download or read book Fast Neutron Scattering from the 182 184 and 186 Isotopes of Tungsten written by D. Lister and published by . This book was released on 1967 with total page 36 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Analysis of the Recent TSF Secondary Gamma ray Experiment

Download or read book Analysis of the Recent TSF Secondary Gamma ray Experiment written by F. L. Keller and published by . This book was released on 1958 with total page 56 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Neutrons and Related Gamma Ray Problems Neutronen und Verwandte Gammastrahlprobleme

Download or read book Neutrons and Related Gamma Ray Problems Neutronen und Verwandte Gammastrahlprobleme written by Edoardo Amaldi and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 874 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.