Author: Martin Walt
Publisher:
ISBN:
Category :
Languages : en
Pages : 134
Book Description
The Scattering of 1-Mev Neutrons by Medium and Heavy Elements
Diffusion of Neutrons in a Heavy Elements Medium and Application to the Multigroup Diffusion Theory
Elastic Scattering of Polarized 4 MeV Neutrons by Medium and Heavy Nuclei
Fast-neutron Scattering from Elemental Mo, Sn, Sb, and Te
Author: A. B. Smith
Publisher:
ISBN:
Category : Fast neutrons
Languages : en
Pages : 38
Book Description
Publisher:
ISBN:
Category : Fast neutrons
Languages : en
Pages : 38
Book Description
Elastic Scattering of Neutrons by Atomic Nuclei
Author: T. A. Goloborod'ko
Publisher:
ISBN:
Category : Neutrons
Languages : en
Pages : 18
Book Description
Publisher:
ISBN:
Category : Neutrons
Languages : en
Pages : 18
Book Description
Small Angle Neutron Scattering at 4.3 MeV from Heavy Elements
Author: Robert Cassin McFadden
Publisher:
ISBN:
Category : Neutron cross sections
Languages : en
Pages : 200
Book Description
Publisher:
ISBN:
Category : Neutron cross sections
Languages : en
Pages : 200
Book Description
Nuclear Science Abstracts
Elements of Slow-Neutron Scattering
Author: J. M. Carpenter
Publisher: Cambridge University Press
ISBN: 0521857813
Category : Science
Languages : en
Pages : 539
Book Description
This book provides a comprehensive and up-to-date introduction to the fundamental theory and applications of slow-neutron scattering.
Publisher: Cambridge University Press
ISBN: 0521857813
Category : Science
Languages : en
Pages : 539
Book Description
This book provides a comprehensive and up-to-date introduction to the fundamental theory and applications of slow-neutron scattering.
Anisotropic Elastic Scattering Neutrons
Author: C. M. Copenhaver
Publisher:
ISBN:
Category : Elastic scattering
Languages : en
Pages : 28
Book Description
Publisher:
ISBN:
Category : Elastic scattering
Languages : en
Pages : 28
Book Description
Neutrons and Related Gamma Ray Problems / Neutronen und Verwandte Gammastrahlprobleme
Author: Edoardo Amaldi
Publisher: Springer Science & Business Media
ISBN: 364245920X
Category : Science
Languages : en
Pages : 874
Book Description
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.
Publisher: Springer Science & Business Media
ISBN: 364245920X
Category : Science
Languages : en
Pages : 874
Book Description
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.