Articoli correlati a Neutrons and Related Gamma Ray Problems / Neutronen...

Neutrons and Related Gamma Ray Problems / Neutronen Und Verwandte Gammastrahlprobleme: 8 / 38 / 2 - Brossura

 
9783642459221: Neutrons and Related Gamma Ray Problems / Neutronen Und Verwandte Gammastrahlprobleme: 8 / 38 / 2
Vedi tutte le copie di questo ISBN:
 
 
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.

Le informazioni nella sezione "Riassunto" possono far riferimento a edizioni diverse di questo titolo.

Contenuti:
The Production and Slowing Down of Neutrons.- A. Introduction.- I. The discovery of the neutron.- II. The properties of the neutron as a fundamental particle and its role in nuclear structure.- III. General remarks on the interaction of neutrons with matter. The first neutron reactions.- IV. The artificial radioactivity. Various reactions produced by neutrons and their general description.- V. The effect of hydrogeneous substances. The mechanism of the slowing down of neutrons.- VI. A few important properties of slow neutrons and the quantum mechanical representation of processes produced by neutrons.- VII. The velocities reached by slow neutrons.- VIII. Selective capture of slow neutrons.- IX. The main processes involved in the slowing down of neutrons.- B. Reactions with emission of neutrons and neutron sources.- I. The application of the conservation laws to nuclear reactions.- II. The excitation curves of nuclear reactions.- III. The (?, n) reactions.- IV. The (?, n) reactions.- V. The (p, n) reactions.- VI. The (d, n) reactions.- VII. Neutrons in nature.- C. The slowing down of neutrons of energy larger than a few ev.- I. General principles and elementary approach to the problem of slowing down of neutrons.- II. The integral spectrum of the neutrons during the slowing down in an infinite medium.- III. The spatial distribution of neutrons in a medium as a function of the energy.- IV. Experimental data on the space and time distributions of the flux of neutrons of energy ? 1 ev in an infinite medium.- V. Measurements of integral effects produced by epi-cadmium neutrons.- D. Slowing down and diffusion of neutrons in the chemical region, i.e. E less than or of the order of 1 ev.- I. Survey of the main features of the problem.- II. The scattering of slow neutrons by molecules.- III. The scattering of slow neutrons by polycrystalline materials.- IV. The slowing down and diffusion of neutrons.- E. The diffusion of thermal neutrons.- I. General features and mathematical aspects of the diffusion of thermal neutrons.- II. Measurements of the diffusion of thermal neutrons.- III. Detection and absorption of thermal neutrons.- Penetration and Diffusion of X Rays.- A. Elementary processes.- B. General theory.- C. Calculation of flux distributions in infinite homogeneous media.- D. Effects of boundaries and inhomogeneities.- E. Experimental aspects.- Appendix. Notation, units and normalization.- Sachverzeichnis (Deutsch/Englisch).- Subject Index (English/German).

Le informazioni nella sezione "Su questo libro" possono far riferimento a edizioni diverse di questo titolo.

  • EditoreSpringer Nature
  • Data di pubblicazione2013
  • ISBN 10 3642459226
  • ISBN 13 9783642459221
  • RilegaturaCopertina flessibile
  • Numero di pagine881

Spese di spedizione: EUR 23,00
Da: Germania a: U.S.A.

Destinazione, tempi e costi

Aggiungere al carrello

Altre edizioni note dello stesso titolo

9783540024132: Neutrons and Related Gamma Ray Problems / Neutronen und Verwandte Gammastrahlprobleme: 8 / 38 / 2

Edizione in evidenza

ISBN 10:  3540024131 ISBN 13:  9783540024132
Casa editrice: Springer-Verlag Berlin and Heide..., 1959
Rilegato

I migliori risultati di ricerca su AbeBooks

Immagini fornite dal venditore

Edoardo Amaldi
ISBN 10: 3642459226 ISBN 13: 9783642459221
Nuovo Taschenbuch Quantità: 2
Print on Demand
Da:
BuchWeltWeit Ludwig Meier e.K.
(Bergisch Gladbach, Germania)
Valutazione libreria

Descrizione libro Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 884 pp. Englisch. Codice articolo 9783642459221

Informazioni sul venditore | Contatta il venditore

Compra nuovo
EUR 160,49
Convertire valuta

Aggiungere al carrello

Spese di spedizione: EUR 23,00
Da: Germania a: U.S.A.
Destinazione, tempi e costi
Immagini fornite dal venditore

Edoardo Amaldi|U. Fano|L. V. Spencer|M. J. Berger
ISBN 10: 3642459226 ISBN 13: 9783642459221
Nuovo Brossura Quantità: > 20
Print on Demand
Da:
moluna
(Greven, Germania)
Valutazione libreria

Descrizione libro Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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, attentio. Codice articolo 5061731

Informazioni sul venditore | Contatta il venditore

Compra nuovo
EUR 136,16
Convertire valuta

Aggiungere al carrello

Spese di spedizione: EUR 48,99
Da: Germania a: U.S.A.
Destinazione, tempi e costi
Immagini fornite dal venditore

Edoardo Amaldi
ISBN 10: 3642459226 ISBN 13: 9783642459221
Nuovo Taschenbuch Quantità: 1
Da:
AHA-BUCH GmbH
(Einbeck, Germania)
Valutazione libreria

Descrizione libro Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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. Codice articolo 9783642459221

Informazioni sul venditore | Contatta il venditore

Compra nuovo
EUR 164,82
Convertire valuta

Aggiungere al carrello

Spese di spedizione: EUR 32,99
Da: Germania a: U.S.A.
Destinazione, tempi e costi