Incoherent scattering is one of the major processes by which gamma rays interact with matter in the energy range from 100 KeV to I MeV. The effect was simultaneously but separately observed by Compton (1923) and Debye (1923) based on Einstein's light quantum hypothesis. Debye suggested that the effect should bear Compton's name alone and hence it was named "Compton effect". Tabulations are presented of the atomic form factor, F (α, Z), and the incoherent scattering function, S (x, Z), for values of x (=sin ϑ/2)/λ) from 0.005 Å−1 to 109 Å−1, for all elements A=1 to 100. These tables are constructed from available state‐of‐the‐art theoretical data, including the Pirenne formulas for Z=1, configuration‐into action results by Brown using Brown‐Fontana and Weiss correlated wave functions for Z=2 to 6 non‐relativistic Hartree‐Fock results by Cromer for Z=7 to 100 and a relativistic K‐shell analytic expression for F(x, Z) by Bethe Levinger for x≳10 Å−1 for all elements Z=2 to 100. These tabulated values are graphically compared with available photon scattering angular distribution measurements.
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Gurvinder Singh Bajwa➢ Ph.D in the field of Electronics from Monad University, Hapur, 2013➢ M-Tech Total Quality Engineering and Management from PEC University Chandigarh➢ M-Tech Electronics and Telecommunication from J.R.N.R.V University Udaipur with specialization inInstrumentation and Control, 2007➢ B-Tech (Electronics & Instrumentation).
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Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany
Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Incoherent scattering is one of the major processes by which gamma rays interact with matter in the energy range from 100 KeV to I MeV. The effect was simultaneously but separately observed by Compton (1923) and Debye (1923) based on Einstein's light quantum hypothesis. Debye suggested that the effect should bear Compton's name alone and hence it was named 'Compton effect'. Tabulations are presented of the atomic form factor, F ( , Z), and the incoherent scattering function, S (x, Z), for values of x (=sin /2)/ ) from 0.005 Å-1 to 109 Å-1, for all elements A=1 to 100. These tables are constructed from available state-of-the-art theoretical data, including the Pirenne formulas for Z=1, configuration-into action results by Brown using Brown-Fontana and Weiss correlated wave functions for Z=2 to 6 non-relativistic Hartree-Fock results by Cromer for Z=7 to 100 and a relativistic K-shell analytic expression for F(x, Z) by Bethe Levinger for x 10 Å-1 for all elements Z=2 to 100. These tabulated values are graphically compared with available photon scattering angular distribution measurements. 168 pp. Englisch. Seller Inventory # 9783330324725
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Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Bajwa Gurvinder SinghGurvinder Singh Bajwa? Ph.D in the field of Electronics from Monad University, Hapur, 2013? M-Tech Total Quality Engineering and Management from PEC University Chandigarh? M-Tech Electronics and Telecommunication. Seller Inventory # 151238030
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Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Incoherent scattering is one of the major processes by which gamma rays interact with matter in the energy range from 100 KeV to I MeV. The effect was simultaneously but separately observed by Compton (1923) and Debye (1923) based on Einstein's light quantum hypothesis. Debye suggested that the effect should bear Compton's name alone and hence it was named 'Compton effect'. Tabulations are presented of the atomic form factor, F (¿, Z), and the incoherent scattering function, S (x, Z), for values of x (=sin ¿/2)/¿) from 0.005 Å¿1 to 109 Å¿1, for all elements A=1 to 100. These tables are constructed from available state¿of¿the¿art theoretical data, including the Pirenne formulas for Z=1, configuration¿into action results by Brown using Brown¿Fontana and Weiss correlated wave functions for Z=2 to 6 non¿relativistic Hartree¿Fock results by Cromer for Z=7 to 100 and a relativistic K¿shell analytic expression for F(x, Z) by Bethe Levinger for x¿10 Å¿1 for all elements Z=2 to 100. These tabulated values are graphically compared with available photon scattering angular distribution measurements.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 168 pp. Englisch. Seller Inventory # 9783330324725
Seller: preigu, Osnabrück, Germany
Taschenbuch. Condition: Neu. A Study on Whole-Atom Integral Incoherent Scattering Cross Sections | with Respect to Gamma X-Ray | Gurvinder Singh Bajwa (u. a.) | Taschenbuch | 168 S. | Englisch | 2017 | LAP LAMBERT Academic Publishing | EAN 9783330324725 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu. Seller Inventory # 109342015
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Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Incoherent scattering is one of the major processes by which gamma rays interact with matter in the energy range from 100 KeV to I MeV. The effect was simultaneously but separately observed by Compton (1923) and Debye (1923) based on Einstein's light quantum hypothesis. Debye suggested that the effect should bear Compton's name alone and hence it was named 'Compton effect'. Tabulations are presented of the atomic form factor, F ( , Z), and the incoherent scattering function, S (x, Z), for values of x (=sin /2)/ ) from 0.005 Å-1 to 109 Å-1, for all elements A=1 to 100. These tables are constructed from available state-of-the-art theoretical data, including the Pirenne formulas for Z=1, configuration-into action results by Brown using Brown-Fontana and Weiss correlated wave functions for Z=2 to 6 non-relativistic Hartree-Fock results by Cromer for Z=7 to 100 and a relativistic K-shell analytic expression for F(x, Z) by Bethe Levinger for x 10 Å-1 for all elements Z=2 to 100. These tabulated values are graphically compared with available photon scattering angular distribution measurements. Seller Inventory # 9783330324725