scholarly journals Photodisintegration of the Deuteron in Medium Energy Range and the Pion Theoretical Nuclear Forces

1960 ◽  
Vol 24 (4) ◽  
pp. 797-816 ◽  
Author(s):  
Junji Iwadare ◽  
Masahiko Matsumoto
Keyword(s):  
Energy Range ◽  
Nuclear Forces ◽  
Medium Energy

Deuteron Photodisintegration in the Medium Energy Range

1960 ◽  
Vol 119 (5) ◽  
pp. 1627-1631 ◽  
Author(s):  
Gustav Kramer ◽  
Carl Werntz
Keyword(s):  
Energy Range ◽  
Medium Energy ◽  
Deuteron Photodisintegration

scholarly journals Photodisintegration of the deuteron in the medium energy range

Physica ◽  
1959 ◽  
Vol 25 (7-12) ◽  
pp. 1001-1015 ◽  
Author(s):  
J.J. De Swart ◽  
R.E. Marshak
Keyword(s):  
Energy Range ◽  
Medium Energy

Preliminary experiments for a new cosmic gamma-ray telescope in the medium energy range 10–30 MeV

1978 ◽  
Vol 153 (1) ◽  
pp. 279-282
Author(s):  
Eiki Suzuki ◽  
Tadashi Kubota ◽  
Yo Hirashima
Keyword(s):  
Energy Range ◽  
Gamma Ray ◽  
Medium Energy

Gamma-ray cross sections and effective atomic numbers in some alloys in the energy range 32 to 662 keV

1984 ◽  
Vol 62 (2) ◽  
pp. 178-182 ◽  
Author(s):  
K. Suresh Babu ◽  
S. Chandra Lingam ◽  
D. V. Krishna Reddy
Keyword(s):  
Energy Range ◽  
Cross Sections ◽  
Experimental Error ◽  
Gamma Ray ◽  
Scintillation Detectors ◽  
Medium Energy ◽  
Subtraction Method ◽  
Total Attenuation ◽  
Effective Atomic Numbers ◽  
Scattering Cross Sections

Total attenuation cross sections in four alloys, telphy, dilver P, anhyster DS, and anhyster M, at 32.1, 52, 72.1, 84.3, 145.4, 279.2, and 661.6-keV photon energies are measured in a good geometry setup using two NaI(Tl) scintillation detectors for low and medium energy photons. Experimental total attenuation cross sections are compared with the theoretical values of Storm and Israel and found to be within experimental error. Using the subtraction method, photoelectric and scattering cross sections are obtained at appropriate photon energies and compared with theoretical values. The effective atomic numbers for photoelectric and total gamma-ray interactions are derived and their variation with energy is discussed.

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