Gamma-ray strength functions and their relation to astrophysics

The nuclear {gamma}-ray strength function is one of the indispensable inputs needed for reaction-rate calculations, and is particularly important for the neutron-capture cross section. The nuclear physics group at the Oslo Cyclotron Laboratory has developed a method to extract simultaneously nuclear...

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Bibliographische Detailangaben
Hauptverfasser:	Larsen, A. C., Buerger, A., Guttormsen, M., Hagen, T. W., Nyhus, H. T., Rekstad, J. B., Renstroem, T., Rose, S. J., Ruud, I. E., Siem, S., Syed, N. U. H., Toft, H. K., Tveten, G. M., Wikan, K., Goriely, S., Algin, E., Agvaanluvsan, U., MonAme Scientific Research Center, Ulaanbaatar, Goergen, A., Department of Physics/SAFE, University of Oslo, N-0316 Oslo, Loennroth, T., Mitchell, G. E., Triangle Universities Nuclear Laboratory, Durham, NC 27708
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	ASTROPHYSICS BARYON REACTIONS CAPTURE CROSS SECTIONS DIPOLES ELECTROMAGNETIC RADIATION ENERGY-LEVEL DENSITY FUNCTIONS GAMMA RADIATION GIANT RESONANCE HADRON REACTIONS IONIZING RADIATIONS ISOTOPES KINETICS MULTIPOLES NEUTRON REACTIONS NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEAR REACTION KINETICS NUCLEAR REACTIONS NUCLEAR STRUCTURE NUCLEON REACTIONS OSCILLATION MODES PHYSICS RADIATIONS REACTION KINETICS RESONANCE STRENGTH FUNCTIONS TIN ISOTOPES
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