Measurement of the stellar<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mn>58</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mn>59</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>cross section with accelerator mass spectrometry

P. Ludwig(Excellence Cluster Universe), A. Wallner(Australian National University), G. Korschinek(Technical University of Munich), Georg Rugel(Technical University of Munich), I. Dillmann(GSI Helmholtz Centre for Heavy Ion Research), K. Knie(Technical University of Munich), Karin Hain(Excellence Cluster Universe), L. Fimiani(Excellence Cluster Universe), Michael Heil(Excellence Cluster Universe), Franz Käppeler(Karlsruhe Institute of Technology), Johannes Lachner(Helmholtz-Zentrum Dresden-Rossendorf), M. Poutivtsev(Technical University of Munich), T. Faestermann(Technical University of Munich)
Physical Review C
March 9, 2017
Cited by 9


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