A. Kankainen

2 ta ish

University of Jyväskylä

1. Evolution of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>50</mml:mn></mml:math>Shell Gap Energy towards<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mn>78</mml:mn></mml:mmultiscripts></mml:math>

   J. Hakala, S. Rahaman, V.-V. Elomaa +12

   MaqolaOAOchiq kirish20082 iqtibos

   ABIABI:AkademIndex/2026.other.164254

2. First evidence for non 1− pygmy dipole resonance in neutron-rich nuclei

   R. Li, V. Yu. Ponomarev, M.N. Harakeh +28

   PreprintOAOchiq kirishNuclear physics research studiesResearch Square20230 iqtibos

   ABIABI:AkademIndex/2023.preprint.000064