A. Schiller

3 ta ish

National Superconducting Cyclotron Laboratory

1. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn>50</mml:mn></mml:math>Shell Gap near<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mn>100</mml:mn></mml:mmultiscripts></mml:math>from Intermediate-Energy Coulomb Excitations in Even-Mass<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>106</mml:mn><mml:mo>−</mml:mo><mml:mn>112</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>Isotopes

   C. Vaman, C. Andreoiu, D. Bazin +21

   MaqolaOAOchiq kirish20075 iqtibos

   ABIABI:AkademIndex/2026.other.155814

2. Discovery of 40Mg and 42Al suggests neutron drip-line slant towards heavier isotopes

   T. Baumann, A. M. Amthor, D. Bazin +13

   Maqola20073 iqtibos

   ABIABI:AkademIndex/2026.other.160173

3. New isotope<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Si</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>44</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and systematics of the production cross sections of the most neutron-rich nuclei

   O. Tarasov, T. Baumann, A. M. Amthor +13

   MaqolaOAOchiq kirish20073 iqtibos

   ABIABI:AkademIndex/2026.other.160176