← Ishga qaytish
Ushbu ishga iqtibos qilgan ishlar
4 ta ish
Ish: Spectroscopic factors and cluster decay half-lives of heavy nuclei
Production of the doubly magic nucleus<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>100</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>in fusion and quasifission reactions via light particle and cluster emission channels
Sh. A. Kalandarov, G. G. Adamian, N. V. Antonenko +1
ABIExpected production of new exotic<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>α</mml:mi></mml:math>emitters<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Xe</mml:mi><mml:mprescripts/><mml:none/><mml:mn>108</mml:mn></mml:mmultiscripts></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Ba</mml:mi><mml:mprescripts/><mml:none/><mml:mn>112</mml:mn></mml:mmultiscripts></mml:math>in complete fusion reactions
Sh. A. Kalandarov, G. G. Adamian, N. V. Antonenko +1
ABI