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Иш: Half-lives of neutron-rich<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Cd</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>128</mml:mn><mml:mo>–</mml:mo><mml:mn>130</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>
Synthesis of the Elements in Stars
E. M. Burbidge, G. R. Burbidge, William A. Fowler +1
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C. Freiburghaus, Stephan Rosswog, F.‐K. Thielemann
Мақола19996 иқтибосABIOn the astrophysical robustness of the neutron star merger r-process
O. Korobkin, S. Rosswog, A. Arcones +1
Мақола20125 иқтибосABIEnergy levels and transition probabilities in 130Sn
B. Fogelberg, K. Heyde, J. Sau
Мақола19814 иқтибосABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>82</mml:mn></mml:math>Shell Quenching of the Classical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>r</mml:mi></mml:math>-Process “Waiting-Point” Nucleus<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>130</mml:mn></mml:mmultiscripts></mml:math>
I. Dillmann, Karl Kratz, A. Wöhr +10
Мақола20033 иқтибосABIOn the astrophysical robustness of neutron star merger r-process
O. Korobkin, S. Rosswog, A. Arcones +1
Мақола20122 иқтибосABI