<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>14</mml:mn></mml:mrow></mml:math>and 16 shell gaps in neutron-rich oxygen isotopesM. Stănoiu, A. Yamamoto, F. Azaiez et al.|Physical Review C|2004Cited by 212
Excited states in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>103</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Sn</mml:mi><mml:mo>:</mml:mo></mml:math>Neutron single-particle energies with respect to<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>100</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Sn</mml:mi></mml:math>C. Fahlander, M. Wolińska, J. Nyberg et al.|Physical Review C|2001Cited by 30
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Study of neutron rich Carbon and Oxygen nuclei up to drip lineM. Stănoiu, A. Yamamoto, F. Azaiez et al.|Nuclear Physics A|2004Cited by 16