Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: Varying shell gap and deformation in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mi>∼</mml:mi><mml:mn>20</mml:mn></mml:math>unstable nuclei studied by the Monte Carlo shell model

1. New neutron magic number N = 16 for neutron-rich nuclei

   Z. Dlouhý, D. Baiborodin, J. Mrázek

   БобNuclear physics research studiesExotic Nuclei and Atomic Masses20030 иқтибос

   ABIABI:AkademIndex/openalex/2003.chapter.000010

2. Probing<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi mathvariant="italic">sd</mml:mi><mml:mtext>−</mml:mtext><mml:mi mathvariant="italic">fp</mml:mi></mml:mrow></mml:math>cross-shell interactions via terminating configurations in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Sc</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>42</mml:mn><mml:mo>,</mml:mo><mml:mn>43</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

   C. J. Chiara, M. Devlin, E. Ideguchi +20

   МақолаNuclear physics research studiesPhysical Review C20070 иқтибос

   ABIABI:AkademIndex/openalex/2007.article.000042

3. Isospin symmetry in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>s</mml:mi><mml:mi>d</mml:mi></mml:mrow></mml:math>shell: Transition strengths in the neutron-deficient<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>s</mml:mi><mml:mi>d</mml:mi></mml:mrow></mml:math>shell nucleus<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ar</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>33</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

   A. Wendt, J. Taprogge, P. Reiter +42

   МақолаNuclear physics research studiesPhysical Review C20140 иқтибос

   ABIABI:AkademIndex/openalex/2014.article.000177