Decay properties of exotic<i>N</i>≃28 S and Cl nuclei and the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Ca</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>48</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mo>/</mml:mo></mml:mrow><mml:mrow><mml:mn>46</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>Ca abundance ratioO. Sorlin, W. Hillebrandt, R. Anne et al.|Physical Review C|1993Cited by 142
Search for 28O and study of neutron-rich nuclei near the N = 20 shell closureO. Tarasov, J. S. Winfield, R. G. Allatt et al.|Physics Letters B|1997Cited by 132
Radioactivity of neutron-rich oxygen, fluorine, and neon isotopesA. T. Reed, S. M. Vincent, O. Tarasov et al.|Physical Review C|1999Cited by 78
The decay modes of proton drip-line nuclei with A between 42 and 47V. Borrel, O. Sorlin, R. Anne et al.|Zeitschrift für Physik A Hadrons and Nuclei|1992Cited by 55
Neutrino absorption efficiency of an<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Ar</mml:mi></mml:math>detector from the β decay of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Ti</mml:mi></mml:math>Mahasweta Bhattacharya, O. Sorlin, A. Garcı́a et al.|Physical Review C|1998Cited by 43