Conveners
TUE3
- Dolores Cortina
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Maria Jose Garcia Borge (Consejo Superior de Investigaciones Cientificas (CSIC) (ES)), Vicente Garcia Tavora (Consejo Superior de Investigaciones Cientificas (CSIC) (ES))28/06/2022, 14:40Oral contribution
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Dr László Stuhl (Center for Exotic Nuclear Studies, Institute of Basic Science)28/06/2022, 15:00Oral contribution
We started a program [1] at the RIKEN Radioactive Isotope Beam Factory (RIBF) aiming to measure the spin-isospin responses of light nuclei along the neutron drip line. There is no available data on spin-isospin collectivity for nuclei with large isospin asymmetry factors, where (N−Z)/A>0.25 [2]. We investigated this unexplored region up to (N−Z)/A=0.5.
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The spin-isospin responses of $^{11}$Li... -
Dr Manuela Rodríguez-Gallardo (Universidad de Sevilla)28/06/2022, 15:20Oral contribution
The Borromean nucleus $^{11}$Li presents a two-neutron halo structure that still hides a lot of information about it. Several experimental and theoretical works have tried to shed light in its structure and reaction dynamics during the past decade [Phys. Rev. Lett 109 (2012) 262701; 110 (2013) 142701; 114 (2015) 192502; Phys. Lett. B 774 (2017) 268; Phys. Rev. C 85 (2012) 054610; 92 (2015)...
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Dr Jesús Casal (Universidad de Sevilla)28/06/2022, 15:40Oral contribution
The correlation among the valence neutrons in Borromean halo nuclei are a key element to explain the stability of such loosely bound systems [1,2]. The characterization of the dineutron correlation is therefore an important step in the description of the neutron dripline.
We present here a comparative study of three different two-neutron halos, $^{11}$Li, $^{14}$Be and $^{17}$B,...
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Dr Heshani Jayatissa (Argonne National Laboratory)28/06/2022, 16:00Oral contribution
The dominant (p,$\gamma$) nucleosynthesis flow in Type I X-ray bursts (XRBs) is halted at several waiting point nuclei such as $^{22}$Mg, $^{24-26}$Si, $^{28-30}$S and $^{34}$Ar due to ($p,\gamma$)-($\gamma,p$) equilibrium. Reactions such as ($\alpha$,p) reactions assist the nucleosynthesis flow to bypass these waiting points. The present uncertainties in the relevant ($\alpha,p$) reaction...
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