26–29 Mar 2012
Aula Magna, Faculty of SMFN
Europe/Rome timezone

Session

Session 3

26 Mar 2012, 14:10
Aula Magna, Faculty of SMFN

Aula Magna, Faculty of SMFN

<a target="_blank" href=http://www.smfn.unipi.it/Informazioni/mappa.aspx>Facoltà di Scienze Matematiche, Fisiche e Naturali</a> Largo Bruno Pontecorvo, 3 I-56127 Pisa (Italy)

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  1. David Jenkins Jenkins (University of York)
    26/03/2012, 14:10
    Talk
    The 18Ne(a,p) reaction is seen to be one of the key reactions determining the break-out from the hot-CNO cycle. There are wide discrepancies between measured cross-sections for this reaction, which may reflect the difficulty in such direct radioactive beam measurements. Moreover, the cross-sections in the literature are inconsistent with measurements of the time-reversed 21Na(p,a)...
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  2. Christian Diget (University of York)
    26/03/2012, 14:35
    Talk
    We here present some of the first direct-reaction data with radioactive ion beams utilising the TIGRESS and SHARC particle-gamma detector systems. In the experiment, transfer reactions in inverse kinematics were used as indirect probes of the 18Ne(alpha,p)21Na and 23Mg(p,gamma)24Al reactions. The SHARC array (Silicon Highly-segmented Array for Reactions and Coulex) is a new multi-purpose...
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  3. Brian Roeder (Texas A&amp;M University)
    26/03/2012, 15:00
    Talk
    The detection of gamma rays from the decay of the 26Al ground state in the galaxy gives evidence that nucleosynthesis is occurring in present-day stars, but its origin is not yet clear. This implies that reactions involving 26Al are important for astrophysical processes. In a recent experiment at Texas A&M University, reactions with the ground state and isomeric state of 26Al were...
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  4. Masaki Sasano (RIKEN Nishina Center for Accelerator-Based Science)
    26/03/2012, 15:25
    Talk
    Electron-capture (EC) and beta-decay play important roles in type-II and typeIa supernovae. They occur through the Gamow-Teller (GT) and Fermi transitions in nuclei, which are extensively studied to reliably estimate the weak-interactions rates. Experimentally, a powerful probe to study GT transitions has been provided by the charge-exchange reactions at intermediate energies such as the...
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