Constraining the electron-capture rates of neutron rich nuclei with (d,<sup>2</sup>He) reaction in inverse kinematics.
ORAL
Abstract
Nuclear charge-exchange reactions can be used to estimate the electron-capture rates which are key quantities in a variety of astrophysical scenarios. Over the past decades, great progress has been made to constrain electron-capture rates on stable nuclei by using reactions in forward kinematics. However, the unstable neutron-rich nuclei capturing the most during, for example, the core-collapse supernovae, remained inaccessible. Recently a (d,2He) charge-exchange reaction in inverse kinematics with the Active-Target Time-Projection Chamber and the S800 Spectrograph was developed at NSCL, for extracting Gamow-Teller strengths in the β+ direction on unstable nuclei. This makes it possible, for the first time, to constrain electron-capture rates on neutron-rich nuclei. In this talk I will discuss recent results of the pilot 14O(d,2He) experiment.
*This work is supported by the National Science Foundation under Grant PHY-193247145, "Windows on the Universe: Nuclear Astrophysics at the NSCL".
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Presenters
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Simon Giraud
- Michigan State University NSCL/FRIB
- FRIB/NSCL