DREB2018 -- 10th International Conference on Direct Reactions with Exotic Beams

Session

Session 8

Jun 5, 2018, 4:00 PM

Kunibiki Messe (Matsue)

14. From Nuclei to Neutron Stars with a Microscopic Approach

Prof. Francesca Sammarruca (University of Idaho)

6/5/18, 4:00 PM

Oral contribution

Neutron-rich systems are associated with a variety of important and still open questions such as: the location of neutron drip lines, the thickness of neutron skins, and the structure of neutron stars. Common to these diverse situations is the equation of state (EoS) of neutron-rich matter, namely the energy per particle in isospin-asymmetric matter as a function of density (and other...

8. A POSSIBLE NUCLEAR SOLUTION TO THE 18F DEFICIENCY IN NOVAE

Dr marco la cognata (infn-lns)

6/5/18, 4:18 PM

Oral contribution

A POSSIBLE NUCLEAR SOLUTION TO THE 18F DEFICIENCY IN NOVAE

M. La Cognata1, R. G. Pizzone1, J. José2,3, M. Hernanz3,4, S. Cherubini1,5, M. Gulino1,6, G. G. Rapisarda1,5, and C. Spitaleri1,5

1 INFN - Laboratori Nazionali del Sud, Catania, Italy
2 Departament de Física, EEBE, Universitat Politècnica de Catalunya, E-08019 Barcelona, Spain
3 Institut d’Estudis Espacials de Catalunya,...

29. X-ray bursts: Indirect measurement of the astrophysical 23Al(p,γ) reaction

Dr Mohamad Moukaddam (University of Surrey)

6/5/18, 4:36 PM

Oral contribution

X-ray bursts are the most frequent stellar explosions to occur throughout the cosmos and as such, represent key research environments for the field of nuclear astrophysics. These cataclysmic binary systems are known to exhibit distinctive light curves, which have now been observed with unprecedented sensitivity, that provide a detailed reflection of the underlying nuclear physics processes...

82. Direct Measurement of Resonances in ⁷Be<em>(&alpha;,&gamma;)</em>¹¹C With DRAGON

Dr Devin Connolly (TRIUMF)

6/5/18, 4:54 PM

Oral contribution

Nucleosynthesis of the p-nuclei is one of the remaining unsolved puzzles in nuclear astrophysics. One possible mechanism for production of p-nuclei is the νp-process, which is thought to occur in the ejecta of core-collapse supernovae. A recent study found that the p-p chain breakout reaction ⁷Be(α,γ)¹¹C...

105. Study of 19Ne using the 15O + alpha experiment

Ms Dahee Kim (Department of Physics, Ewha Womans University, Seoul, Korea)

6/5/18, 5:12 PM

Oral contribution

Classical novae are one of the most energetic stellar events in the Universe. In this site, intense γ-rays due to the beta decay of 18F produced are emitted by the HCNO cycle. The amount of 18F is determined by two destructive channels 18F(p,α)15O and 18F(p,γ)19Ne[1]. The reaction rates of the two destructive channels affect to the novae calculation model[2,3]. For this reason, many...