Towards an ab initio description of light-nuclei radiative captures

The 3He(α, γ)7Be and 3H(α, γ)7Li astrophysical S factors are evaluated at low collision energies (less than 2.5 MeV in the centre-of-mass frame) within the no-core shell model with continuum using a renormalized chiral nucleon-nucleon interaction.

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Bibliographische Detailangaben
Hauptverfasser:	Dohet-Eraly, Jérémy, Navrátil, Petr, Quaglioni, Sofia, Horiuchi, Wataru, Hupin, Guillaume
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	Nucleon-nucleon interactions
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	The 3He(α, γ)7Be and 3H(α, γ)7Li astrophysical S factors are evaluated at low collision energies (less than 2.5 MeV in the centre-of-mass frame) within the no-core shell model with continuum using a renormalized chiral nucleon-nucleon interaction.
ISSN:	2100-014X 2101-6275 2100-014X
DOI:	10.1051/epjconf/201611306002