First Direct Limit on the 334 Kev Resonance Strength in $$^{22}$$ne($$\alpha $$,$$\gamma $$)$$^{26}$$mg Reaction
Piatti D.,Masha E.,Aliotta M.,Balibrea-Correa J.,Barile F.,Bemmerer D.,Best A.,Boeltzig A.,Broggini C.,Bruno C. G.,Caciolli A.,Cavanna F.,Chillery T.,Ciani G. F.,Compagnucci A.,Corvisiero P.,Csedreki L.,Davinson T.,Depalo R.,Leva A. di,Elekes Z.,Ferraro F.,Fiore E. M.,Formicola A.,Fülöp Zs.,Gervino G.,Guglielmetti A.,Gustavino C.,Gyürky Gy.,Imbriani G.,Junker M.,Lugaro M.,Marigo P.,Menegazzo R.,Mossa V.,Pantaleo F. R.,Paticchio V.,Perrino R.,Prati P.,Rapagnani D.,Schiavulli L.,Skowronski J.,Stöckel K.,Straniero O.,Szücs T.,Takács M. P.,Zavatarelli S. The European Physical Journal A（2022）
Key words
Astrophysical Reaction Rates,Resonance
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