The reported strengths of newly discovered resonances in original Letter were affected by an error in the analysis. The energy straggling of the ion beam was erroneously neglected. When taking this effect into account, 18-19% higher values are found for the resonance strengths. The astrophysical implications are unchanged. The astrophysical consequences shown in original Letter and [2] used a previous calculation [8] and remain valid. For newer astrophysical work, see Ref. [9], which is also unaffected by the present correction. (Formula Presented). (Table Presented).

Erratum: Three new low-energy resonances in the Ne 22 (p,γ) Na 23 reaction (Physical Review Letters (2015) 115 (252501) DOI: 10.1103/PhysRevLett.115.252501) / F. Cavanna, R. Depalo, M. Aliotta, M. Anders, D. Bemmerer, A. Best, A. Boeltzig, C. Broggini, C.G. Bruno, A. Caciolli, P. Corvisiero, T. Davinson, A. Di Leva, Z. Elekes, F. Ferraro, A. Formicola, Z. Fülöp, G. Gervino, A. Guglielmetti, C. Gustavino, G. Gyürky, G. Imbriani, M. Junker, R. Menegazzo, V. Mossa, F.R. Pantaleo, P. Prati, D.A. Scott, E. Somorjai, O. Straniero, F. Strieder, T. Szücs, M.P. Takács, D. Trezzi. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 120:23(2018 Jun 05). [10.1103/PhysRevLett.120.239901]

Erratum: Three new low-energy resonances in the Ne 22 (p,γ) Na 23 reaction (Physical Review Letters (2015) 115 (252501) DOI: 10.1103/PhysRevLett.115.252501)

R. Depalo;F. Ferraro;A. Guglielmetti;D. Trezzi
2018

Abstract

The reported strengths of newly discovered resonances in original Letter were affected by an error in the analysis. The energy straggling of the ion beam was erroneously neglected. When taking this effect into account, 18-19% higher values are found for the resonance strengths. The astrophysical implications are unchanged. The astrophysical consequences shown in original Letter and [2] used a previous calculation [8] and remain valid. For newer astrophysical work, see Ref. [9], which is also unaffected by the present correction. (Formula Presented). (Table Presented).
physics and astronomy (all)
Settore FIS/04 - Fisica Nucleare e Subnucleare
5-giu-2018
Article (author)
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/583340
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