First Direct Measurement of the 64.5 keV Resonance Strength in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>17</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">F</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>18</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:mrow></mml:math> Reaction-Reference-Cited by-同舟云学术

First Direct Measurement of the 64.5 keV Resonance Strength in the O17(p,γ)F18 Reaction

Published:2024-07-30 Issue:5 Volume:133 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Gesuè R. M.¹²^ORCID,Ciani G. F.³⁴,Piatti D.⁵⁶^ORCID,Boeltzig A.⁷,Rapagnani D.⁸⁹,Aliotta M.¹⁰,Ananna C.⁸⁹,Barbieri L.¹⁰,Barile F.⁴,Bemmerer D.⁷,Best A.⁸⁹,Broggini C.⁶,Bruno C. G.¹⁰,Caciolli A.⁵⁶,Campostrini M.¹¹,Casaburo F.¹²¹³,Cavanna F.¹⁴,Colombetti P.¹⁵¹⁴,Compagnucci A.¹²,Corvisiero P.¹²¹³,Csedreki L.¹⁶,Davinson T.¹⁰,De Gregorio G. M.¹⁷¹⁸,Dell’Aquila D.⁸⁹,Depalo R.¹⁷¹⁸,Di Leva A.⁸⁹,Elekes Z.¹⁶¹⁹,Ferraro F.²,Formicola A.²⁰,Fülöp Zs.¹⁶,Gervino G.¹⁵¹⁴,Guglielmetti A.¹⁷¹⁸,Gustavino C.²⁰,Gyürky Gy.¹⁶,Imbriani G.⁸⁹,Junker M.²,Lugaro M.²¹²²²³,Marigo P.⁵⁶,Marsh J.¹⁰,Masha E.⁷,Menegazzo R.⁶,Mercogliano D.⁸⁹,Paticchio V.⁴,Perrino R.⁴,Prati P.¹²¹³,Rigato V.¹¹,Robb D.¹⁰,Schiavulli L.³⁴,Sidhu R. S.¹⁰,Skowronski J.⁵⁶,Straniero O.²⁴²⁰,Szücs T.¹⁶,Zavatarelli S.¹³¹²,

Affiliation:

1. Gran Sasso Science Institute

2. Laboratori Nazionali del Gran Sasso

3. Università degli Studi di Bari “A. Moro

4. INFN, Sezione di Bari

5. Università degli Studi di Padova

6. INFN, Sezione di Padova

7. Helmholtz-Zentrum Dresden-Rossendorf

8. Università degli Studi di Napoli

9. INFN, Sezione di Napoli

10. SUPA

11. Laboratori Nazionali di Legnaro

12. Università degli Studi di Genova

13. INFN, Sezione di Genova

14. INFN, Sezione di Torino

15. Università degli Studi di Torino

16. HUN-REN Institute for Nuclear Research (HUN-REN ATOMKI)

17. Università degli Studi di Milano

18. INFN, Sezione di Milano

19. University of Debrecen

20. INFN, Sezione di Roma

21. Konkoly Observatory

22. HUN-REN

23. ELTE Eötvös Loránd University

24. Osservatorio Astronomico d’Abruzzo

Funder

Instituto Nazionale di Fisica Nucleare

Ministero dell’Istruzione, dell’Università e della Ricerca

European Commission

European Research Council

UK Research and Innovation

Deutsche Forschungsgemeinschaft

Helmholtz-Gemeinschaft

Nemzeti Kutatási, Fejlesztési és Innovaciós Alap

European Cooperation in Science and Technology

Magyar Tudományos Akadémia

Science and Technology Facilities Council

ChETEC-INFRA

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.133.052701/fulltext

Reference53 articles.

1. A COMPARISON OF STELLAR ELEMENTAL ABUNDANCE TECHNIQUES AND MEASUREMENTS

2. The AME 2020 atomic mass evaluation (II). Tables, graphs and references*

3. Experimental determination of theO17(p,α)N14andO17(p,γ)F18reaction rates

4. Nuclear Physics of Stars

5. Oxygen isotopic abundances in the atmospheres of seven red giant stars