Experimental Determination of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi></mml:mrow></mml:math> Widths of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math> Levels in the Region of Astrophysical Interest: New <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><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:mrow><mml:mo>+</mml:mo><mml:mi>α</mml:mi></mml:mrow></mml:math> Reaction Rates and Impact on the Weak <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>s</mml:mi></mml:math> Process-Reference-Cited by-同舟云学术

Experimental Determination of α Widths of Ne21 Levels in the Region of Astrophysical Interest: New O17+α Reaction Rates and Impact on the Weak s Process

Published:2024-05-01 Issue:18 Volume:132 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Hammache F.¹,Adsley P.²³^ORCID,Lamia L.⁴⁵⁶,Harrouz D. S.¹^ORCID,de Séréville N.¹,Bastin B.⁷^ORCID,Choplin A.⁸^ORCID,Faestermann T.⁹^ORCID,Fougères C.⁷^ORCID,Hertenberger R.¹⁰^ORCID,Hirschi R.¹¹¹²,La Cognata M.⁴^ORCID,Meyer A.¹,Palmerini S.¹³¹⁴^ORCID,Pizzone R. G.⁴^ORCID,de Oliveira Santos F.⁷^ORCID,Romano S.⁴⁵⁶,Tumino A.⁴¹⁵,Wirth H.-F.¹⁰

Affiliation:

1. Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France

2. School of Physics, University of the Witwatersrand, Johannesburg 2050, South Africa

3. iThemba Laboratory for Accelerator Based Sciences, Somerset West 7129, South Africa

4. Laboratori Nazionali del Sud—Istituto Nazionale di Fisica Nucleare, Via Santa Sofia 62, 95123 Catania, Italy

5. Dipartimento di Fisica e Astronomia E. Majorana, Universitã di Catania, Catania, Italy

6. Centro Siciliano di Fisica Nucleare e Struttura della Materia-CSFNSM, Catania, Italy

7. Grand Accélérateur National d’Ions Lourds (GANIL), CEA/DRF-CNRS/IN2P3, Boulevard Henri Becquerel, 14076 Caen, France

8. Institut d’Astronomie et d’Astrophysique, Université libre de Bruxelles, CP 225, B-1050 Brussels, Belgium

9. Physik Department E12, Technische Universität München, D-85748 Garching, Germany

10. Fakultät für Physik, Ludwig-Maximilians-Universität München, D-85748 Garching, Germany

11. Astrophysics Research Center, Keele University, Keele, Staffordshire ST5 5BG, United Kingdom

12. Kavli IPMU (WPI), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan

13. Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy

14. Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy

15. Facoltà di Ingegneria e Architettura, Università degli Studi di Enna, Italy

Funder

Ministry of Education, Culture, Sports, Science and Technology

Science and Technology Facilities Council

Horizon 2020 Framework Programme

National Science Foundation

Fonds De La Recherche Scientifique—FNRS

World Premier International Research Centre Initiative

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.132.182701/fulltext

Reference32 articles.

1. Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo

2. Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations

3. Non-standard s-process in massive rotating stars

4. The impact of 17O + α reaction rate uncertainties on the s-process in rotating massive stars

5. The ion optical properties of the Munich Q3D-spectrograph investigated by means of a special experimental ray tracing method

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1. Experimental Determination of α Widths of Ne21 Levels in the Region of Astrophysical Interest: New O17+α Reaction Rates and Impact on the Weak s Process;Physical Review Letters;2024-05-01