Direct cross-section measurement of the weak <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>r</mml:mi></mml:math> -process <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Sr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>88</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Zr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>91</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>ν</mml:mi></mml:math> -driven winds of core-collapse supernovae-Reference-Cited by-同舟云学术

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Direct cross-section measurement of the weak r -process Sr88(α,n)Zr91 reaction in ν -driven winds of core-collapse supernovae

Published:2024-06-17 Issue:6 Volume:109 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Fougères C.¹^ORCID,Avila M. L.¹^ORCID,Jayatissa H.¹²,Santiago-Gonzalez D.¹^ORCID,Brandenburg K.³,Meisel Z.³,Mohr P.⁴,Montes F.⁵,Müller-Gatermann C.¹^ORCID,Neto D.⁶^ORCID,Ong W.-J.⁷,Pereira J.⁵,Rehm K. E.¹^ORCID,Tang T. L.¹⁸^ORCID,Tolstukhin I. A.¹^ORCID,Varriano L.⁹^ORCID,Wilson G.¹¹⁰,Wu J.¹¹¹

Affiliation:

1. Argonne National Laboratory

2. Los Alamos National Laboratory

3. Ohio University

4. HUN-REN Institute for Nuclear Research

5. Facility for Rare Isotope Beams

6. University of Illinois Chicago

7. Lawrence Livermore National Laboratory

8. Florida State University

9. University of Chicago

10. Louisiana State University

11. Brookhaven National Laboratory

Funder

U.S. Department of Energy

Nuclear Physics

Argonne National Laboratory

Nemzeti Kutatási Fejlesztési és Innovációs Hivatal

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.109.065805/fulltext

Reference51 articles.

1. r-Process nucleosynthesis in gravitational-wave and other explosive astrophysical events

2. Thesprocess: Nuclear physics, stellar models, and observations

3. Production of C-14 and neutrons in red giants

4. The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status

5. Neutrino-Induced Nucleosynthesis ofA>64Nuclei: TheνpProcess

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