Reevaluation of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mn>22</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Na</mml:mi><mml:mprescripts/><mml:none/><mml:mn>23</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction rate-Reference-Cited by-同舟云学术

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Reevaluation of the Ne22(p,γ)Na23 reaction rate

Published:2024-04-16 Issue:4 Volume:109 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Ali Sk Mustak¹^ORCID,Santra Rajkumar²,Sharma Sathi³,Mondal Ashok Kumar³

Affiliation:

1. Facility for Rare Isotope Beams, Michigan State University, East Lansing, Michigan 48824, USA

2. Variable Energy Cyclotron Centre, 1/AF, Bidhan Nagar, Kolkata 700064, India

3. Department of Physics, Manipal University, Jaipur, Rajasthan 303007, India

Funder

National Science Foundation

Texas A and M University

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.109.045809/fulltext

Reference33 articles.

1. Nuclear Reactions with the Neon Isotopes in Stars.

2. Hydrogen burning of 20Ne and 22Ne in stars

3. Nuclear reactions in stellar helium burning and later hydrostatic burning stages

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

5. Multiple populations in globular clusters

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