Strength measurement of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msubsup><mml:mi>E</mml:mi><mml:mrow><mml:mi>α</mml:mi></mml:mrow><mml:mi>lab</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mn>830</mml:mn></mml:mrow></mml:math> keV resonance in 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>α</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Mg</mml:mi><mml:mprescripts/><mml:none/><mml:mn>25</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction using a stilbene detector-Reference-Cited by-同舟云学术

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Strength measurement of the Eαlab=830 keV resonance in the Ne22(α,n)Mg25 reaction using a stilbene detector

Published:2024-07-03 Issue:1 Volume:110 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Shahina ¹^ORCID,deBoer R. J.¹^ORCID,Görres J.¹,Fang R.¹^ORCID,Febbraro M.²³,Kelmar R.¹,Matney M.¹,Manukyan K.¹^ORCID,Nattress J. T.²,Robles E.¹^ORCID,Ruland T. J.²,King T. T.²^ORCID,Sanchez A.¹^ORCID,Sidhu R. S.⁴^ORCID,Stech E.¹^ORCID,Wiescher M.¹^ORCID

Affiliation:

1. University of Notre Dame

2. Oak Ridge National Laboratory

3. Air Force Institute of Technology

4. University of Edinburgh

Funder

National Science Foundation

Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements

Science and Technology Facilities Council

Royal Society International Exchanges

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.110.015801/fulltext

Reference44 articles.

1. THE WEAKs-PROCESS IN MASSIVE STARS AND ITS DEPENDENCE ON THE NEUTRON CAPTURE CROSS SECTIONS

2. The branchings of the main s-process: their sensitivity to α-induced reactions on 13C and 22Ne and to the uncertainties of the nuclear network

3. A Possible Alternative to the R-Process

4. Reaction rates for O-18(alpha, gamma)Ne-22, Ne-22(alpha, gamma)Mg-26, and Ne-22(alpha, n)Mg-25 in stellar helium burning and s-process nucleosynthesis in massive stars

5. Study of the 22Ne(α, n)25Mg reaction: a possible source of stellar neutronS

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