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Title: Low-lying resonances in Si 26 relevant for the determination of the astrophysical Al 25 ( p , γ ) Si 26 reaction rate

Journal Article · · Physical Review. C

Sponsoring Organization:
USDOE
Grant/Contract Number:
FG02-96ER40978
OSTI ID:
1856560
Journal Information:
Physical Review. C, Journal Name: Physical Review. C Vol. 105 Journal Issue: 3; ISSN 2469-9985
Publisher:
American Physical SocietyCopyright Statement
Country of Publication:
United States
Language:
English

References (34)

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Classical-Nova Contribution to the Milky Way’s Al 26 Abundance: Exit Channel of the Key Al 25 ( p , γ ) Si 26 Resonance journal December 2013
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  • Perello, J. F.; Almaraz-Calderon, S.; Asher, B. W.
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Simultaneous measurement of β -delayed proton and γ emission of P 26 for the Al 25 ( p , γ ) Si 26 reaction rate journal February 2020
Observation of the $^{26}Al$ emission distribution throughout the Galaxy with INTEGRAL/SPI conference August 2016
Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs journal February 1998
Nuclear Uncertainties in the NeNa‐MgAl Cycles and Production of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $^{22}$ \end{document} Na and \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $^{26}$ \end{document} Al during Nova Outbursts journal July 1999
Transfer Reactions As a Tool in Nuclear Astrophysics journal March 2021
Thermonuclear Al 25 ( p , γ ) Si 26 reaction rate in classical novae and Galactic Al 26 journal March 2009
Charged-particle thermonuclear reaction rates: II. Tables and graphs of reaction rates and probability density functions journal October 2010
Structure of resonances in the Gamow burning window for the Al 25 ( p , γ ) Si 26 reaction in novae journal September 2015
Excited states above the proton threshold in 26Si journal September 2014
Level structure of Si 26 and its implications for the astrophysical reaction rate of Al 25 ( p ,γ) Si 26 journal June 2007
Identification of new states in 26 Si using the 29 Si ( 3 He , 6 He ) 26 Si reaction and consequences for the 25 Al ( p , γ ) 26 Si reaction rate in explosive hydrogen burning environments journal May 2002
A Population of Heavily Reddened, Optically Missed Novae from Palomar Gattini-IR: Constraints on the Galactic Nova Rate journal April 2021
The Si 28 ( p , t ) Si 26 * ( p ) reaction and implications for the astrophysical Al 25 ( p , γ ) Si 26 reaction rate journal October 2010
Astrophysically important Si 26 states studied with the Si 28 ( p , t ) Si 26 reaction. II. Spin of the 5.914-MeV Si 26 level and galactic Al 26 production journal October 2006
The AME 2020 atomic mass evaluation (II). Tables, graphs and references* journal March 2021
New stellar reaction rates for Mg 25 ( p ) 26 Al and Al 25 ( p ) 26 Si journal January 1996
Nuclear Data Sheets for A = 26 journal May 2016

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