Resonances above the proton threshold in 26Si

Chipps, Kelly A.

doi:10.1103/PhysRevC.93.035801

Title: Resonances above the proton threshold in 26Si

Abstract

26Al remains an intriguing target for observational gamma-ray astronomy, thanks to its characteristic decay. The 25Al(p, )26Si reaction is part of a chain that bypasses the production of the observable 26Alg in favor of the isomeric state; its rate at novae temperatures is dominated by a resonance around 400 keV, the precise location and J assignment of which has been hotly debated. Considerable confusion in this regard has arisen from the use of outdated excitation energies and masses. Here, a reanalysis of previous work is completed to first, elucidate the confusion regarding the level structure just above the proton threshold, and second, provide focus to future studies.

Authors:

Chipps, Kelly A. ^[1]

Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)

Publication Date:: Sun Mar 06 00:00:00 EST 2016

Research Org.:: Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)

Sponsoring Org.:: USDOE Office of Science (SC)

OSTI Identifier:: 1240524

Alternate Identifier(s):: OSTI ID: 1240214

Grant/Contract Number:: AC05-00OR22725

Resource Type:: Accepted Manuscript

Journal Name:: Physical Review C

Additional Journal Information:: Journal Volume: 93; Journal Issue: 3; Journal ID: ISSN 2469-9985

Publisher:: APS

Country of Publication:: United States

Language:: English

Subject:: 74 ATOMIC AND MOLECULAR PHYSICS

Citation Formats


                    Chipps, Kelly A. Resonances above the proton threshold in 26Si.  United States: N. p., 2016. 
Web.  doi:10.1103/PhysRevC.93.035801.

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                    Chipps, Kelly A. Resonances above the proton threshold in 26Si.  United States.  https://doi.org/10.1103/PhysRevC.93.035801

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                    Chipps, Kelly A. Sun .  
"Resonances above the proton threshold in 26Si".  United States.  https://doi.org/10.1103/PhysRevC.93.035801.  https://www.osti.gov/servlets/purl/1240524.

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@article{osti_1240524,

  title        = {Resonances above the proton threshold in 26Si},

  author       = {Chipps, Kelly A.},

  abstractNote = {26Al remains an intriguing target for observational gamma-ray astronomy, thanks to its characteristic decay. The 25Al(p, )26Si reaction is part of a chain that bypasses the production of the observable 26Alg in favor of the isomeric state; its rate at novae temperatures is dominated by a resonance around 400 keV, the precise location and J assignment of which has been hotly debated. Considerable confusion in this regard has arisen from the use of outdated excitation energies and masses. Here, a reanalysis of previous work is completed to first, elucidate the confusion regarding the level structure just above the proton threshold, and second, provide focus to future studies.},

  doi          = {10.1103/PhysRevC.93.035801},

  journal      = {Physical Review C},

  number       = 3,

  volume       = 93,

  place        = {United States},

  year         = {Sun Mar 06 00:00:00 EST 2016},

  month        = {Sun Mar 06 00:00:00 EST 2016}

}

Copy to clipboard

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Works referenced in this record:

Penning trap mass measurement of ${}^{26}{Si}$
journal, May 2010

Kwiatkowski, A. A.; Barquest, B. R.; Bollen, G.
Physical Review C, Vol. 81, Issue 5
DOI: 10.1103/physrevc.81.058501

Recent advances in the modelling of classical novae and type I X-ray bursts
journal, February 2012

José, J.; Casanova, J.; Parikh, A.
Journal of Physics: Conference Series, Vol. 337
DOI: 10.1088/1742-6596/337/1/012038

Spectral and intensity variations of Galactic $\mathsf{^{26}}$Al emission
journal, February 2009

Wang, W.; Lang, M. G.; Diehl, R.
Astronomy & Astrophysics, Vol. 496, Issue 3
DOI: 10.1051/0004-6361/200811175

The Imprint of Nova Nucleosynthesis in Presolar Grains
journal, September 2004

Jose, Jordi; Hernanz, Margarita; Amari, Sachiko
The Astrophysical Journal, Vol. 612, Issue 1
DOI: 10.1086/422569

THE EFFECTS OF THERMONUCLEAR REACTION RATE VARIATIONS ON ²⁶ Al PRODUCTION IN MASSIVE STARS: A SENSITIVITY STUDY
journal, March 2011

Iliadis, Christian; Champagne, Art; Chieffi, Alessandro
The Astrophysical Journal Supplement Series, Vol. 193, Issue 1
DOI: 10.1088/0067-0049/193/1/16

Beta-decay properties of 25 Si and 26 P
journal, September 2004

Thomas, J. -C.; Achouri, L.; Äystö, J.
The European Physical Journal A, Vol. 21, Issue 3
DOI: 10.1140/epja/i2003-10218-8

26Al imaging details from COMPTEL
journal, May 1995

Diehl, R.; Knödlseder, J.; Bennett, K.
Advances in Space Research, Vol. 15, Issue 5
DOI: 10.1016/0273-1177(94)00050-b

Radioactive 26Al from massive stars in the Galaxy
journal, January 2006

Diehl, Roland; Halloin, Hubert; Kretschmer, Karsten
Nature, Vol. 439, Issue 7072
DOI: 10.1038/nature04364

Reply to “Comment on ‘Properties of $^{26}$ Mg and $^{26}$ Si in the $s d$ shell model and the determination of the $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si reaction rate' ”
journal, November 2011

Richter, W. A.; Brown, B. Alex; Signoracci, A.
Physical Review C, Vol. 84, Issue 5
DOI: 10.1103/physrevc.84.059802

Thermal Equilibration of ²⁶ Al
journal, August 2001

Runkle, R. C.; Champagne, A. E.; Engel, J.
The Astrophysical Journal, Vol. 556, Issue 2
DOI: 10.1086/321594

Comment on “Properties of $^{26}$ Mg and $^{26}$ Si in the $s d$ shell model and the determination of the $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si reaction rate”
journal, November 2011

Chipps, K. A.; Bardayan, D. W.; Chae, K. Y.
Physical Review C, Vol. 84, Issue 5
DOI: 10.1103/physrevc.84.059801

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work
journal, October 2010

Iliadis, C.; Longland, R.; Champagne, A. E.
Nuclear Physics A, Vol. 841, Issue 1-4
DOI: 10.1016/j.nuclphysa.2010.04.012

Study of the reactions 24,26Mg(3He, n)26,28Si and 28Si(3He, n)30S
journal, April 1982

Bohne, W.; Büchs, K. D.; Fuchs, H.
Nuclear Physics A, Vol. 378, Issue 3
DOI: 10.1016/0375-9474(82)90463-8

Astrophysically Important 26Si States Studied with the 28Si(4He,6He)26Si Reaction
journal, August 2008

Kwon, Y. K.; Lee, C. S.; Moon, J. Y.
Journal of the Korean Physical Society, Vol. 53, Issue 9(2)
DOI: 10.3938/jkps.53.1141

The Ame2012 atomic mass evaluation
journal, December 2012

Wang, M.; Audi, G.; Wapstra, A. H.
Chinese Physics C, Vol. 36, Issue 12
DOI: 10.1088/1674-1137/36/12/003

The Ame2012 atomic mass evaluation
journal, December 2012

Audi, G.; Wang, M.; Wapstra, A. H.
Chinese Physics C, Vol. 36, Issue 12
DOI: 10.1088/1674-1137/36/12/002

26Al in galaxy regions: massive-star interactions with the ISM
journal, February 2004

Diehl, R.; Cerviño, M.; Hartmann, D. H.
New Astronomy Reviews, Vol. 48, Issue 1-4
DOI: 10.1016/j.newar.2003.11.048

Excited states above the proton threshold in 26Si
journal, September 2014

Komatsubara, T.; Kubono, S.; Hayakawa, T.
The European Physical Journal A, Vol. 50, Issue 9
DOI: 10.1140/epja/i2014-14136-4

Strong $^{25} Al + p$ resonances via elastic proton scattering with a radioactive $^{25} Al$ beam
journal, January 2012

Chen, J.; Chen, A. A.; Amádio, G.
Physical Review C, Vol. 85, Issue 1
DOI: 10.1103/physrevc.85.015805

Classical-Nova Contribution to the Milky Way’s ${}^{26}{Al}$ Abundance: Exit Channel of the Key ${}^{25}{Al} (p, γ) {}^{26}{Si}$ Resonance
journal, December 2013

Bennett, M. B.; Wrede, C.; Chipps, K. A.
Physical Review Letters, Vol. 111, Issue 23
DOI: 10.1103/PhysRevLett.111.232503

Constraint of the Astrophysical ${}^{26 g}{Al} (p, γ) {}^{27}{Si}$ Destruction Rate at Stellar Temperatures
journal, May 2015

Pain, S. D.; Bardayan, D. W.; Blackmon, J. C.
Physical Review Letters, Vol. 114, Issue 21
DOI: 10.1103/PhysRevLett.114.212501

New stellar reaction rates for ${}^{25}{Mg}$ ( p ,γ $)^{26}$ Al and ${}^{25}{Al}$ ( p ,γ $)^{26}$ Si
journal, January 1996

Iliadis, C.; Buchmann, L.; Endt, P. M.
Physical Review C, Vol. 53, Issue 1
DOI: 10.1103/PhysRevC.53.475

( $p, t$ ) Reaction on Even-Even $N = Z$ Nuclei in the $2 s 1 d$ Shell
journal, February 1972

Paddock, R. A.
Physical Review C, Vol. 5, Issue 2
DOI: 10.1103/PhysRevC.5.485

Astrophysically important $^{26} Si$ states studied with the $^{28} Si {(p, t)}^{26} Si$ reaction
journal, March 2002

Bardayan, D. W.; Blackmon, J. C.; Champagne, A. E.
Physical Review C, Vol. 65, Issue 3
DOI: 10.1103/PhysRevC.65.032801

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

Caggiano, J. A.; Bradfield-Smith, W.; Lewis, R.
Physical Review C, Vol. 65, Issue 5
DOI: 10.1103/PhysRevC.65.055801

Astrophysically important ${}^{26}{Si}$ states studied with the $({}^{3}{He}, n)$ reaction and the ${}^{25}{Al} (p, γ) {}^{26}{Si}$ reaction rates in explosive hydrogen burning environments
journal, December 2004

Parpottas, Y.; Grimes, S. M.; Al-Quraishi, S.
Physical Review C, Vol. 70, Issue 6
DOI: 10.1103/PhysRevC.70.065805

Mass measurements of ${}^{22}{Mg}$ and ${}^{26}{Si}$ via the ${}^{24}{Mg} (p, t) {}^{22}{Mg}$ and ${}^{28}{Si} (p, t) {}^{26}{Si}$ reactions
journal, May 2005

Parikh, A.; Caggiano, J. A.; Deibel, C.
Physical Review C, Vol. 71, Issue 5
DOI: 10.1103/PhysRevC.71.055804

Astrophysically important ${}^{26}{Si}$ states studied with the ${}^{28}{Si}$ ( $p, t$ ) ${}^{26}{Si}$ reaction. II. Spin of the 5.914-MeV ${}^{26}{Si}$ level and galactic ${}^{26}{Al}$ production
journal, October 2006

Bardayan, D. W.; Howard, J. A.; Blackmon, J. C.
Physical Review C, Vol. 74, Issue 4
DOI: 10.1103/PhysRevC.74.045804

Level structure of ${}^{26}{Si}$ and its implications for the astrophysical reaction rate of ${}^{25}{Al}$ ( $p$ ,γ) ${}^{26}{Si}$
journal, June 2007

Seweryniak, D.; Woods, P. J.; Carpenter, M. P.
Physical Review C, Vol. 75, Issue 6
DOI: 10.1103/PhysRevC.75.062801

Thermonuclear ${}^{25}{Al} (p, γ) {}^{26}{Si}$ reaction rate in classical novae and Galactic ${}^{26}{Al}$
journal, March 2009

Wrede, C.
Physical Review C, Vol. 79, Issue 3
DOI: 10.1103/PhysRevC.79.035803

Lowest $l = 0$ proton resonance in ${}^{26}{Si}$ and implications for nucleosynthesis of ${}^{26}{Al}$
journal, March 2009

Peplowski, P. N.; Baby, L. T.; Wiedenhöver, I.
Physical Review C, Vol. 79, Issue 3
DOI: 10.1103/PhysRevC.79.032801

High-precision ( $p$ , $t$ ) reaction to determine ${}^{25}{Al}$ ( $p, γ$ ) ${}^{26}{Si}$ reaction rates
journal, August 2010

Matic, A.; van den Berg, A. M.; Harakeh, M. N.
Physical Review C, Vol. 82, Issue 2
DOI: 10.1103/PhysRevC.82.025807

The ${}^{28}{Si}$ ( $p, t$ ) ${}^{26}{Si}$ $^{*}$ ( $p$ ) reaction and implications for the astrophysical ${}^{25}{Al}$ ( $p, γ$ ) ${}^{26}{Si}$ reaction rate
journal, October 2010

Chipps, K. A.; Bardayan, D. W.; Chae, K. Y.
Physical Review C, Vol. 82, Issue 4
DOI: 10.1103/PhysRevC.82.045803

$^{26}$ Si excited states via one-neutron removal from a $^{27}$ Si radioactive ion beam
journal, April 2012

Chen, J.; Chen, A. A.; Amthor, A. M.
Physical Review C, Vol. 85, Issue 4
DOI: 10.1103/PhysRevC.85.045809

Spectroscopic factor of the 1 $^{+}$ , $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si resonance at $E_{x} = 5.68$ MeV
journal, October 2013

Parikh, A.; José, J.
Physical Review C, Vol. 88, Issue 4
DOI: 10.1103/PhysRevC.88.048801

Structure of resonances in the Gamow burning window for the ${}^{25}{Al} (p, γ) {}^{26}{Si}$ reaction in novae
journal, September 2015

Doherty, D. T.; Woods, P. J.; Seweryniak, D.
Physical Review C, Vol. 92, Issue 3
DOI: 10.1103/PhysRevC.92.035808

Mass and $Q_{EC}$ value of ${}^{26}{Si}$
journal, March 2009

Eronen, T.; Elomaa, V. -V.; Hager, U.
Physical Review C, Vol. 79, Issue 3
DOI: 10.1103/PhysRevC.79.032802

Discovery of $^{34 g, m} Cl {(p, γ)}^{35} Ar$ resonances activated at classical nova temperatures
journal, January 2015

Fry, C.; Wrede, C.; Bishop, S.
Physical Review C, Vol. 91, Issue 1
DOI: 10.1103/PhysRevC.91.015803

Properties of ${}^{26}{Mg}$ and ${}^{26}{Si}$ in the $sd$ shell model and the determination of the ${}^{25}{Al}$ ( $p$ , $γ$ ) ${}^{26}{Si}$ reaction rate
journal, June 2011

Richter, W. A.; Brown, B. Alex; Signoracci, A.
Physical Review C, Vol. 83, Issue 6
DOI: 10.1103/PhysRevC.83.065803

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work
text, January 2010

R., Longland,; A., Coc,; A. E., Champagne,
The University of North Carolina at Chapel Hill University Libraries
DOI: 10.17615/0w2r-1s08

Radioactive 26Al and massive stars in the Galaxy
text, January 2006

Diehl, Roland; Halloin, Hubert; Kretschmer, Karsten
arXiv
DOI: 10.48550/arxiv.astro-ph/0601015

Beta-decay properties of $^{25}$Si and $^{26}$P
text, January 2004

Thomas, J. -C.; Achouri, L.; Aysto, J.
arXiv
DOI: 10.48550/arxiv.nucl-ex/0411026

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Title: Resonances above the proton threshold in 26Si

Abstract

Citation Formats

Penning trap mass measurement of Si 26 journal, May 2010

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The Imprint of Nova Nucleosynthesis in Presolar Grains journal, September 2004

THE EFFECTS OF THERMONUCLEAR REACTION RATE VARIATIONS ON 26 Al PRODUCTION IN MASSIVE STARS: A SENSITIVITY STUDY journal, March 2011

Beta-decay properties of 25 Si and 26 P journal, September 2004

26Al imaging details from COMPTEL journal, May 1995

Radioactive 26Al from massive stars in the Galaxy journal, January 2006

Reply to “Comment on ‘Properties of 26 Mg and 26 Si in the s d shell model and the determination of the 25 Al( p , γ ) 26 Si reaction rate' ” journal, November 2011

Thermal Equilibration of 26 Al journal, August 2001

Comment on “Properties of 26 Mg and 26 Si in the s d shell model and the determination of the 25 Al( p , γ ) 26 Si reaction rate” journal, November 2011

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work journal, October 2010

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Astrophysically Important 26Si States Studied with the 28Si(4He,6He)26Si Reaction journal, August 2008

The Ame2012 atomic mass evaluation journal, December 2012

The Ame2012 atomic mass evaluation journal, December 2012

26Al in galaxy regions: massive-star interactions with the ISM journal, February 2004

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Strong 25 Al + p resonances via elastic proton scattering with a radioactive 25 Al beam journal, January 2012

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

Constraint of the Astrophysical Al 26 g ( p , γ ) Si 27 Destruction Rate at Stellar Temperatures journal, May 2015

New stellar reaction rates for Mg 25 ( p ,γ ) 26 Al and Al 25 ( p ,γ ) 26 Si journal, January 1996

( p , t ) Reaction on Even-Even N = Z Nuclei in the 2 s 1 d Shell journal, February 1972

Astrophysically important 26 Si states studied with the 28 Si ( p , t ) 26 Si reaction journal, March 2002

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

Astrophysically important Si 26 states studied with the ( He 3 , n ) reaction and the Al 25 ( p , γ ) Si 26 reaction rates in explosive hydrogen burning environments journal, December 2004

Mass measurements of Mg 22 and Si 26 via the Mg 24 ( p , t ) Mg 22 and Si 28 ( p , t ) Si 26 reactions journal, May 2005

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

Level structure of Si 26 and its implications for the astrophysical reaction rate of Al 25 ( p ,γ) Si 26 journal, June 2007

Thermonuclear Al 25 ( p , γ ) Si 26 reaction rate in classical novae and Galactic Al 26 journal, March 2009

Lowest l = 0 proton resonance in Si 26 and implications for nucleosynthesis of Al 26 journal, March 2009

High-precision ( p , t ) reaction to determine Al 25 ( p , γ ) Si 26 reaction rates journal, August 2010

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

26 Si excited states via one-neutron removal from a 27 Si radioactive ion beam journal, April 2012

Spectroscopic factor of the 1 + , 25 Al( p , γ ) 26 Si resonance at E x = 5.68 MeV journal, October 2013

Structure of resonances in the Gamow burning window for the Al 25 ( p , γ ) Si 26 reaction in novae journal, September 2015

Mass and Q EC value of Si 26 journal, March 2009

Discovery of 34 g , m Cl ( p , γ ) 35 Ar resonances activated at classical nova temperatures journal, January 2015

Properties of Mg 26 and Si 26 in the sd shell model and the determination of the Al 25 ( p , γ ) Si 26 reaction rate journal, June 2011

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work text, January 2010

Radioactive 26Al and massive stars in the Galaxy text, January 2006

Beta-decay properties of $^{25}$Si and $^{26}$P text, January 2004

Penning trap mass measurement of ${}^{26}{Si}$
journal, May 2010

Recent advances in the modelling of classical novae and type I X-ray bursts
journal, February 2012

Spectral and intensity variations of Galactic $\mathsf{^{26}}$Al emission
journal, February 2009

The Imprint of Nova Nucleosynthesis in Presolar Grains
journal, September 2004

THE EFFECTS OF THERMONUCLEAR REACTION RATE VARIATIONS ON ²⁶ Al PRODUCTION IN MASSIVE STARS: A SENSITIVITY STUDY
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Beta-decay properties of 25 Si and 26 P
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26Al imaging details from COMPTEL
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Radioactive 26Al from massive stars in the Galaxy
journal, January 2006

Reply to “Comment on ‘Properties of $^{26}$ Mg and $^{26}$ Si in the $s d$ shell model and the determination of the $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si reaction rate' ”
journal, November 2011

Thermal Equilibration of ²⁶ Al
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Comment on “Properties of $^{26}$ Mg and $^{26}$ Si in the $s d$ shell model and the determination of the $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si reaction rate”
journal, November 2011

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work
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Study of the reactions 24,26Mg(3He, n)26,28Si and 28Si(3He, n)30S
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Astrophysically Important 26Si States Studied with the 28Si(4He,6He)26Si Reaction
journal, August 2008

The Ame2012 atomic mass evaluation
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26Al in galaxy regions: massive-star interactions with the ISM
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Excited states above the proton threshold in 26Si
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Strong $^{25} Al + p$ resonances via elastic proton scattering with a radioactive $^{25} Al$ beam
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New stellar reaction rates for ${}^{25}{Mg}$ ( p ,γ $)^{26}$ Al and ${}^{25}{Al}$ ( p ,γ $)^{26}$ Si
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( $p, t$ ) Reaction on Even-Even $N = Z$ Nuclei in the $2 s 1 d$ Shell
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Astrophysically important $^{26} Si$ states studied with the $^{28} Si {(p, t)}^{26} Si$ reaction
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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
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Thermonuclear ${}^{25}{Al} (p, γ) {}^{26}{Si}$ reaction rate in classical novae and Galactic ${}^{26}{Al}$
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Lowest $l = 0$ proton resonance in ${}^{26}{Si}$ and implications for nucleosynthesis of ${}^{26}{Al}$
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High-precision ( $p$ , $t$ ) reaction to determine ${}^{25}{Al}$ ( $p, γ$ ) ${}^{26}{Si}$ reaction rates
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Spectroscopic factor of the 1 $^{+}$ , $^{25}$ Al( $p$ , $γ$ ) $^{26}$ Si resonance at $E_{x} = 5.68$ MeV
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Discovery of $^{34 g, m} Cl {(p, γ)}^{35} Ar$ resonances activated at classical nova temperatures
journal, January 2015

Properties of ${}^{26}{Mg}$ and ${}^{26}{Si}$ in the $sd$ shell model and the determination of the ${}^{25}{Al}$ ( $p$ , $γ$ ) ${}^{26}{Si}$ reaction rate
journal, June 2011

Charged-particle thermonuclear reaction rates: IV. Comparison to previous work
text, January 2010

Radioactive 26Al and massive stars in the Galaxy
text, January 2006

Beta-decay properties of $^{25}$Si and $^{26}$P
text, January 2004