New recommended ωγ for the Erc.m.=458 keV resonance in Ne22(p,γ)Na23

Kelly, K. J.; Champagne, A. E.; Longland, R.; Buckner, M. Q.

doi:10.1103/PhysRevC.92.035805

Title: New recommended $ω γ$ for the $E_{r}^{c . m .} = 458$ keV resonance in ${}^{22}{Ne} (p, γ) {}^{23}{Na}$

Abstract

The $E_{r}^{c.m.} = 458$ keV resonance in ${}_{22}{Ne} (p, γ) {}_{23}{Na}$ is an ideal reference resonance for measurements of cross sections and resonance strengths in noble gas targets. We report on a new measurement of the strength of this resonance. Data analysis employed the TFractionFitter class of root combined with geant simulations of potential decay cascades from this resonance. This approach allowed us to extract precise primary branching ratios for decays from the resonant state, including a new primary branch to the 7082-keV state in ${}_{23}{Na}$ . Our new resonance strength of $ω γ$ (458 keV) = 0.583(43) eV is more than $1 σ$ higher than a recent high-precision result that relied on literature branching ratios.

Authors:

Kelly, K. J. ^[1]; Champagne, A. E. ^[1]; Longland, R. ^[2]; Buckner, M. Q. ^[3]

Univ. of North Carolina, Chapel Hill, NC (United States); Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory
North Carolina State Univ., Raleigh, NC (United States); Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory
Univ. of North Carolina, Chapel Hill, NC (United States); Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory; Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)

Publication Date:: Fri Sep 04 00:00:00 EDT 2015

Research Org.:: University of North Carolina, Chapel Hill, NC (United States); Duke Univ., Durham, NC (United States). Triangle Universities Nuclear Laboratory

Sponsoring Org.:: USDOE Office of Science (SC), Nuclear Physics (NP)

OSTI Identifier:: 1600485

Alternate Identifier(s):: OSTI ID: 1213967

Grant/Contract Number:: FG02-97ER41041

Resource Type:: Accepted Manuscript

Journal Name:: Physical Review C, Nuclear Physics

Additional Journal Information:: Journal Volume: 92; Journal Issue: 3; Journal ID: ISSN 0556-2813

Publisher:: American Physical Society (APS)

Country of Publication:: United States

Language:: English

Subject:: 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; experimental nuclear astrophysics

Citation Formats


                    Kelly, K. J., Champagne, A. E., Longland, R., and Buckner, M. Q. New recommended ωγ for the Erc.m.=458 keV resonance in Ne22(p,γ)Na23.  United States: N. p., 2015. 
Web.  doi:10.1103/PhysRevC.92.035805.

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                    Kelly, K. J., Champagne, A. E., Longland, R., & Buckner, M. Q. New recommended ωγ for the Erc.m.=458 keV resonance in Ne22(p,γ)Na23.  United States.  https://doi.org/10.1103/PhysRevC.92.035805

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                    Kelly, K. J., Champagne, A. E., Longland, R., and Buckner, M. Q. Fri .  
"New recommended ωγ for the Erc.m.=458 keV resonance in Ne22(p,γ)Na23".  United States.  https://doi.org/10.1103/PhysRevC.92.035805.  https://www.osti.gov/servlets/purl/1600485.

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@article{osti_1600485,

  title        = {New recommended ωγ for the Erc.m.=458 keV resonance in Ne22(p,γ)Na23},

  author       = {Kelly, K. J. and Champagne, A. E. and Longland, R. and Buckner, M. Q.},

  abstractNote = {The Erc.m.=458 keV resonance in Ne22(p,γ)Na23 is an ideal reference resonance for measurements of cross sections and resonance strengths in noble gas targets. We report on a new measurement of the strength of this resonance. Data analysis employed the TFractionFitter class of root combined with geant simulations of potential decay cascades from this resonance. This approach allowed us to extract precise primary branching ratios for decays from the resonant state, including a new primary branch to the 7082-keV state in Na23. Our new resonance strength of ωγ(458 keV) = 0.583(43) eV is more than 1σ higher than a recent high-precision result that relied on literature branching ratios.},

  doi          = {10.1103/PhysRevC.92.035805},

  journal      = {Physical Review C, Nuclear Physics},

  number       = 3,

  volume       = 92,

  place        = {United States},

  year         = {Fri Sep 04 00:00:00 EDT 2015},

  month        = {Fri Sep 04 00:00:00 EDT 2015}

}

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Title: New recommended ω γ for the E r c . m . = 458 keV resonance in Ne 22 ( p , γ ) Na 23

Abstract

Citation Formats

Measurement of the E r c.m. = 138 keV resonance in the 23 Na( p , γ ) 24 Mg reaction and the abundance of sodium in AGB stars journal, December 2013

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Ratio of germanium detector peak efficiencies at photon energies of 4.4 and 11.7MeV: Experiment versus simulation journal, June 2010

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Geant4—a simulation toolkit journal, July 2003

Nuclear Physics of Stars book, January 2007

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Fitting using finite Monte Carlo samples journal, October 1993

Monte Carlo simulation of the LENA detector system journal, November 2013

The N 14 ( p , γ ) O 15 reaction studied with a composite germanium detector journal, April 2011

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Measurement of the $E_{r}^{c.m.} = 138$ keV resonance in the $^{23}$ Na( $p$ , $γ$ ) $^{24}$ Mg reaction and the abundance of sodium in AGB stars
journal, December 2013

Coincidence summing in gamma-ray spectroscopy
journal, May 1990

Testing the equivalence of several algorithms for calculation of coincidence summing corrections
journal, October 2009

Intercomparison of methods for coincidence summing corrections in gamma-ray spectrometry
journal, July 2010

Nuclear astrophysics studies at LENA: The accelerators
journal, November 2010

Fast procedures for coincidence-summing correction in γ-ray spectrometry
journal, March 2000

Coincidence summing corrections in Ge(Li)-spectrometry at low source-to-detector distances
journal, January 1979

Supplement to energy levels of A = 21–44 nuclei (VII)
journal, April 1998

The energy levels of 23Na
journal, April 1973

Ratio of germanium detector peak efficiencies at photon energies of 4.4 and 11.7MeV: Experiment versus simulation
journal, June 2010

Experimental validation of coincidence summing corrections computed by the ETNA software
journal, October 2006

A tool for processing decay scheme data that encompasses coincidence summing calculations
journal, June 2008

Accurate computation of coincidence summing corrections in low level gamma-ray spectrometry
journal, July 2000

S-factor of 14N(p,γ)15O at astrophysical energies⋆
journal, September 2005

ROOT — An object oriented data analysis framework
journal, April 1997

Thermonuclear reaction rate of $^{18}$ O( $p$ , $γ$ ) $^{19}$ F
journal, December 2012

Energy levels of light nuclei A = 13–15
journal, February 1991

Nuclear astrophysics studies at the LENA facility: The -ray detection system
journal, October 2006

Monte Carlo simulation of the response of a germanium detector for low-level spectrometry measurements using GEANT4
journal, August 2004

Calculation of coincidence summing corrections for X-ray peaks and for sum peaks with X-ray contributions
journal, October 2006

A study of the excited states of23Na from the22Ne(p, γ)23Na reaction
journal, October 1971

Search for a resonance in the $^{14} N (p, γ)^{15} O$ reaction at $E_{p} = 127 keV$
journal, August 2002

High-intensity-beam study of ${}^{17}O (p, γ) {}^{18}F$ and thermonuclear reaction rates for ${}^{17}O + p$
journal, January 2015

Minuit - a system for function minimization and analysis of the parameter errors and correlations
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Nuclear Data Sheets for A = 23
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Astrophysical S-factor of 14N(p,γ)15O
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Resonance strength in ${}^{22}{Ne}$ ( $p, γ$ ) ${}^{23}{Na}$ from depth profiling in aluminum
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