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Title: Low energy scattering cross section ratios of N 14 ( p , p ) N 14

Abstract

Background: The slowest reaction in the first CNO cycle is 14N(p, γ) 15O, therefore its rate determines the overall energy production efficiency of the entire cycle. The cross section presents several strong resonance contributions, especially for the ground-state transition. Some of the properties of the corresponding levels in the 15O compound nucleus remain uncertain, which affects the uncertainty in extrapolating the capture cross section to the low energy range of astrophysical interest. Purpose: The 14N (p, γ) 15O cross section can be described by using the phenomenological R matrix. Over the energy range of interest, only the proton and γ-ray channels are open. Since resonance capture makes significant contributions to the 14N (p, γ) 15O cross section, resonant proton scattering data can be used to provide additional constraints on the R-matrix fit of the capture data. Methods: A 4 MV KN Van de Graaff accelerator was used to bombard protons onto a windowless gas target containing enriched 14N gas over the proton energy range from Ep =1.0 to 3.0 MeV. Scattered protons were detected at θlab = 90,120°,135 °,150°, and 160° using ruggedized silicon detectors. In addition, a 10 MV FN Tandem Van de Graaff accelerator was used to acceleratemore » protons onto a solid Adenine ( C 5 H 5 N 5 ) target, of natural isotopic abundance, evaporated onto a thin self-supporting carbon backing, over the energy range from E p = 1.8 to 4.0 MeV. Scattered protons were detected at 28 angles between θ lab = 30. 4° and 167. 7° by using silicon photodiode detectors. Results: Relative cross sections were extracted from both measurements. While the relative cross sections do not provide as much constraint as absolute measurements, they greatly reduce the dependence of the data on otherwise significant systematic uncertainties, which are more difficult to quantify. The data are fit simultaneously using an R-matrix analysis and level energies and proton widths are extracted. Even with relative measurements, the statistics and large angular coverage of the measurements result in more confident values for the energies and proton widths of several levels; in particular, the broad resonance at Ec.m. = 2.21 MeV, which corresponds to the 3/2+ level at Ex = 9.51 MeV in 15O. In particular, the s - and d -wave angular-momentum channels are separated. Conclusion: The relative cross sections provide a consistent set of data that can be used to better constrain a full multichannel R-matrix extrapolation of the capture data. It has been demonstrated how the scattering data reduce the uncertainty through a preliminary Monte Carlo uncertainty analysis, but several other issues remain that make large contributions to the uncertainty, which must be addressed by further capture and lifetime measurements.« less

Authors:
 [1];  [1];  [1];  [1];  [1];  [1];  [1];  [1];  [1];  [1];  [2];  [2];  [3]
  1. Univ. of Notre Dame, IN (United States). Joint Inst. for Nuclear Astrophysics
  2. Univ. of North Carolina, Chapel Hill, NC (United States); Triangle Universities Nuclear Lab., Durham, NC (United States)
  3. Ball State Univ., Muncie, IN (United States)
Publication Date:
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:
1600481
Alternate Identifier(s):
OSTI ID: 1178478
Grant/Contract Number:  
FG02-97ER41041
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review C, Nuclear Physics
Additional Journal Information:
Journal Volume: 91; Journal Issue: 4; 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

deBoer, R. J., Bardayan, D. W., Görres, J., LeBlanc, P. J., Manukyan, K. V., Moran, M. T., Smith, K., Tan, W., Uberseder, E., Wiescher, M., Bertone, P. F., Champagne, A. E., and Islam, M. S. Low energy scattering cross section ratios of N14(p,p)N14. United States: N. p., 2015. Web. doi:10.1103/PhysRevC.91.045804.
deBoer, R. J., Bardayan, D. W., Görres, J., LeBlanc, P. J., Manukyan, K. V., Moran, M. T., Smith, K., Tan, W., Uberseder, E., Wiescher, M., Bertone, P. F., Champagne, A. E., & Islam, M. S. Low energy scattering cross section ratios of N14(p,p)N14. United States. https://doi.org/10.1103/PhysRevC.91.045804
deBoer, R. J., Bardayan, D. W., Görres, J., LeBlanc, P. J., Manukyan, K. V., Moran, M. T., Smith, K., Tan, W., Uberseder, E., Wiescher, M., Bertone, P. F., Champagne, A. E., and Islam, M. S. Mon . "Low energy scattering cross section ratios of N14(p,p)N14". United States. https://doi.org/10.1103/PhysRevC.91.045804. https://www.osti.gov/servlets/purl/1600481.
@article{osti_1600481,
title = {Low energy scattering cross section ratios of N14(p,p)N14},
author = {deBoer, R. J. and Bardayan, D. W. and Görres, J. and LeBlanc, P. J. and Manukyan, K. V. and Moran, M. T. and Smith, K. and Tan, W. and Uberseder, E. and Wiescher, M. and Bertone, P. F. and Champagne, A. E. and Islam, M. S.},
abstractNote = {Background: The slowest reaction in the first CNO cycle is 14N(p, γ) 15O, therefore its rate determines the overall energy production efficiency of the entire cycle. The cross section presents several strong resonance contributions, especially for the ground-state transition. Some of the properties of the corresponding levels in the 15O compound nucleus remain uncertain, which affects the uncertainty in extrapolating the capture cross section to the low energy range of astrophysical interest. Purpose: The 14N (p, γ) 15O cross section can be described by using the phenomenological R matrix. Over the energy range of interest, only the proton and γ-ray channels are open. Since resonance capture makes significant contributions to the 14N (p, γ) 15O cross section, resonant proton scattering data can be used to provide additional constraints on the R-matrix fit of the capture data. Methods: A 4 MV KN Van de Graaff accelerator was used to bombard protons onto a windowless gas target containing enriched 14N gas over the proton energy range from Ep =1.0 to 3.0 MeV. Scattered protons were detected at θlab = 90,120°,135 °,150°, and 160° using ruggedized silicon detectors. In addition, a 10 MV FN Tandem Van de Graaff accelerator was used to accelerate protons onto a solid Adenine ( C 5 H 5 N 5 ) target, of natural isotopic abundance, evaporated onto a thin self-supporting carbon backing, over the energy range from E p = 1.8 to 4.0 MeV. Scattered protons were detected at 28 angles between θ lab = 30. 4° and 167. 7° by using silicon photodiode detectors. Results: Relative cross sections were extracted from both measurements. While the relative cross sections do not provide as much constraint as absolute measurements, they greatly reduce the dependence of the data on otherwise significant systematic uncertainties, which are more difficult to quantify. The data are fit simultaneously using an R-matrix analysis and level energies and proton widths are extracted. Even with relative measurements, the statistics and large angular coverage of the measurements result in more confident values for the energies and proton widths of several levels; in particular, the broad resonance at Ec.m. = 2.21 MeV, which corresponds to the 3/2+ level at Ex = 9.51 MeV in 15O. In particular, the s - and d -wave angular-momentum channels are separated. Conclusion: The relative cross sections provide a consistent set of data that can be used to better constrain a full multichannel R-matrix extrapolation of the capture data. It has been demonstrated how the scattering data reduce the uncertainty through a preliminary Monte Carlo uncertainty analysis, but several other issues remain that make large contributions to the uncertainty, which must be addressed by further capture and lifetime measurements.},
doi = {10.1103/PhysRevC.91.045804},
journal = {Physical Review C, Nuclear Physics},
number = 4,
volume = 91,
place = {United States},
year = {Mon Apr 20 00:00:00 EDT 2015},
month = {Mon Apr 20 00:00:00 EDT 2015}
}

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Works referenced in this record:

R-Matrix Theory of Nuclear Reactions
journal, April 1958


Age Estimates of Globular Clusters in the Milky Way: Constraints on Cosmology
journal, January 2003


Asymptotic normalization coefficients for 14 N + p 15 O and the astrophysical S factor for 14 N ( p , γ ) 15 O
journal, June 2003


Measurement of elastic C 12 + α scattering: Details of the experiment, analysis, and discussion of phase shifts
journal, May 2009


The R -matrix theory
journal, February 2010


Evaluation of non-Rutherford proton elastic scattering cross section for nitrogen
journal, April 2008

  • Gurbich, A.
  • Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, Vol. 266, Issue 8
  • DOI: 10.1016/j.nimb.2007.11.026

Helium burning of22Ne
journal, December 1989

  • Wolke, K.; Harms, V.; Becker, H. W.
  • Zeitschrift f�r Physik A Atomic Nuclei, Vol. 334, Issue 4
  • DOI: 10.1007/BF01294757

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


The 14N(p,)15O low-energy -factor
journal, July 2001


Solar Neutrinos: Status and Prospects
journal, August 2013


Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars
journal, June 1987


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


Measurement of elastic 12 C + α scattering: Above the proton separation energy
journal, April 2012


Alternative parametrization of R -matrix theory
journal, October 2002


Connection between asymptotic normalization coefficients, subthreshold bound states, and resonances
journal, June 1999


Solar fusion cross sections. II. The p p chain and CNO cycles
journal, April 2011

  • Adelberger, E. G.; García, A.; Robertson, R. G. Hamish
  • Reviews of Modern Physics, Vol. 83, Issue 1
  • DOI: 10.1103/RevModPhys.83.195

Minuit - a system for function minimization and analysis of the parameter errors and correlations
journal, December 1975


Low-energy-threshold analysis of the Phase I and Phase II data sets of the Sudbury Neutrino Observatory
journal, May 2010


Direct Measurement of the N 14 ( p , γ ) O 15 S Factor
journal, March 2005


Lifetime of the 6793-keV State in O 15
journal, September 2001


N 22 e ( α , n ) M 25 g : The Key Neutron Source in Massive Stars
journal, October 2001


E1 strength of the subthreshold 3/2+ state in 15O studied by Coulomb excitation
journal, January 2004


14 N ( 3 He , d ) 15 O as a probe of direct capture in the 14 N ( p , γ ) 15 O reaction
journal, November 2002


Monte Carlo uncertainty of the He 3 ( α , γ ) Be 7 reaction rate
journal, September 2014


AZURE: An R -matrix code for nuclear astrophysics
journal, April 2010


Precision Measurement of the Be 7 Solar Neutrino Interaction Rate in Borexino
journal, September 2011


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New investigations of the 10 B(p,${\alpha }_{0}$) 7 Be reaction at bombarding energies between 0.6 and 1 MeV
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  • Lombardo, I.; Dell’Aquila, D.; Conte, F.
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 43, Issue 4
  • DOI: 10.1088/0954-3899/43/4/045109

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