Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate

D. W. Bardayan; K. A. Chipps; S. Ahn; J. C. Blackmon; S. Carmichael; U. Greife; K. L. Jones; J. José; A. Kontos; R. L. Kozub; L. Linhardt; B. Manning; M. Matoš; P. D. O'Malley; S. Ota; S. D. Pain; W. A. Peters; S. T. Pittman; A. Sachs; K. T. Schmitt; M. S. Smith; P. Thompson

doi:10.1103/PhysRevC.96.055806

Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate

D. W. Bardayan
, K. A. Chipps
, S. Ahn
, J. C. Blackmon
, S. Carmichael
, U. Greife
, K. L. Jones
, J. José
, A. Kontos
, R. L. Kozub
, L. Linhardt
, B. Manning
, M. Matoš
, P. D. O'Malley
, S. Ota
, S. D. Pain
, W. A. Peters
, S. T. Pittman
, A. Sachs
, K. T. Schmitt

M. S. Smith, P. Thompson

Research output: Contribution to journal › Article › peer-review

8 Scopus citations

Abstract

The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target was used to perform spectroscopic studies of Ne20+p reactions. Levels in Ne19 were probed via the Ne20(p,d)Ne19 reaction to constrain the astrophysical rate of the F18(p,α)O15 reaction. Additionally, the first spectroscopic study of the Ne20(p,He3)F18 reaction was performed. Angular distribution data were used to determine or confirm the spins of several previously observed levels, and the existence of a strong subthreshold F18(p,α)O15 resonance was verified.

Original language	English
Article number	055806
Journal	Physical Review C
Volume	96
Issue number	5
DOIs	https://doi.org/10.1103/PhysRevC.96.055806
State	Published - Nov 16 2017

Funding

This work was supported in part by the US Department of Energy under Contracts No. DE-FG02-10ER41704, No. DE-FG02-93ER40789 (CSM), No. DE-FG52-08NA28552 (Rutgers), No. DE-FG02-96ER40983 (UTK), No. DE-FG02-96ER40955 (TTU) and No. DE-AC05-00OR22725 (ORNL), and by the National Science Foundation under Contracts No. PHY-1419765 (Notre Dame) and No. PHY-0822648 (JINA). J.J. acknowledges partial support by the Spanish MINECO Grant No. AYA201459084P, and by the AGAUR/Generalitat de Catalunya Grant No. SGR0038/2014.

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Bardayan, D. W., Chipps, K. A., Ahn, S., Blackmon, J. C., Carmichael, S., Greife, U., Jones, K. L., José, J., Kontos, A., Kozub, R. L., Linhardt, L., Manning, B., Matoš, M., O'Malley, P. D., Ota, S., Pain, S. D., Peters, W. A., Pittman, S. T., Sachs, A., ... Thompson, P. (2017). Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate. Physical Review C, 96(5), Article 055806. https://doi.org/10.1103/PhysRevC.96.055806

@article{80fb542b3f7d47d28c55b8497fc949d5,

title = "Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate",

abstract = "The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target was used to perform spectroscopic studies of Ne20+p reactions. Levels in Ne19 were probed via the Ne20(p,d)Ne19 reaction to constrain the astrophysical rate of the F18(p,α)O15 reaction. Additionally, the first spectroscopic study of the Ne20(p,He3)F18 reaction was performed. Angular distribution data were used to determine or confirm the spins of several previously observed levels, and the existence of a strong subthreshold F18(p,α)O15 resonance was verified.",

author = "Bardayan, \{D. W.\} and Chipps, \{K. A.\} and S. Ahn and Blackmon, \{J. C.\} and S. Carmichael and U. Greife and Jones, \{K. L.\} and J. Jos{\'e} and A. Kontos and Kozub, \{R. L.\} and L. Linhardt and B. Manning and M. Mato{\v s} and O'Malley, \{P. D.\} and S. Ota and Pain, \{S. D.\} and Peters, \{W. A.\} and Pittman, \{S. T.\} and A. Sachs and Schmitt, \{K. T.\} and Smith, \{M. S.\} and P. Thompson",

note = "Publisher Copyright: {\textcopyright} 2017 American Physical Society.",

year = "2017",

month = nov,

day = "16",

doi = "10.1103/PhysRevC.96.055806",

language = "English",

volume = "96",

journal = "Physical Review C",

issn = "2469-9985",

publisher = "American Physical Society",

number = "5",

}

Bardayan, DW, Chipps, KA, Ahn, S, Blackmon, JC, Carmichael, S, Greife, U, Jones, KL, José, J, Kontos, A, Kozub, RL, Linhardt, L, Manning, B, Matoš, M, O'Malley, PD, Ota, S, Pain, SD, Peters, WA, Pittman, ST, Sachs, A, Schmitt, KT, Smith, MS & Thompson, P 2017, 'Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate', Physical Review C, vol. 96, no. 5, 055806. https://doi.org/10.1103/PhysRevC.96.055806

TY - JOUR

T1 - Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate

AU - Bardayan, D. W.

AU - Chipps, K. A.

AU - Ahn, S.

AU - Blackmon, J. C.

AU - Carmichael, S.

AU - Greife, U.

AU - Jones, K. L.

AU - José, J.

AU - Kontos, A.

AU - Kozub, R. L.

AU - Linhardt, L.

AU - Manning, B.

AU - Matoš, M.

AU - O'Malley, P. D.

AU - Ota, S.

AU - Pain, S. D.

AU - Peters, W. A.

AU - Pittman, S. T.

AU - Sachs, A.

AU - Schmitt, K. T.

AU - Smith, M. S.

AU - Thompson, P.

PY - 2017/11/16

Y1 - 2017/11/16

N2 - The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target was used to perform spectroscopic studies of Ne20+p reactions. Levels in Ne19 were probed via the Ne20(p,d)Ne19 reaction to constrain the astrophysical rate of the F18(p,α)O15 reaction. Additionally, the first spectroscopic study of the Ne20(p,He3)F18 reaction was performed. Angular distribution data were used to determine or confirm the spins of several previously observed levels, and the existence of a strong subthreshold F18(p,α)O15 resonance was verified.

AB - The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target was used to perform spectroscopic studies of Ne20+p reactions. Levels in Ne19 were probed via the Ne20(p,d)Ne19 reaction to constrain the astrophysical rate of the F18(p,α)O15 reaction. Additionally, the first spectroscopic study of the Ne20(p,He3)F18 reaction was performed. Angular distribution data were used to determine or confirm the spins of several previously observed levels, and the existence of a strong subthreshold F18(p,α)O15 resonance was verified.

UR - https://www.scopus.com/pages/publications/85036652205

U2 - 10.1103/PhysRevC.96.055806

DO - 10.1103/PhysRevC.96.055806

M3 - Article

AN - SCOPUS:85036652205

SN - 2469-9985

VL - 96

JO - Physical Review C

JF - Physical Review C

IS - 5

M1 - 055806

ER -

Spectroscopic study of Ne 20 +p reactions using the JENSA gas-jet target to constrain the astrophysical F 18 (p,α) O 15 rate

Abstract

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