Using 19F(3He, t)19Ne∗(γ) to study astrophysically important levels near the 18F+ p threshold

M. R. Hall; D. W. Bardayan; S. Ahn; J. M. Allen; J. T. Anderson; A. D. Ayangeakaa; T. Baugher; J. C. Blackmon; D. Blankstein; S. Burcher; M. P. Carpenter; S. M. Cha; K. Y. Chae; K. A. Chipps; J. A. Cizewski; M. Febbraro; B. Frentz; O. Hall; S. L. Henderson; J. Hu; C. L. Jiang; K. L. Jones; E. J. Lee; A. Lepailleur; D. S. Monteiro; P. D. O'Malley; S. Ota; S. D. Pain; B. C. Rasco; A. Ratkiewicz; J. Riggins; D. Santiago-Gonzalez; D. Seweryniak; A. Simon; H. Sims; K. Smith; W. P. Tan; P. Thompson; C. Thornsberry; R. O. Torres-Isea; B. Vande Kolk; R. L. Varner; D. Walter; G. L. Wilson; S. Zhu

doi:10.1063/1.5127732

Using ¹⁹F(³He, t)¹⁹Ne^∗(γ) to study astrophysically important levels near the ¹⁸F+ p threshold

M. R. Hall, D. W. Bardayan, S. Ahn, J. M. Allen, J. T. Anderson, A. D. Ayangeakaa, T. Baugher, J. C. Blackmon, D. Blankstein, S. Burcher, M. P. Carpenter, S. M. Cha, K. Y. Chae, K. A. Chipps, J. A. Cizewski, M. Febbraro, B. Frentz, O. Hall, S. L. Henderson, J. HuC. L. Jiang, K. L. Jones, E. J. Lee, A. Lepailleur, D. S. Monteiro, P. D. O'Malley, S. Ota, S. D. Pain, B. C. Rasco, A. Ratkiewicz, J. Riggins, D. Santiago-Gonzalez, D. Seweryniak, A. Simon, H. Sims, K. Smith, W. P. Tan, P. Thompson, C. Thornsberry, R. O. Torres-Isea, B. Vande Kolk, R. L. Varner, D. Walter, G. L. Wilson, S. Zhu

Nuclear Structure and Nuclear Astrophysi

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

1 Scopus citations

Abstract

A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, ¹⁸F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of ¹⁸F is thought to be the ¹⁸F(p,α)¹⁵O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in ¹⁹Ne above the ¹⁸F+p threshold. To measure the properties of these levels, the ¹⁹F(³He,t)¹⁹Ne^-(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.

Original language	English
Title of host publication	25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018
Publisher	American Institute of Physics Inc.
ISBN (Electronic)	9780735419056
DOIs	https://doi.org/10.1063/1.5127732
State	Published - Oct 2 2019
Event	25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018 - Grapevine, United States Duration: Aug 12 2018 → Aug 17 2018

Publication series

Name	AIP Conference Proceedings
Volume	2160
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018
Country/Territory	United States
City	Grapevine
Period	08/12/18 → 08/17/18

Funding

This work was supported in part by the National Science Foundation Grant Number PHY-1419765, the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Cooperative Agreement DE-NA002132. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under contract numbers DE-AC02-06CH11357, DE-AC05-00OR22725, DE-FG02-96ER40963, and DE-FG02-96ER40978. This research used resources of ANL’s ATLAS facility, which is a DOE Office of Science User Facility. The authors would like to thank the ATLAS staff for their support during the GODDESS campaign and the Clovershare collaboration for providing the HPGe clover detectors. This work was supported in part by the National Science Foundation Grant Number PHY-1419765, the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Cooperative Agreement DE-NA002132. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under contract numbers DE-AC02-06CH11357, DE-AC05-00OR22725, DE-FG02-96ER40963, and DE-FG02-96ER40978. This research used resources of ANL's ATLAS facility, which is a DOE Office of Science User Facility. The authors would like to thank the ATLAS staff for their support during the GODDESS campaign and the Clovershare collaboration for providing the HPGe clover detectors.

Access to Document

10.1063/1.5127732

Cite this

Hall, M. R., Bardayan, D. W., Ahn, S., Allen, J. M., Anderson, J. T., Ayangeakaa, A. D., Baugher, T., Blackmon, J. C., Blankstein, D., Burcher, S., Carpenter, M. P., Cha, S. M., Chae, K. Y., Chipps, K. A., Cizewski, J. A., Febbraro, M., Frentz, B., Hall, O., Henderson, S. L., ... Zhu, S. (2019). Using ¹⁹F(³He, t)¹⁹Ne^∗(γ) to study astrophysically important levels near the ¹⁸F+ p threshold. In 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018 Article 070009 (AIP Conference Proceedings; Vol. 2160). American Institute of Physics Inc.. https://doi.org/10.1063/1.5127732

@inproceedings{00c6bbad0f424b17a96042b247f8c5a7,

title = "Using 19F(3He, t)19Ne∗(γ) to study astrophysically important levels near the 18F+ p threshold",

abstract = "A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne-(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.",

author = "Hall, {M. R.} and Bardayan, {D. W.} and S. Ahn and Allen, {J. M.} and Anderson, {J. T.} and Ayangeakaa, {A. D.} and T. Baugher and Blackmon, {J. C.} and D. Blankstein and S. Burcher and Carpenter, {M. P.} and Cha, {S. M.} and Chae, {K. Y.} and Chipps, {K. A.} and Cizewski, {J. A.} and M. Febbraro and B. Frentz and O. Hall and Henderson, {S. L.} and J. Hu and Jiang, {C. L.} and Jones, {K. L.} and Lee, {E. J.} and A. Lepailleur and Monteiro, {D. S.} and O'Malley, {P. D.} and S. Ota and Pain, {S. D.} and Rasco, {B. C.} and A. Ratkiewicz and J. Riggins and D. Santiago-Gonzalez and D. Seweryniak and A. Simon and H. Sims and K. Smith and Tan, {W. P.} and P. Thompson and C. Thornsberry and Torres-Isea, {R. O.} and {Vande Kolk}, B. and Varner, {R. L.} and D. Walter and Wilson, {G. L.} and S. Zhu",

note = "Publisher Copyright: {\textcopyright} 2019 Author(s).; 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018 ; Conference date: 12-08-2018 Through 17-08-2018",

year = "2019",

month = oct,

day = "2",

doi = "10.1063/1.5127732",

language = "English",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

booktitle = "25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018",

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Hall, MR, Bardayan, DW, Ahn, S, Allen, JM, Anderson, JT, Ayangeakaa, AD, Baugher, T, Blackmon, JC, Blankstein, D, Burcher, S, Carpenter, MP, Cha, SM, Chae, KY, Chipps, KA, Cizewski, JA, Febbraro, M, Frentz, B, Hall, O, Henderson, SL, Hu, J, Jiang, CL, Jones, KL, Lee, EJ, Lepailleur, A, Monteiro, DS, O'Malley, PD, Ota, S, Pain, SD, Rasco, BC, Ratkiewicz, A, Riggins, J, Santiago-Gonzalez, D, Seweryniak, D, Simon, A, Sims, H, Smith, K, Tan, WP, Thompson, P, Thornsberry, C, Torres-Isea, RO, Vande Kolk, B, Varner, RL, Walter, D, Wilson, GL & Zhu, S 2019, Using ¹⁹F(³He, t)¹⁹Ne^∗(γ) to study astrophysically important levels near the ¹⁸F+ p threshold. in 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018., 070009, AIP Conference Proceedings, vol. 2160, American Institute of Physics Inc., 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018, Grapevine, United States, 08/12/18. https://doi.org/10.1063/1.5127732

Using ¹⁹F(³He, t)¹⁹Ne^∗(γ) to study astrophysically important levels near the ¹⁸F+ p threshold. / Hall, M. R.; Bardayan, D. W.; Ahn, S. et al.
25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018. American Institute of Physics Inc., 2019. 070009 (AIP Conference Proceedings; Vol. 2160).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Using 19F(3He, t)19Ne∗(γ) to study astrophysically important levels near the 18F+ p threshold

AU - Hall, M. R.

AU - Bardayan, D. W.

AU - Ahn, S.

AU - Allen, J. M.

AU - Anderson, J. T.

AU - Ayangeakaa, A. D.

AU - Baugher, T.

AU - Blackmon, J. C.

AU - Blankstein, D.

AU - Burcher, S.

AU - Carpenter, M. P.

AU - Cha, S. M.

AU - Chae, K. Y.

AU - Chipps, K. A.

AU - Cizewski, J. A.

AU - Febbraro, M.

AU - Frentz, B.

AU - Hall, O.

AU - Henderson, S. L.

AU - Hu, J.

AU - Jiang, C. L.

AU - Jones, K. L.

AU - Lee, E. J.

AU - Lepailleur, A.

AU - Monteiro, D. S.

AU - O'Malley, P. D.

AU - Ota, S.

AU - Pain, S. D.

AU - Rasco, B. C.

AU - Ratkiewicz, A.

AU - Riggins, J.

AU - Santiago-Gonzalez, D.

AU - Seweryniak, D.

AU - Simon, A.

AU - Sims, H.

AU - Smith, K.

AU - Tan, W. P.

AU - Thompson, P.

AU - Thornsberry, C.

AU - Torres-Isea, R. O.

AU - Vande Kolk, B.

AU - Varner, R. L.

AU - Walter, D.

AU - Wilson, G. L.

AU - Zhu, S.

PY - 2019/10/2

Y1 - 2019/10/2

N2 - A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne-(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.

AB - A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne-(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.

UR - http://www.scopus.com/inward/record.url?scp=85074249956&partnerID=8YFLogxK

U2 - 10.1063/1.5127732

DO - 10.1063/1.5127732

M3 - Conference contribution

AN - SCOPUS:85074249956

T3 - AIP Conference Proceedings

BT - 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018

PB - American Institute of Physics Inc.

T2 - 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018

Y2 - 12 August 2018 through 17 August 2018

ER -

Hall MR, Bardayan DW, Ahn S, Allen JM, Anderson JT, Ayangeakaa AD et al. Using ¹⁹F(³He, t)¹⁹Ne^∗(γ) to study astrophysically important levels near the ¹⁸F+ p threshold. In 25th International Conference on the Application of Accelerators in Research and Industry, CAARI 2018. American Institute of Physics Inc. 2019. 070009. (AIP Conference Proceedings). doi: 10.1063/1.5127732