The 21Na(p, γ)22Mg reaction from E c.m.=200 to 1103 keV in novae and x-ray bursts

J. M. D'Auria; R. E. Azuma; S. Bishop; L. Buchmann; M. L. Chatterjee; A. A. Chen; S. Engel; D. Gigliotti; U. Greife; D. Hunter; A. Hussein; D. Hutcheon; C. C. Jewett; J. José; J. D. King; A. M. Laird; M. Lamey; R. Lewis; W. Liu; A. Olin; D. Ottewell; P. Parker; J. Rogers; C. Ruiz; M. Trinczek; C. Wrede

doi:10.1103/PhysRevC.69.065803

The ²¹Na(p, γ)²²Mg reaction from E _c.m.=200 to 1103 keV in novae and x-ray bursts

J. M. D'Auria
, R. E. Azuma
, S. Bishop
, L. Buchmann
, M. L. Chatterjee
, A. A. Chen
, S. Engel
, D. Gigliotti
, U. Greife
, D. Hunter
, A. Hussein
, D. Hutcheon
, C. C. Jewett
, J. José
, J. D. King
, A. M. Laird
, M. Lamey
, R. Lewis
, W. Liu
, A. Olin

D. Ottewell, P. Parker, J. Rogers, C. Ruiz, M. Trinczek, C. Wrede

Simon Fraser University
University of Toronto
Riken
TRIUMF
Saha Institute of Nuclear Physics
McMaster University
Max-Planck-lnstitut für Kohlenforschung
Univ. of Northern British Columbia
Colorado School of Mines
Langara College
UPC BarcelonaTech
University of York
Yale University

Publikation: Beitrag in Fachzeitschrift › Artikel › Begutachtung

87 Zitate (Scopus)

Abstract

The long-lived radioactive nuclide ²²Na (t_1/2=2.6 yr) is an astronomical observable for understanding the physical processes of oxygen-neon novae. Yields of ²²Na in these events are sensitive to the unknown total rate of the ²¹Na(p, γ)²²Mg reaction. Using a high intensity ²¹Na beam at the TRIUMF-ISAC facility, the strengths of seven resonances in ²²Mg, of potential astrophysical importance, have been directly measured at center of mass energies from E_c.m.=200 to 1103 keV. We report the results obtained for these resonances and their respective contributions to the ²¹Na(p, γ)²²Mg rate in novae and x-ray bursts, and their impact on ²²Na production in novae.

Originalsprache	Englisch
Aufsatznummer	065803
Seiten (von - bis)	065803-1-065803-16
Fachzeitschrift	Physical Review C - Nuclear Physics
Jahrgang	69
Ausgabenummer	6
DOIs	https://doi.org/10.1103/PhysRevC.69.065803
Publikationsstatus	Veröffentlicht - Juni 2004
Extern publiziert	Ja

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10.1103/PhysRevC.69.065803

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D'Auria, J. M., Azuma, R. E., Bishop, S., Buchmann, L., Chatterjee, M. L., Chen, A. A., Engel, S., Gigliotti, D., Greife, U., Hunter, D., Hussein, A., Hutcheon, D., Jewett, C. C., José, J., King, J. D., Laird, A. M., Lamey, M., Lewis, R., Liu, W., ... Wrede, C. (2004). The ²¹Na(p, γ)²²Mg reaction from E _c.m.=200 to 1103 keV in novae and x-ray bursts. Physical Review C - Nuclear Physics, 69(6), 065803-1-065803-16. Artikel 065803. https://doi.org/10.1103/PhysRevC.69.065803

@article{727e9418e50c41f3a9f4ba1809884249,

title = "The 21Na(p, γ)22Mg reaction from E c.m.=200 to 1103 keV in novae and x-ray bursts",

abstract = "The long-lived radioactive nuclide 22Na (t1/2=2.6 yr) is an astronomical observable for understanding the physical processes of oxygen-neon novae. Yields of 22Na in these events are sensitive to the unknown total rate of the 21Na(p, γ)22Mg reaction. Using a high intensity 21Na beam at the TRIUMF-ISAC facility, the strengths of seven resonances in 22Mg, of potential astrophysical importance, have been directly measured at center of mass energies from Ec.m.=200 to 1103 keV. We report the results obtained for these resonances and their respective contributions to the 21Na(p, γ)22Mg rate in novae and x-ray bursts, and their impact on 22Na production in novae.",

author = "D'Auria, \{J. M.\} and Azuma, \{R. E.\} and S. Bishop and L. Buchmann and Chatterjee, \{M. L.\} and Chen, \{A. A.\} and S. Engel and D. Gigliotti and U. Greife and D. Hunter and A. Hussein and D. Hutcheon and Jewett, \{C. C.\} and J. Jos{\'e} and King, \{J. D.\} and Laird, \{A. M.\} and M. Lamey and R. Lewis and W. Liu and A. Olin and D. Ottewell and P. Parker and J. Rogers and C. Ruiz and M. Trinczek and C. Wrede",

note = "Funding Information: The DRAGON group thanks the TRIUMF staff for their support. They are the hidden heroes that keep the facility going, particularly in the machine and electronics shops, computer support, beam lines, controls group, design office, cyclotron division, and the ISAC operations group. Special thanks go to the accelerator physicists, R. Laxdal, Z. Peng, and M. Pasini, for the tuning of the beam and M. Dombsky for the radioactive beam production. Financial support received from the Natural Sciences and Engineering Research Council of Canada, from the U.S. Department of Energy (DE-FG03-93ER40789 and DE-FG02-91ER40609), and from TRIUMF is gratefully acknowledged.",

year = "2004",

month = jun,

doi = "10.1103/PhysRevC.69.065803",

language = "English",

volume = "69",

pages = "065803--1--065803--16",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

publisher = "American Physical Society",

number = "6",

}

D'Auria, JM, Azuma, RE, Bishop, S, Buchmann, L, Chatterjee, ML, Chen, AA, Engel, S, Gigliotti, D, Greife, U, Hunter, D, Hussein, A, Hutcheon, D, Jewett, CC, José, J, King, JD, Laird, AM, Lamey, M, Lewis, R, Liu, W, Olin, A, Ottewell, D, Parker, P, Rogers, J, Ruiz, C, Trinczek, M & Wrede, C 2004, 'The ²¹Na(p, γ)²²Mg reaction from E _c.m.=200 to 1103 keV in novae and x-ray bursts', Physical Review C - Nuclear Physics, Jg. 69, Nr. 6, 065803, S. 065803-1-065803-16. https://doi.org/10.1103/PhysRevC.69.065803

TY - JOUR

T1 - The 21Na(p, γ)22Mg reaction from E c.m.=200 to 1103 keV in novae and x-ray bursts

AU - D'Auria, J. M.

AU - Azuma, R. E.

AU - Bishop, S.

AU - Buchmann, L.

AU - Chatterjee, M. L.

AU - Chen, A. A.

AU - Engel, S.

AU - Gigliotti, D.

AU - Greife, U.

AU - Hunter, D.

AU - Hussein, A.

AU - Hutcheon, D.

AU - Jewett, C. C.

AU - José, J.

AU - King, J. D.

AU - Laird, A. M.

AU - Lamey, M.

AU - Lewis, R.

AU - Liu, W.

AU - Olin, A.

AU - Ottewell, D.

AU - Parker, P.

AU - Rogers, J.

AU - Ruiz, C.

AU - Trinczek, M.

AU - Wrede, C.

N1 - Funding Information: The DRAGON group thanks the TRIUMF staff for their support. They are the hidden heroes that keep the facility going, particularly in the machine and electronics shops, computer support, beam lines, controls group, design office, cyclotron division, and the ISAC operations group. Special thanks go to the accelerator physicists, R. Laxdal, Z. Peng, and M. Pasini, for the tuning of the beam and M. Dombsky for the radioactive beam production. Financial support received from the Natural Sciences and Engineering Research Council of Canada, from the U.S. Department of Energy (DE-FG03-93ER40789 and DE-FG02-91ER40609), and from TRIUMF is gratefully acknowledged.

PY - 2004/6

Y1 - 2004/6

N2 - The long-lived radioactive nuclide 22Na (t1/2=2.6 yr) is an astronomical observable for understanding the physical processes of oxygen-neon novae. Yields of 22Na in these events are sensitive to the unknown total rate of the 21Na(p, γ)22Mg reaction. Using a high intensity 21Na beam at the TRIUMF-ISAC facility, the strengths of seven resonances in 22Mg, of potential astrophysical importance, have been directly measured at center of mass energies from Ec.m.=200 to 1103 keV. We report the results obtained for these resonances and their respective contributions to the 21Na(p, γ)22Mg rate in novae and x-ray bursts, and their impact on 22Na production in novae.

AB - The long-lived radioactive nuclide 22Na (t1/2=2.6 yr) is an astronomical observable for understanding the physical processes of oxygen-neon novae. Yields of 22Na in these events are sensitive to the unknown total rate of the 21Na(p, γ)22Mg reaction. Using a high intensity 21Na beam at the TRIUMF-ISAC facility, the strengths of seven resonances in 22Mg, of potential astrophysical importance, have been directly measured at center of mass energies from Ec.m.=200 to 1103 keV. We report the results obtained for these resonances and their respective contributions to the 21Na(p, γ)22Mg rate in novae and x-ray bursts, and their impact on 22Na production in novae.

UR - https://www.scopus.com/pages/publications/4143127856

U2 - 10.1103/PhysRevC.69.065803

DO - 10.1103/PhysRevC.69.065803

M3 - Article

AN - SCOPUS:4143127856

SN - 0556-2813

VL - 69

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JO - Physical Review C - Nuclear Physics

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