Nuclear astrophysics studies at DRAGON: The 21Na(p,γ 22 reaction and oxygen-neon novae

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

doi:10.1016/S0375-9474(03)00726-7

Nuclear astrophysics studies at DRAGON: The ²¹Na(p,γ ²² reaction and oxygen-neon novae

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

D. Ottewell, P. D. Parker, J. Rogers, C. Wrede

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

1 Scopus citations

Abstract

The rate of the ²¹Na(p,γ)²²Mg reaction is expected to play a major role in the nucleosynthesis of ²²Na in Oxygen-Neon novae, leading to the emission of a characteristic 1.28 MeV gamma-line. This paper reports on preliminary results of the first direct measurements of this reaction and its astrophysical implications.

Original language	English
Pages (from-to)	263-266
Number of pages	4
Journal	Nuclear Physics, Section A
Volume	723
Issue number	1-2
DOIs	https://doi.org/10.1016/S0375-9474(03)00726-7
State	Published - 28 Jul 2003
Externally published	Yes

Access to Document

10.1016/S0375-9474(03)00726-7

Cite this

Bishop, S., Azuma, R., Buchmann, L., Chen, A. A., Chatterjee, M. L., D'Auria, J. M., Engel, S., Gigliotti, D., Greife, U., Hunter, D., Hussein, A., Hutcheon, D., Jewett, C., King, J., Kubono, S., Lamey, M., Lewis, R., Liu, W., Michimasa, S., ... Wrede, C. (2003). Nuclear astrophysics studies at DRAGON: The ²¹Na(p,γ ²² reaction and oxygen-neon novae. Nuclear Physics, Section A, 723(1-2), 263-266. https://doi.org/10.1016/S0375-9474(03)00726-7

@article{c06c0819ba44499f966765d95efdae50,

title = "Nuclear astrophysics studies at DRAGON: The 21Na(p,γ 22 reaction and oxygen-neon novae",

abstract = "The rate of the 21Na(p,γ)22Mg reaction is expected to play a major role in the nucleosynthesis of 22Na in Oxygen-Neon novae, leading to the emission of a characteristic 1.28 MeV gamma-line. This paper reports on preliminary results of the first direct measurements of this reaction and its astrophysical implications.",

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

year = "2003",

month = jul,

day = "28",

doi = "10.1016/S0375-9474(03)00726-7",

language = "English",

volume = "723",

pages = "263--266",

journal = "Nuclear Physics, Section A",

issn = "0375-9474",

publisher = "Elsevier B.V.",

number = "1-2",

}

Bishop, S, Azuma, R, Buchmann, L, Chen, AA, Chatterjee, ML, D'Auria, JM, Engel, S, Gigliotti, D, Greife, U, Hunter, D, Hussein, A, Hutcheon, D, Jewett, C, King, J, Kubono, S, Lamey, M, Lewis, R, Liu, W, Michimasa, S, Olin, A, Ottewell, D, Parker, PD, Rogers, J & Wrede, C 2003, 'Nuclear astrophysics studies at DRAGON: The ²¹Na(p,γ ²² reaction and oxygen-neon novae', Nuclear Physics, Section A, vol. 723, no. 1-2, pp. 263-266. https://doi.org/10.1016/S0375-9474(03)00726-7

TY - JOUR

T1 - Nuclear astrophysics studies at DRAGON

T2 - The 21Na(p,γ 22 reaction and oxygen-neon novae

AU - Bishop, S.

AU - Azuma, R.

AU - Buchmann, L.

AU - Chen, A. A.

AU - Chatterjee, M. L.

AU - D'Auria, J. M.

AU - Engel, S.

AU - Gigliotti, D.

AU - Greife, U.

AU - Hunter, D.

AU - Hussein, A.

AU - Hutcheon, D.

AU - Jewett, C.

AU - King, J.

AU - Kubono, S.

AU - Lamey, M.

AU - Lewis, R.

AU - Liu, W.

AU - Michimasa, S.

AU - Olin, A.

AU - Ottewell, D.

AU - Parker, P. D.

AU - Rogers, J.

AU - Wrede, C.

PY - 2003/7/28

Y1 - 2003/7/28

N2 - The rate of the 21Na(p,γ)22Mg reaction is expected to play a major role in the nucleosynthesis of 22Na in Oxygen-Neon novae, leading to the emission of a characteristic 1.28 MeV gamma-line. This paper reports on preliminary results of the first direct measurements of this reaction and its astrophysical implications.

AB - The rate of the 21Na(p,γ)22Mg reaction is expected to play a major role in the nucleosynthesis of 22Na in Oxygen-Neon novae, leading to the emission of a characteristic 1.28 MeV gamma-line. This paper reports on preliminary results of the first direct measurements of this reaction and its astrophysical implications.

UR - https://www.scopus.com/pages/publications/0038181110

U2 - 10.1016/S0375-9474(03)00726-7

DO - 10.1016/S0375-9474(03)00726-7

M3 - Article

AN - SCOPUS:0038181110

SN - 0375-9474

VL - 723

SP - 263

EP - 266

JO - Nuclear Physics, Section A

JF - Nuclear Physics, Section A

IS - 1-2

ER -

Nuclear astrophysics studies at DRAGON: The ²¹Na(p,γ ²² reaction and oxygen-neon novae

Abstract

Access to Document

Other files and links

Fingerprint

Cite this