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

被引：0
|
作者：
Bishop, S [1 ]
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
机构：
[1] Simon Fraser Univ, Burnaby, BC V5A 1S6, Canada
[2] Univ Toronto, Toronto, ON, Canada
[3] TRIUMF, Vancouver, BC, Canada
[4] Saha Inst Nucl Phys, Kolkata 700009, W Bengal, India
[5] Ruhr Univ Bochum, D-4630 Bochum, Germany
[6] Univ No British Columbia, Prince George, BC V2L 5P2, Canada
[7] Colorado Sch Mines, Golden, CO 80401 USA
[8] Univ Tokyo, Tokyo, Japan
[9] Yale Univ, New Haven, CT USA
来源：
NUCLEAR PHYSICS A | 2003年 / 718卷
关键词：
D O I：
10.1016/S0375-9474(03)00726-7
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
The rate of the Na-21(p,gamma)Mg-22 reaction is expected to play a major role in the nucleosynthesis of Na-22 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.
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收藏
页码：263C / 266C
页数：4
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