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.

引用

页码：263C / 266C

页数：4