Nucleosynthesis of gamma-ray emitter Al-26 in the Galxy
Project/Area Number |
21540295
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Research Category |
Grant-in-Aid for Scientific Research (C)
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Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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Research Institution | University of Tsukuba |
Principal Investigator |
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Co-Investigator(Renkei-kenkyūsha) |
HAYAKAWA Takehito 日本原子力研究開発機構, 研究主幹 (70343944)
SHIZUMA Toshiyuki 日本原子力研究開発機構, 研究主幹 (50282299)
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Project Period (FY) |
2009 – 2011
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Project Status |
Completed (Fiscal Year 2011)
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Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2011: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2010: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2009: ¥2,730,000 (Direct Cost: ¥2,100,000、Indirect Cost: ¥630,000)
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Keywords | 原子核(実験) / 宙元素合成 / アルミニウム26 / ガンマ線分光 / ガンマ線同時計数 / ガンマ線角度相関測定 / 原子核構造 / ゲルマニウム検出器 / 宇宙元素合 / ビッグバン / 原子核反応 / 原子核構 / ガンマ線 / スピン・パリティ / 超新星爆発 / Al-26 / 宇宙元素合成 |
Research Abstract |
Observation of gamma-rays originated from radioactive nucleus <26>^Al, whose half life is 720 thousand yr, is the crucial proof of nuclear synthesis in the Galaxy. In order to reproduce yield of the gamma-rays from <26>^Al, information of excited states in <26>^Si, which is located in bypass sequence of the <26>^Al creation cascade, is quite important. In our present study with gamma-ray spectroscopy, we newly observed one level at 5889-keV in the <26>^Si. Spin parity of this level is determined as 0^+ by our angular correlation measurements.
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Report
(4 results)
Research Products
(15 results)
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[Journal Article] Nuclear Clusters in Astrophysics2010
Author(s)
S. Kubono, Dam N. Binh, S. Hayakawa, H. Hashimoto, D. Kahl, Y. Wakabayashi, H. Yamaguchi, T. Teranishi, N. Iwasa, T. Komatsubara, S. Kato, Le H. Khiem
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Journal Title
Nucl. Phys. A
Volume: 834
Issue: 1-4
Pages: 647c-650c
DOI
Related Report
Peer Reviewed
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