Charge state distribution of 16O from the 4He(12C,16O)γ reaction of astrophysical interest studied both experimentally and theoretically-Reference-Cited by-同舟云学术

Charge state distribution of 16O from the 4He(12C,16O)γ reaction of astrophysical interest studied both experimentally and theoretically

Published:2014-06 Issue: Volume:328 Page:14-19
ISSN:0168-583X
Container-title:Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
language:en
Short-container-title:Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms

Author:

Liu Shengjin,Sakurai Makoto,Sagara Kenshi,Teranishi Takashi,Fujita Kunihiro,Yamaguchi Hiroyuki,Matsuda Sayaka,Mitsuzumi Tatsuki,Iwazaki Makoto,Rosary Mariya T.,Kato Daiji,Tolstikhina I.Yu.

Publisher

Elsevier BV

Subject

Instrumentation,Nuclear and High Energy Physics

Reference35 articles.

1. Nucleosynthesis in massive stars and the 12C(α, γ)16O reaction rate

2. Direct measurement of [sup 4]He([sup 12]C, [sup 16]O)γ reaction near stellar energy

3. H. Oba, Kyushu University, 2007 Doctor thesis: Direct measurement of nuclear astrophysical reaction 4He(12C,16O)γ cross section near stellar temperature.

4. Systematics of equilibrium charge distributions of ions passing through a carbon foil over the rangesZ=4–92 andE=0.02–6 MeV/u

5. Equilibrium-charge-state distributions of energetic ions (Z > 2) in gaseous and solid media

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