Study of Some Levels ofC12Using theB10(He3, p)C12*Reactions
- 15 May 1959
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 114 (4) , 1040-1053
- https://doi.org/10.1103/PhysRev.114.1040
Abstract
Studies of the reaction using 2-Mev ions showed proton groups corresponding to levels in at 0, 4.43, 7.65, 9.60, 10.76, 11.82, 12.78, 13.37, 14.03, 15.10, 16.10, and 16.64 Mev±0.10 Mev. The ratio was measured to be 0.75(±0.20) for the 15.1-Mev state and 0.02(±0.01) for the 12.78-Mev state. No other alpha unstable level had a measurable ; for the 7.65-Mev state a limit 0.01 is set on this ratio. The gamma-ray de-excitation of the 15.1-Mev state is both to the ground state (97%) and to the 4.43-Mev state (3.1±0.6%). Only a ground state transition was observed from the 12.78-Mev level. These measurements support assignments, , , of 1, +, 1 to the 15.1 level and 1, +, 0 to the 12.78-Mev state. The known properties of are in fair agreement with the intermediate coupling shell-model calculations of Kurath. The reactions (15.1 Mev) and to the ground and first excited state of were observed.
Keywords
This publication has 31 references indexed in Scilit:
- ,, and the Red GiantsPhysical Review B, 1957
- Photon Self-Absorption and Scattering by the 15.1-Mev Level inPhysical Review B, 1957
- Intermediate Coupling in the-ShellPhysical Review B, 1956
- () Reactions on Boron and CarbonPhysical Review B, 1955
- Energy Levels of Light Nuclei. VReviews of Modern Physics, 1955
- Emission of High-Energy Gamma Line fromPhysical Review B, 1954
- Search for 15-Mev Gamma Radiation fromN14+dandBe9+αPhysical Review B, 1954
- On Nuclear Reactions Occuring in Very Hot STARS.I. the Synthesis of Elements from Carbon to Nickel.The Astrophysical Journal Supplement Series, 1954
- Energy Levels ofandfrom Photographic Plate Observation of Neutron SpectraPhysical Review B, 1952
- Nuclear Reactions in Stars Without Hydrogen.The Astrophysical Journal, 1952