Systematics of alpha-particle strengths of low-lying levels in light sd- shell nuclei
Conference
·
OSTI ID:4093077
- eds.
A survey of alpha-particle spectroscopic factors of low-lying levels in sd-shell nuclei with A less than or equal to 29 as measured by the ($sup 6$Li,d) reaction at energies up to 36 MeV is presented. A comparison is made with theoretical predictions not only for inter- and intra-band transitions in a given nucleus, but also with the absolute ground state to ground state transitions. Substantial agreement is obtained, but some unexplained discrepancies remain. (auth)
- Research Organization:
- Univ. of Rochester, NY; Maryland Univ., College Park (USA). Dept. of Physics and Astronomy
- NSA Number:
- NSA-33-018910
- OSTI ID:
- 4093077
- Report Number(s):
- ORO--4856-26; CONF-750447--
- Country of Publication:
- United States
- Language:
- English
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·
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Related Subjects
*LIGHT NUCLEI-- LITHIUM 6 REACTIONS
*LITHIUM 6 REACTIONS-- STRIPPING
*MAGNESIUM 24-- ENERGY-LEVEL TRANSITIONS
*NEON 20-- ENERGY-LEVEL TRANSITIONS
*NEON 22-- ENERGY-LEVEL TRANSITIONS
*SILICON 28-- ENERGY-LEVEL TRANSITIONS
642203*
ALPHA PARTICLES
ALPHA-TRANSFER REACTIONS
ANGULAR DISTRIBUTION
MAGNESIUM 25
MEV RANGE 10-100
N68431* --Physics (Nuclear
Experimental)--Nuclear Properties & Reactions
20 <= A <= 38--Energy Levels & Transitions
N68432 --Physics (Nuclear
Theoretical)--Nuclear Properties & Reactions
20 <= A <= 38--Energy Levels & Transitions
NEON 21
OXYGEN 16
OXYGEN 18
SILICON 29
SPECTROSCOPIC FACTORS
*LITHIUM 6 REACTIONS-- STRIPPING
*MAGNESIUM 24-- ENERGY-LEVEL TRANSITIONS
*NEON 20-- ENERGY-LEVEL TRANSITIONS
*NEON 22-- ENERGY-LEVEL TRANSITIONS
*SILICON 28-- ENERGY-LEVEL TRANSITIONS
642203*
ALPHA PARTICLES
ALPHA-TRANSFER REACTIONS
ANGULAR DISTRIBUTION
MAGNESIUM 25
MEV RANGE 10-100
N68431* --Physics (Nuclear
Experimental)--Nuclear Properties & Reactions
20 <= A <= 38--Energy Levels & Transitions
N68432 --Physics (Nuclear
Theoretical)--Nuclear Properties & Reactions
20 <= A <= 38--Energy Levels & Transitions
NEON 21
OXYGEN 16
OXYGEN 18
SILICON 29
SPECTROSCOPIC FACTORS