6533b85cfe1ef96bd12bc9f1
RESEARCH PRODUCT
Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process
R. G. T. ZegersR. G. T. ZegersAlexander HegerAlexander HegerAlfredo EstradeD. WeisshaarT. GlasmacherR. KesslerDaniel GalavizDaniel GalavizDaniel GalavizJ. PereiraJ. PereiraM. E. HowardFernando MontesFernando MontesAlexandra GadeZs. FülöpHendrik SchatzHendrik SchatzAtsushi TamiiY. ShimbaraA. ChenT. ElliotJ. M. CookA. L. ColeAna BecerrilMilan MatosMichael WiescherA. M. AmthorA. M. AmthorE. SmithMark WallaceD. BazinB. A. BrownGiuseppe LorussoKarl SmithAndreas StolzW. MüllerF. SchertzB. M. SherrillB. M. Sherrillsubject
Nuclear reactionPhysicsHistoryProton010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Nuclear TheoryCyclotronrp-process[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]7. Clean energy01 natural sciencesComputer Science ApplicationsEducationlaw.inventionNuclear physicsIsotopes of potassiumlawNucleosynthesis0103 physical sciencesr-processAtomic physics010306 general physicsNuclear ExperimentRadioactive decaydescription
Experience NSCL; International audience; We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of < 10 keV. This will allow a reduction in the determination of the astrophysical (p, ) reaction rate under rp-process conditions.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2009-06-08 |