2016
DOI: 10.1103/physrevc.94.024606
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Elastic Coulomb breakup ofNa34

Abstract: Background: 34 Na is conjectured to play an important role in the production of seed nuclei in the alternate r -process paths involving light neutron rich nuclei very near the β-stability line, and as such, it is important to know its ground state properties and structure to calculate rates of the reactions it might be involved in, in the stellar plasma. Found in the region of 'island of inversion', its ground state might not be in agreement with normal shell model predictions.Purpose: The aim of this paper is… Show more

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Cited by 19 publications
(92 citation statements)
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“…1 ), we write the relative energy spectrum for the breakup of this two-body composite system ( 34 Na) as [29]: The three-body Jacobi coordinate system. The r 's are the corresponding position vectors [34].…”
Section: Formalismmentioning
confidence: 99%
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“…1 ), we write the relative energy spectrum for the breakup of this two-body composite system ( 34 Na) as [29]: The three-body Jacobi coordinate system. The r 's are the corresponding position vectors [34].…”
Section: Formalismmentioning
confidence: 99%
“…To explore the prospective role of 34 Na in the r -process and in the elemental abundance near the drip line, we study its Coulomb dissociation (CD) on a heavy target and use the observables so obtained to calculate the rate of the 33 Na(n,γ) 34 Na capture reaction at stellar temperatures. The method we use for CD studies is the FRDWBA which has been advanced to include the effects of deformation on a nucleus [23].…”
Section: Formalismmentioning
confidence: 99%
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