2016
DOI: 10.1103/physrevc.93.065807
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Coulomb dissociation ofN20,21

Abstract: Neutron-rich light nuclei and their reactions play an important role for the creation of chemical elements. Here, data from a Coulomb dissociation experiment on 20,21 N are reported. Relativistic 20,21 N ions impinged on a lead target and the Coulomb dissociation cross section was determined in a kinematically complete experiment. Using the detailed balance theorem, the 19 N(n, γ) 20 N and 20 N(n, γ) 21 N excitation functions and thermonuclear reaction rates have been determined. The 19 N(n, γ) 20 N rate is up… Show more

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Cited by 9 publications
(28 citation statements)
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References 29 publications
(45 reference statements)
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“…A detailed description of the setup can be found in Refs. [25,[29][30][31][32]. The experiment was performed with CH 2 (458 and 922 mg=cm 2 ) and C (558 and 935 mg=cm 2 ) targets as well as with an empty target frame.…”
mentioning
confidence: 99%
“…A detailed description of the setup can be found in Refs. [25,[29][30][31][32]. The experiment was performed with CH 2 (458 and 922 mg=cm 2 ) and C (558 and 935 mg=cm 2 ) targets as well as with an empty target frame.…”
mentioning
confidence: 99%
“…The experiment was performed at GSI, Darmstadt in Germany, where the isotopes 29,30 Na and 33 Mg and 35 Al were produced by fragmentation of a 40 Ar beam with an energy of 540A MeV using the FRS-ALADIN-LAND setup. The fragments were separated by the fragment separator (FRS) [37] and the secondary beams were transported to the experimental site for complete kinematic measurements using 208 Pb, 12 C, and empty secondary targets.…”
Section: Methodsmentioning
confidence: 99%
“…The data for the neutron capture reaction rate on light neutronrich nuclei are also important for understanding r-process concerning the neutrino-driven wind model and the impact of light neutron-rich nuclei as seed nuclei. Until recently, (n, γ ) capture cross sections measured using this method have been reported only for lower sd-shell neutron-rich nuclei [32,33]. In this work, we shall report the measurements of the neutron capture cross sections for the upper sd and p f shell neutron-rich nuclei, 28 Na(n, γ ) 29 Na, 29 Na(n, γ ) 30 Na, 32 Mg(n, γ ) 33 Mg, and 34 Al(n, γ ) 35 Al that were considered as seed nuclei in the neutrino-driven wind model.…”
Section: Introductionmentioning
confidence: 99%
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