Photoexcitation of astrophysically important states in Mg-26. II. Ground-state-transition partial widths

dc.contributor.author

DeBoer, RJ

dc.contributor.author

Wiescher, M

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Görres, J

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Longland, R

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Iliadis, C

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Rusev, G

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Tonchev, AP

dc.date.accessioned

2011-06-21T17:27:47Z

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2011-06-21T17:27:47Z

dc.date.issued

2010

dc.description.abstract

The level structure of Mg-26 near the neutron-separation energy, which is of interest for s-process nucleosynthesis, was studied at the High Intensity Gamma-Ray Source of the Triangle Universities Nuclear Laboratory using the method of nuclear resonance fluorescence. A nearly monoenergetic and linearly polarized gamma-ray beam was used to scan the excitation energy range from 10.5 to 11.7 MeV. For the five states observed, the total widths and partial widths are determined. Precise measurement of these widths is necessary for the prediction of neutron production for the s-process.

dc.description.version

Version of Record

dc.identifier.citation

deBoer,R. J.;Wiescher,M.;Gorres,J.;Longland,R.;Iliadis,C.;Rusev,G.;Tonchev,A. P.. 2010. Photoexcitation of astrophysically important states in Mg-26. II. Ground-state-transition partial widths. Physical Review C 82(2): 25802-25802.

dc.identifier.issn

0556-2813

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https://hdl.handle.net/10161/4267

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en_US

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American Physical Society (APS)

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10.1103/PhysRevC.82.025802

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Physical Review C

dc.subject

s-process nucleosynthesis

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magnesium isotopes

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intermediate-mass

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stellar neutrons

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alpha-capture

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shell nuclei

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scattering

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resonances

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energies

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stars

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physics, nuclear

dc.title

Photoexcitation of astrophysically important states in Mg-26. II. Ground-state-transition partial widths

dc.title.alternative
dc.type

Other article

duke.date.pubdate

2010-8-9

duke.description.issue

2

duke.description.volume

82

pubs.begin-page

25802

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