Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths

Details Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phrvc..82b5802d&link_type=abstract

Physical Review C, vol. 82, Issue 2, id. 025802

Physics

1

S-Process, Angular Distribution And Correlation Measurements, Multipole Matrix Elements, 20<=A<=38

Scientific paper

The level structure of Mg26 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 γ-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.

Affiliated with

Also associated with

No associations

Rating

Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photoexcitation of astrophysically important states in Mg26. II. Ground-state-transition partial widths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1125254