Yayınlanmış 1 Ocak 2012 | Sürüm v1
Dergi makalesi Açık

Investigation of alpha-induced reactions on I-127 for the astrophysical gamma process

  • 1. Inst Nucl Res ATOMKI, H-4001 Debrecen, Hungary
  • 2. Univ Basel, Dept Phys, CH-4056 Basel, Switzerland

Açıklama

Background: The. process in core-collapse supernova explosions is thought to explain the origin of proton-rich isotopes between Se and Hg, the so-called p nuclei. The majority of the reaction rates for gamma process reaction network studies has to be predicted in Hauser-Feshbach statistical model calculations. Recent investigations have shown problems in the prediction of alpha widths at astrophysical energies. This impacts the reliability of abundance predictions in the upper mass range of the p nuclei.

Dosyalar

bib-885579d5-d8ab-4e19-a08c-1f5cd4c97f74.txt

Dosyalar (234 Bytes)

Ad Boyut Hepisini indir
md5:ef9960c14bccdb4540c7c9d01d611b5e
234 Bytes Ön İzleme İndir