0-8 MeV Enerji Bölgesinde 13C(α,n)16O Reaksiyonu için Tesir Kesitleri ve Astrofiziksel S-Faktörlerin Hesaplanması

Reaksiyon tesir kesiti bir nükleer reaksiyonun gerçekleşme olasılığını ifade eder. Ayrıca reaksiyon tesir kesiti verileri çok geniş bir alanda kullanılmaktadır. Kimyasal elementlerin kökeni, modern fiziğin doğmasından bu yana nicel çalışmalara konu olmuştur ve on yıllar boyunca, deneysel ve teorik çalışan nükleer fizikçilerin yanı sıra kozmologların, astrofizikçilerin ve astronomların ilgisini çekmiştir. 13C(α,n)16O reaksiyonu, s-sürecinin ana bileşeni olarak 90

Calculation of Cross Sections and Astrophysical S-Factors for 13C (α,n) 16O Reaction in 0-8 MeV Energy Zone

Reaction cross section refers to the probability of a nuclear reaction’s occurrence. In addition, data is also used in a wide range of reaction area. The origin of the chemical elements has been the subject of quantitative work since the birth of modern physics, and for decades has attracted the attention of cosmologists, astrophysicists and astronomers as well as experimental and theoretical nuclear physicists. The 13C (α,n)16O reaction is the origin of the neutron for the major component of the s-process, in charge of for the production process of plenty of the nuclei in the mass range 90

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