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Yıl 2020, Cilt: 21 Sayı: 1, 205 - 209, 31.03.2020

Ercan Yıldız İsmail Hakkı Sarpün

https://doi.org/10.18038/estubtda.632019

Öz

Kaynakça

  • Referans1 Paradellis T, Kossionides S, Doukellis G, Aslanoglou A, Assimakopouls P, Pakou A, Rolfs C. and Langanke K. Astrophysical S(E) factor of 8Li(α,n0)11B and inhomogeneous Big Bang nucleosynthesis, Zeitschrift für Physik A Atomic Nuclei, 1990; 337: 211-220.
  • Referans2 Terasawa M, Sumiyoshi K, Kajino T, G. J. Mathews G. J. and Tanihata I. New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light, Neutron-rich Nuclei, The Astrophysical Journal, 2001; 562: 470-479.
  • Referans3 Miyatake H, Ishiyama H, Tanakaa M. H, Watanabea Y. X, N. Yoshikawa N, Jeonga S. C, Matsuyama Y, Fuchia Y, Nomuraa T, Hashimotoh T. Exclusive measurement of the astrophysical 8Li(a,n) reaction cross section, Nuclear Physics A, 2004; 738: 401-405.
  • Referans4 Yıldız E, 0-8 MeV Enerji Bölgesinde 13C(α,n)16O Reaksiyonu için Astrofiziksel S-Faktörlerin Hesaplanması, Süleyman Demirel Üniversitesi Fen Edebiyat Fakültesi Fen Dergisi, 2018; 13: 25-28.
  • Referans5 Guimarâes V. and Bertulani C. A. Light radioactive nuclei capture reactions with phenomenological potential models, AIP Conference Proceedings, 2010; 30: 1245.
  • Referans6 Alinka L. S. and Descouvermont P. Nuclear astrophysics: Nucleosynthesis in the Universe International, Journal of Astrobiology, 2012, 11: 243-250.
  • Referans7 Koning A. J, Hilaire S. and Goriely S. TALYS–1.8 A Nuclear Reaction Program, 2018.
  • Referans8 EXFOR/CSISRS, Brookhaven National Laboratory, National Nuclear Data Center, Database Version of September 2017.
  • Referans9 Gu X, Boyd R. N, Farrel M. M, Kalen J. D, Mitchell C. A, Kolata J. J, Belbot M, Lamkin K, Ashktorab K, Bechetti F. D. The 8Li(α,n)11B reaction and primordial nucleosynthesis, Physics Letter B, 1995; 343: 31-35.
  • Referans10 Ishiyama H, Hashimoto T, Ishikawa T, Watanabe Y. X, Das S. K, Miyatakea H, Mizoi Y, Fukuda T, Tanaka M. H, Fuchi Y. A new measurement of the astrophysical 8Li(α,n) reaction, Physics Letter B, 2006; 640: 82-85.
  • Referans11 Kaplan A, Investigation of Neutron-Production Cross Sections of the Structural Fusion Material 181Ta for (α,xn) Reactions up to 150 MeV Energy, Journal of Fusion Energy, 2013; 32: 382-388.
  • Referans12 Sarpün İ. H, Aydın A, Kaplan A, Koca H, Tel E, Comparison of Fission Barrier and Level Density Models in (a,f) Reactions of Some Heavy Nuclei, Ann. Nucl. Energy 2014; 70: 175-179.
  • Referans13 Aydın A, Tel E, Pekdoğan H, Kaplan A, Nuclear Model Calculations on the Production of 125,123Xe and 133,131,129,128Ba Radioisotopes, Phys. Atom Nucl. 2012; 75: (3), 310-314.

CALCULATION OF CROSS SECTIONS AND ASTROPHYSICAL S-FACTORS AT 0-5 MeV ENERGY RANGE FOR 8Li (α, n)11B REACTION

Yıl 2020, Cilt: 21 Sayı: 1, 205 - 209, 31.03.2020

Ercan Yıldız İsmail Hakkı Sarpün

https://doi.org/10.18038/estubtda.632019

Öz


Explaining the origin and evolution of elements is one of the most important problems in astrophysics. The r-process in the current nucleosynthesis scenario; roughly responsible for the production of half of the nuclei heavier than iron. 8Li(α,n)11B reaction plays an important role in the r-process of this scenario because of being a cosmic radiation induced  reaction. In particular, it is important to know the change with energy in the low energy zone for testing the accuracy of the model calculations. In this study, the astrophysical S-factors of the 8Li(α,n)11B reaction and the probability of reaction at low energies were calculated in the 0-5 MeV energy range. TALYS 1.8 code was used for the theoretical calculations. The obtained theoretical values were compared with experimental data obtained from the EXFOR database.


Anahtar Kelimeler

8Li Cross-Section S-Factor TALYS 1.8

Kaynakça

  • Referans1 Paradellis T, Kossionides S, Doukellis G, Aslanoglou A, Assimakopouls P, Pakou A, Rolfs C. and Langanke K. Astrophysical S(E) factor of 8Li(α,n0)11B and inhomogeneous Big Bang nucleosynthesis, Zeitschrift für Physik A Atomic Nuclei, 1990; 337: 211-220.
  • Referans2 Terasawa M, Sumiyoshi K, Kajino T, G. J. Mathews G. J. and Tanihata I. New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light, Neutron-rich Nuclei, The Astrophysical Journal, 2001; 562: 470-479.
  • Referans3 Miyatake H, Ishiyama H, Tanakaa M. H, Watanabea Y. X, N. Yoshikawa N, Jeonga S. C, Matsuyama Y, Fuchia Y, Nomuraa T, Hashimotoh T. Exclusive measurement of the astrophysical 8Li(a,n) reaction cross section, Nuclear Physics A, 2004; 738: 401-405.
  • Referans4 Yıldız E, 0-8 MeV Enerji Bölgesinde 13C(α,n)16O Reaksiyonu için Astrofiziksel S-Faktörlerin Hesaplanması, Süleyman Demirel Üniversitesi Fen Edebiyat Fakültesi Fen Dergisi, 2018; 13: 25-28.
  • Referans5 Guimarâes V. and Bertulani C. A. Light radioactive nuclei capture reactions with phenomenological potential models, AIP Conference Proceedings, 2010; 30: 1245.
  • Referans6 Alinka L. S. and Descouvermont P. Nuclear astrophysics: Nucleosynthesis in the Universe International, Journal of Astrobiology, 2012, 11: 243-250.
  • Referans7 Koning A. J, Hilaire S. and Goriely S. TALYS–1.8 A Nuclear Reaction Program, 2018.
  • Referans8 EXFOR/CSISRS, Brookhaven National Laboratory, National Nuclear Data Center, Database Version of September 2017.
  • Referans9 Gu X, Boyd R. N, Farrel M. M, Kalen J. D, Mitchell C. A, Kolata J. J, Belbot M, Lamkin K, Ashktorab K, Bechetti F. D. The 8Li(α,n)11B reaction and primordial nucleosynthesis, Physics Letter B, 1995; 343: 31-35.
  • Referans10 Ishiyama H, Hashimoto T, Ishikawa T, Watanabe Y. X, Das S. K, Miyatakea H, Mizoi Y, Fukuda T, Tanaka M. H, Fuchi Y. A new measurement of the astrophysical 8Li(α,n) reaction, Physics Letter B, 2006; 640: 82-85.
  • Referans11 Kaplan A, Investigation of Neutron-Production Cross Sections of the Structural Fusion Material 181Ta for (α,xn) Reactions up to 150 MeV Energy, Journal of Fusion Energy, 2013; 32: 382-388.
  • Referans12 Sarpün İ. H, Aydın A, Kaplan A, Koca H, Tel E, Comparison of Fission Barrier and Level Density Models in (a,f) Reactions of Some Heavy Nuclei, Ann. Nucl. Energy 2014; 70: 175-179.
  • Referans13 Aydın A, Tel E, Pekdoğan H, Kaplan A, Nuclear Model Calculations on the Production of 125,123Xe and 133,131,129,128Ba Radioisotopes, Phys. Atom Nucl. 2012; 75: (3), 310-314.
Toplam 13 adet kaynakça vardır.

Ayrıntılar

Birincil Dil İngilizce
Konular Mühendislik
Bölüm Makaleler
Yazarlar

Ercan Yıldız 0000-0001-8709-4764

İsmail Hakkı Sarpün 0000-0002-9788-699X

Yayımlanma Tarihi 31 Mart 2020
Yayımlandığı Sayı Yıl 2020 Cilt: 21 Sayı: 1

Kaynak Göster

AMA Yıldız E, Sarpün İH. CALCULATION OF CROSS SECTIONS AND ASTROPHYSICAL S-FACTORS AT 0-5 MeV ENERGY RANGE FOR 8Li (α, n)11B REACTION. Eskişehir Technical University Journal of Science and Technology A - Applied Sciences and Engineering. Mart 2020;21(1):205-209. doi:10.18038/estubtda.632019