Yıl 2020,
Cilt: 21 Sayı: 1, 205 - 209, 31.03.2020
Ercan Yıldız
,
İsmail Hakkı Sarpün
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
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.
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.