Optical and Double Folding Analysis for 6Li+16O Elastic Scattering
Available experimental angular distributions for 6Li elastically scattered from 16O nucleus in the energy range 13.0–50.0 MeV are investigated and reanalyzed using optical model of the conventional phenomenological potential and also using double folding optical model of different interaction models: DDM3Y1, CDM3Y1, CDM3Y2, and CDM3Y3. All the involved models of interaction are of M3Y Paris except DDM3Y1 which is of M3Y Reid and the main difference between them lies in the different values for the parameters of the incorporated density distribution function F(ρ). We have extracted the renormalization factor NRfor 6Li+16O nuclear system in the energy range 13.0–50.0 MeV using the aforementioned interaction models.
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[16] K. Bethge, C. M. Fou, and R. W. Zurmuhle, Nucl. Phys. A123, 521 (1969)
[17] M. F. Vineyard, J. Cook, K. W. Kemper, and M. N. Stephens, Phys. Rev. C30, 916 (1984)
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[19] N. Anantaraman, H. W. Fulbright, P. M. Stwertka, Phys. Rev. C22, 501 (1980)
[20] P. Schumacher, N. Ueta, H. H. Duhm, K.-I. Kubo, and W. J. Klages, Nucl. Phys. A212, 573 (1973)
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[22] D. E. Trcka, A. D. Frawley, K. W. Kemper, D. Robson, J. D. Fox, and E. G. Myers, Phys. Rev. C41, 2134 (1990)
[23] R. M. DeVries, D. A. Goldberg, J. W. Watson, M. S. Zisman, J. G. Gramer, Phys. Rev. Lett. 39, 450 (1977)
[24] Mandira Sinha, Subinit Roy, P. Basu, H. Majumdar, S. Santra, V.V. Park, EPJ Web of Conf. 17, 03004 (2011)
[25] M. Hugi, J. Lang, R. Miller, E. Ungricht, K. Bodek, L. Jarczyk. B. Kam, Nucl. Phys. A368, 173 (1981)
[26] A. Nadasen, M. McMaster, M. Fingal, J. Tavormina, P. Schwandt, Phys. Rev. C39, 536 (1989)
[27] A. Pakou, N. Alamanos, A. Lagoyannis, A. Gillibert, E. C. Pollacco, Phys. Lett. B556, 21 (2003)
[28] J. E. Poling, E. Norbeck, and R. R. Carlson, Phys. Rev. C5, 1819 (1972)
[29] P. K. Bindal, K. Nagatani, M. J. Schneider, and P. D. Bond, Phys. Rev. C9, 2154 (1974)
[30] J. E. Poling, E. Norbeck, and R. R. Carlson, Phys. Rev. C13, 648 (1976)
[31] Sh. Hamada, B. Alshahrani, Abd Elrahman Elgamala, N. Darwish, I. Bondouk and Awad A. Ibraheem, Revista Mexicana de Fisica 66(3) (2020) 322
[32] Sh. Hamada and AwadA.Ibraheem, Int. J. Mod. Phys. E28 (2019) 1950108
[33] I. I. Gontchar and M. V. Chushnyakova, Comput. Phys. Commun. 181, 168 (2010)
[34] D. T. Khoa, G. R. Satchler and W. von Oertzen, Phys. Rev.C 56954 (1997)
[35] D. T. Khoa and W. von Oertzen, Phys. Lett.B 304 8 (1993)
[36] S. Qing-biao, F. Da-chun, Z. Yi-Zhong, Phys. Rev. C43, 2773 (1991)
[37] K.H. Bray et al., Nucl. Phys. A 189(1972) 35.
[38] I. J. Thompson, Comput. Phys. Rep.7, 167 (1988)
[1] M. F. Vineyard, J. Cook, K. W. Kemper, and M. N. Stephens, Phys. Rev. C30 (1984) 916
[2] D. L. Gay, E. E. Bartosz, P. D. Cathers, D. D. Caussyn, T. L. Drummer, K. W. Kemper, P. L. Kerr, and D. Robson, Phys. Rev. C54 (1996) 3273
[3] D. E. Trcka, A. D. Frawley, K. W. Kemper, D. Robson, J. D. Fox, and E. G. Myers, Phys. Rev. C41 (1990) 2134
[4] C. L. Woods, B. A. Brown, and N. A. Jelley, J. Phys. G: Nucl. Phys 8 (1982) 1699
[5] A. S. Dem'yanova, J. M. Bang, F. A. Gareev, S. A. Goncharov, S. N. Ershov, A. A. Ogloblin and P. P. Korovin, Nucl. Phys. A501(1989) 336.
[6] L. T. Chua, F. D. Becchetti, J. Janecke and F. L. Milder, Nucl. Phys. A273 (1976) 243
[7] F. Carstoiu, L. Trache, R.E. Tribble, C.A. Gagliardi, Phys. Rev. C70 (2004) 054610
[8] H.G. Bingham, M.L. Halbert, D.C. Hensley, E. Newman, K.W. Kemper, L.A. Charlton, Phys. Rev. C11 (1975) 1913
[9] P. Schwandt, W. W. Jacobs, M. D. Kaitchuck, P. P. Singh, W. O. Ploughe, F. D. Becchetti, J. Janecke, Phys. Rev. C24 (1981) 1522
[10] K. Katori, T. Shimoda, T. Fukuda, S. Shimoura, A. Sakaguchi, M. Tanaka, T. Yamagata, N. Takahash, H. Ogata, M. Kamimura and Y. Sakuragi, Nucl. Phys. A480 (1988) 232
[11] J. Cook, H. J. Gils, H. Rebel, Z. Majka, H. Klewe-Nebenius, Nucl. Phys. A388 (1982) 173.
[12] A. Nadasen, M. McMaster, G. Gunderson, A. Judd, S. Villanueva, P. Schwandt J. van der Plicht, R. E. Warner, F. D. Becchetti and J. W. Janecke, Phys. Rev. C37 (1988) 132
[13] A. Nadasen, T. Stevens, J. Farhat, J. Brusoe, P. Schwandt, J.S. Winfield, G. Yoo N. Anantaraman, F. D. Becchetti, J. Brown, B. Hotz, J. W. Janecke, D.Roberts and R. E. Warner, Phys. Rev. C47 (1993) 647
[14] K. Schwarz, C. Samanta, M. Fujiwara, H. Rebel, R. De Leo, N. Matsuoka, H. Utsunomiya, H. Akimune, I. Daito, H. Fujimura, F. Ihara, K. Ishibashi, Y. Maeda, T. Yamanaka, H. Yoshida, A. Okihana, T. Yoshimura, P. K. J. van Aarle, W. A. T. Uijen, M. Ito, Y. Sakuragi, EPJA 7 (2000) 367
[15] J. E. Poling, E. Norbeck, and R. R. Carlson, Phys. Rev. C13, 648 (1976)
[16] K. Bethge, C. M. Fou, and R. W. Zurmuhle, Nucl. Phys. A123, 521 (1969)
[17] M. F. Vineyard, J. Cook, K. W. Kemper, and M. N. Stephens, Phys. Rev. C30, 916 (1984)
[18] V. V. Davydov, B. G. Novashkii, A. A. Ogloblin, S. B. Sakuta, D. N. Stepanov, V. I. Chuev, J, IZV 35 (11), 2399 (1971)
[19] N. Anantaraman, H. W. Fulbright, P. M. Stwertka, Phys. Rev. C22, 501 (1980)
[20] P. Schumacher, N. Ueta, H. H. Duhm, K.-I. Kubo, and W. J. Klages, Nucl. Phys. A212, 573 (1973)
[21] J. Cook, L. C. Dennis, K. W. Kemper, T. R. Ophel, A. F. Zeller, C. F. Maguire, and Z. Kui, Nucl. Phys. A415, 114 (1984)
[22] D. E. Trcka, A. D. Frawley, K. W. Kemper, D. Robson, J. D. Fox, and E. G. Myers, Phys. Rev. C41, 2134 (1990)
[23] R. M. DeVries, D. A. Goldberg, J. W. Watson, M. S. Zisman, J. G. Gramer, Phys. Rev. Lett. 39, 450 (1977)
[24] Mandira Sinha, Subinit Roy, P. Basu, H. Majumdar, S. Santra, V.V. Park, EPJ Web of Conf. 17, 03004 (2011)
[25] M. Hugi, J. Lang, R. Miller, E. Ungricht, K. Bodek, L. Jarczyk. B. Kam, Nucl. Phys. A368, 173 (1981)
[26] A. Nadasen, M. McMaster, M. Fingal, J. Tavormina, P. Schwandt, Phys. Rev. C39, 536 (1989)
[27] A. Pakou, N. Alamanos, A. Lagoyannis, A. Gillibert, E. C. Pollacco, Phys. Lett. B556, 21 (2003)
[28] J. E. Poling, E. Norbeck, and R. R. Carlson, Phys. Rev. C5, 1819 (1972)
[29] P. K. Bindal, K. Nagatani, M. J. Schneider, and P. D. Bond, Phys. Rev. C9, 2154 (1974)
[30] J. E. Poling, E. Norbeck, and R. R. Carlson, Phys. Rev. C13, 648 (1976)
[31] Sh. Hamada, B. Alshahrani, Abd Elrahman Elgamala, N. Darwish, I. Bondouk and Awad A. Ibraheem, Revista Mexicana de Fisica 66(3) (2020) 322
[32] Sh. Hamada and AwadA.Ibraheem, Int. J. Mod. Phys. E28 (2019) 1950108
[33] I. I. Gontchar and M. V. Chushnyakova, Comput. Phys. Commun. 181, 168 (2010)
[34] D. T. Khoa, G. R. Satchler and W. von Oertzen, Phys. Rev.C 56954 (1997)
[35] D. T. Khoa and W. von Oertzen, Phys. Lett.B 304 8 (1993)
[36] S. Qing-biao, F. Da-chun, Z. Yi-Zhong, Phys. Rev. C43, 2773 (1991)
[37] K.H. Bray et al., Nucl. Phys. A 189(1972) 35.
[38] I. J. Thompson, Comput. Phys. Rep.7, 167 (1988)
@article{"International Journal of Chemical, Materials and Biomolecular Sciences:80112", author = "Abd Elrahman Elgamala and N. Darwish and I. Bondouk and Sh. Hamada", title = "Optical and Double Folding Analysis for 6Li+16O Elastic Scattering", abstract = "Available experimental angular distributions for 6Li elastically scattered from 16O nucleus in the energy range 13.0–50.0 MeV are investigated and reanalyzed using optical model of the conventional phenomenological potential and also using double folding optical model of different interaction models: DDM3Y1, CDM3Y1, CDM3Y2, and CDM3Y3. All the involved models of interaction are of M3Y Paris except DDM3Y1 which is of M3Y Reid and the main difference between them lies in the different values for the parameters of the incorporated density distribution function F(ρ). We have extracted the renormalization factor NR for 6Li+16O nuclear system in the energy range 13.0–50.0 MeV using the aforementioned interaction models.
", keywords = "Elastic scattering, optical model, folding potential, density distribution.", volume = "14", number = "12", pages = "269-6", }
