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008 | 190131s2018 ua d f m 000 0 eng d | ||
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_aEG-GiCUC _beng _cEG-GiCUC |
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041 | 0 | _aeng | |
049 | _aDeposite | ||
097 | _aPh.D | ||
099 | _aCai01.12.20.Ph.D.2018.La.O | ||
100 | 0 | _aLaila Hassan Mohammad Amer | |
245 | 1 | 0 |
_aOn the cluster radioactivity of heavy nuclei / _cLaila Hassan Mohammad Amer ; Supervised Walaa Mohamed Seif , Mahmoud Yahia Ismail , Amal I. Refaei |
246 | 1 | 5 | _aالنشاط الإشعاعى العنقودي للأنوية الثقيلة |
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_aCairo : _bLaila Hassan Mohammad Amer , _c2018 |
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_a112 P. : _bcharts ; _c25cm |
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502 | _aThesis (Ph.D.) - Cairo University - Faculty of Science - Department of Physics | ||
520 | _aThe most probable cluster decays that might be observed from ²¹⁷-²³⁸U isotopes have been investigated. The more-probable binary fragmentations corresponding to the local minima in the driving potentials with respect to the mass number Ac and atomic number Zc, individually, are singled out. The calculations are preformed based on the Skyrme-SLy4 nucleon-nucleon interaction and the folded Coulomb interaction. In the frame work of the preformed cluster model, we calculated the cluster decays half-lives and their branching ratios, with respect to the total half-life of the investigated isotope. The quantum knocking frequency and penetration probability based on the Wentzel-Kramers-Brillouin approximation are used to find the decay width. We considered the more-probable decays that commonly manifest themselves via cold valleys in the driving potentials with respect to both Ac and Zc. Among the indicated favored decays involving emitted light clusters heavier than Ü-particle, 28 decay modes exhibit calculated half-lives less than 10²² years with branching ratio larger than 10-¹⁴% | ||
530 | _aIssued also as CD | ||
653 | 4 | _aCluster radioactivity | |
653 | 4 | _aHalf-life | |
653 | 4 | _aPreformation probability | |
700 | 0 |
_aAmal I. Refaei , _eSupervisor |
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700 | 0 |
_aMahmoud Yahia Ismail , _eSupervisor |
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700 | 0 |
_aWalaa Mohamed Seif , _eSupervisor |
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_aAsmaa _eCataloger |
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_aNazla _eRevisor |
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_2ddc _cTH |
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_c69873 _d69873 |