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dc.contributor.advisorHusin, Abd. Djamil
dc.contributor.authorAkbar, Agie Maliki
dc.date.accessioned2013-10-30T03:23:41Z
dc.date.available2013-10-30T03:23:41Z
dc.date.issued2013
dc.identifier.urihttp://repository.ipb.ac.id/handle/123456789/65762
dc.description.abstractLiquid droplets of nucleic models can be derived equations to estimate the binding energy, binding energy per nucleon, the most stable isotope, and the condition of the occurrence of spontaneous fission. The equations are then converted into a numerical equation form which is then inserted into the MATLAB programming language. Based on the results of the calculations have been carried out in this study, super-heavy nuclei will undergo spontaneous fission in the Z = 135. At Z = 135 the energy needed to create the nucleus undergoing fission or activation energy is very small at around 0:48 MeV. Above Z = 135 the activation energy is negative, it means to form a nucleus with Z> 135 needed some energy. Then at Z = 135 the ratio Z2 / A is 48.86, almost reaching requirement ratio Z2 / A where the nucleic will undergo spontaneous fission is 49. Binding energy per nucleon for super-heavy nuclei up to Z = 200 is about 7 - 5.5 MeV, together with a range of light nuclei are stable. So there may be a super-heavy nuclei are stable at Z <135 and above Z> 135 there will be no stable nucleicen
dc.subjectBogor Agricultural University (IPB)en
dc.subjectpairingen
dc.subjectbinding energy per nucleonen
dc.subjectactivation energyen
dc.subjectspontaneous fissionen
dc.subjectsuper heavy nucleien
dc.titleKajian Stabilitas Inti Super Berat dengan Nomor Atom 110 Sampai dengan 200 Menggunakan Model Inti Tetesan Cairanen


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