Peculiarities of Nuclear Fusion in Synthesis of Superheavy Elements

A. Nasirov, G. Giardina, A. Muminov, G. Mandaglio, R. Utamuratov
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Abstract

The small probabilities of synthesis of new superheavy elements at GSI (Darmstadt, Germany), Joint Institute for Nuclear Research (Dubna, Russia), and RIKEN (Wako, Japan) during the last decade stimulate the experimental and theoretical studies of the nuclear reaction mechanism. 1– 4 In preparation of these experiments, the main aim is to reach maximum cross sections of the yield of evaporation residues (ER) as a result of the de-excitation of the heated compound nucleus which is formed in complete fusion of the projectile and target nuclei. Because the ER excitation function in the synthesis of superheavy elements has very narrow width for “cold fusion” reactions (5–10 MeV) with 208 Pb and 209 Bi targets 5 and the width of the “hot fusion” reactions with 48 Ca projectile on actinide tar
超重元素合成中核聚变的特点
GSI(德国达姆施塔特)、联合核研究所(俄罗斯杜布纳)和RIKEN(日本Wako)在过去十年中合成新的超重元素的小概率刺激了核反应机理的实验和理论研究。在准备这些实验时,主要目的是达到蒸发残留物产率的最大横截面,这是由于在弹丸和靶核完全融合中形成的加热复合核的去激发。因为在超重元素合成中,与208 Pb和209 Bi靶5的冷聚变反应(5 - 10 MeV)和与48 Ca靶在锕系元素上的热聚变反应的激发函数宽度非常窄
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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