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Available Face-Changing Effect
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作者 Xiaobai Ai 《Journal of Modern Physics》 2018年第12期2193-2205,共13页
Based on mathematical foresight and beyond the mainstream inertial thinking pattern, the author believes that if neutrinos were really tachyons, the mystery of neutrinos might be solved. Fortunately, the space-like th... Based on mathematical foresight and beyond the mainstream inertial thinking pattern, the author believes that if neutrinos were really tachyons, the mystery of neutrinos might be solved. Fortunately, the space-like theory of special relativity reveals that there would exist an observable effect i.e. a “face-changing effect”, not oscillation, which was just related to the superluminal motion. As long as the motion velocity of an electron anti-neutrino was greater than c2/v, where v was the instantaneous thermal motion velocity of its mother neutron at the time of &beta;-decay, a corresponding electron neutrino formed from the face-changing would be observed on the journey. Therefore, a special and easy way to judge the physical nature of neutrinos may be suggested the reactor neutrino experimental groups all over the world, in addition to the current studies involving the disappearance mode of , to add a new experimental search after ve in the current, to see whether a few ve neutrinos would exceed the background counting. “Yes” result would reveal the neutrinos being tachyons, and “no” would be not. 展开更多
关键词 Special RELATIVITY in Space-Like Region TACHYON Face-Changing EFFECT mother neutron in β-decay Reactor NEUTRINO Experiments
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Determination of isospin asymmetry effects on α-decay 被引量:1
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作者 B.A.Gheshlagh O.N.Ghodsi 《Chinese Physics C》 SCIE CAS CSCD 2019年第12期100-106,共7页
In this study,we compared the effect of the isospin asymmetry of proton and neutron density distributions in the neutron skin-type(NST)case and in the Hartree-Fock formalism(HF)on the half-life of alpha emitters with ... In this study,we compared the effect of the isospin asymmetry of proton and neutron density distributions in the neutron skin-type(NST)case and in the Hartree-Fock formalism(HF)on the half-life of alpha emitters with the atomic number in the range of 82≤Z≤92.The NST case and HF formalism based on the Skyrme-SLy4 effective interaction reveal different isospin asymmetries for selected alpha emitters.Furthermore,the obtained results reveal an increase in theα-decay widths of about 30%for the NST case in comparison with the equivalent values obtained by HF formalism.The standard deviations for calculated half-lives within the NST case and HF formalism are about 0.438 and 0.391,respectively. 展开更多
关键词 Α-decay HALF-LIFE PREFORMATION factor ISOSPIN asymmetry neutron SKIN thickness
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超铀区缺中子新核素的研究
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作者 郭俊盛 李文新 +2 位作者 刘洪业 甘再国 雷怀宏 《核物理动态》 CSCD 1993年第2期22-24,共3页
超铀核的合成历史及现状,产生缺中子超铀新核素可能的弹靶组合、生成截面的估计和裂变竞争的修正,氦喷咀传输系统及转动轮收集系统是主要的实验装置;而采用母女探测器系统,可以建立产物母子体的遗传关系,从而鉴别未知核。
关键词 超铀核 裂变产物 同位素
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