Alpha decay and double alpha decay are significant decay modes in heavy and super-heavy nuclei. Alpha decay, identified by Ernest Rutherford in 1899 [1] and explained with Frederick Soddy (1902–1903), involves the emission of a helium nucleus (2 protons and 2 neutrons), causing the parent atom to transform into a new element. This well-studied process has been instrumental in understanding nuclear stability and decay chains [2].
Double alpha decay (2α decay), a rare nuclear process, results in the simultaneous or sequential emission of two alpha particles. Theoretical predictions were first made by Giulio Racah, with further insights from Hafstad and Teller (1938) through nuclear cluster models. The first specific prediction of spontaneous double alpha emission was made by Poenaru et al. (1985) [3]. Despite its theoretical importance, experimental observations remain limited. Recent studies, such as Tretyak (2021) [4], have explored double alpha emission from naturally abundant isotopes, pushing the boundaries of nuclear decay research.
Significance of Research: The study of alpha and double alpha decay provides essential insights into nuclear structure and decay mechanisms. It has helped refine nuclear models and cluster theories, enhancing predictions about super-heavy elements. Researchers also explore these decays for their potential role in detecting rare isotopes and studying neutron-proton correlations within nuclei, which could lead to breakthroughs in both theoretical and applied nuclear science.
Alpha Decay vs. Double Alpha Decay:
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