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Nuclear Double Beta Decay, Fundamental Particle Physics, Hot Dark Matter, And Dark Energy

机译:核双β衰变,基本粒子物理,热暗   物质和暗能量

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摘要

Nuclear double beta decay, an extremely rare radioactive decay process, is -in one of its variants - one of the most exciting means of research intoparticle physics beyond the standard model. The large progress in sensitivityof experiments searching for neutrinoless double beta decay in the last twodecades - based largely on the use of large amounts of enriched source materialin "active source experiments" - has lead to the observation of the occurrenceof this process in nature (on a 6.4 sigma level), with the largest half-lifeever observed for a nuclear decay process (2.2 x 10^{25} y). This hasfundamental consequences for particle physics - violation of lepton number,Majorana nature of the neutrino. These results are independent of anyinformation on nuclear matrix elements (NME)*. It further leads to sharprestrictions for SUSY theories, sneutrino mass, right-handed W-boson mass,superheavy neutrino masses, compositeness, leptoquarks, violation of Lorentzinvariance and equivalence principle in the neutrino sector. The masses oflight-neutrinos are found to be degenerate, and to be at least 0.22 +- 0.02 eV.This fixes the contribution of neutrinos as hot dark matter to >=4.7% of thetotal observed dark matter. The neutrino mass determined might solve also thedark energy puzzle. *(It is briefly discussed how important NME for 0nubb decayreally are.)
机译:核双β衰变是一种极为罕见的放射性衰变过程,在其变体之一中,它是标准模型以外研究粒子物理学的最令人兴奋的手段之一。在过去的两个十年中,寻找无中微子双β衰变的实验在灵敏度方面取得了巨大进展-主要是基于在“活性源实验”中使用了大量的富集源物质-导致人们观察到自然界中该过程的发生( 6.4σ级),在核衰变过程中观察到最大的半衰期(2.2 x 10 ^ {25} y)。这对粒子物理学有根本性的影响-轻子数的违反,中微子的主要性质。这些结果与有关核基质元素(NME)*的任何信息无关。它进一步导致对SUSY理论,中微子质量,右旋W玻色子质量,超重中微子质量,复合性,瘦夸克,中微子领域违反Lorentzinvariance和等价原理的严格限制。发现轻中微子的质量已退化,并且至少为0.22±-0.02 eV,这将中微子作为热暗物质的贡献固定为总观测暗物质的> = 4.7%。确定的中微子质量也可能解决暗能量难题。 *(简要讨论了NME对于0nubb衰减的重要性。)

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