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Search for time modulations in the decay constant of 40K and 226Ra at the underground Gran Sasso Laboratory

机译:在地下Gran上的 40 K和 226 Ra的衰减常数中搜索时间调制萨索实验室

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Time modulations at per mil level have been reported to take place in the decay constant of several nuclei with period of one year (most cases) but also of about one month or one day. On the other hand, experiments with similar or better sensitivity have been unable to detect any modulation. In this letter we give the results of the activity study of two different sources: 40 K and 226 Ra. The two gamma spectrometry experiments have been performed underground at the Gran Sasso Laboratory, this way suppressing the time dependent cosmic ray background. Briefly, our measurements reached the sensitivity of 3.4 and 3.5 parts over 10 6 for 40 K and 226 Ra, respectively (1 sigma) and they do not show any statistically significant evidence of time dependence in the decay constant. We also give the results of the activity measurement at the time of the two strong X-class solar flares which took place in September 2017. Our data do not show any unexpected time dependence in the decay rate of 40 K in correspondence with the two flares. To the best of our knowledge, these are the most precise and accurate results on the stability of the decay constant as function of time.
机译:据报道,每密耳级的时间调制发生在几个原子核的衰变常数中,周期为一年(大多数情况下),但周期约为一个月或一天。另一方面,具有相似或更好灵敏度的实验无法检测到任何调制。在这封信中,我们给出了两种不同来源的活性研究结果:40 K和226 Ra。在Gran Sasso实验室的地下进行了两次伽马能谱实验,以这种方式抑制了时间相关的宇宙射线背景。简而言之,对于40 K和226 Ra(1 sigma),我们的测量分别在10 6上达到了3.4和3.5的灵敏度,并且它们没有显示任何统计上显着的衰减常数与时间相关的证据。我们还给出了在2017年9月发生的两次强X级太阳耀斑时的活度测量结果。我们的数据没有显示出与这两个耀斑相对应的40 K衰减率中任何意外的时间依赖性。据我们所知,这是衰减常数作为时间函数的稳定性的最精确和最准确的结果。

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