PHELEX:寻找暗光子的两个测量系列

A. Kopylov, I. Orekhov, V. Petukhov, A. Solomatin
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摘要

本报告介绍了两个系列的测量结果,每个系列 4 次,每次约 50 天。在这些测量中使用了带铁阴极的多阴极计数器。在这两个系列中,我们观测到恒星时的计数率有些过高,而在地球时则没有观测到过高的计数率。在22年12月27日至23年7月24日的第一个系列中,我们观测到恒星时上午8时至12时期间的超额率,置信度超过6(sigma);在23年9月21日至24年4月3日的第二个系列中,我们观测到恒星时下午6时至10时期间的超额率,置信度超过4(sigma)。在地球时,我们没有观测到与恒星时类似的效应,这一事实表明,这种效应很可能源自银河系,而且可能是由暗光子引起的。建议今后采取措施验证这些结果。
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PHELEX: Two Series of Measurements in the Search for Dark Photons
The results of measurements in two series, each series of 4 Runs and about 50 days each Run, are presented. A multi-cathode counter with an iron cathode is used in these measurements. In both series we have observed some excess in count rates in sidereal time while no excess has been observed in terrestrial time. In the first series from 27.12.22 to 24.07.23 we have observed the excess in the period between 8 a.m. and 12 a.m. of sidereal time with a confidence level more than 6 \sigma, in the second series from 21.09.23 to 03.04.24 in the period between 6 p.m. and 10 p.m. of sidereal time with a confidence level more than 4 \sigma. The fact that in terrestrial time we do not observe a similar effect as in sidereal time suggests that probably this effect is of galactic origin and that this may be caused by dark photons. Future steps are suggested to validate these results.
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