P. Belli, R. Bernabei, F. Cappella, V. Caracciolo, R. Cerulli, F. A. Danevich, V. Yu. Denisov, A. Incicchitti, D. V. Kasperovych, V. V. Kobychev, G. P. Kovtun, M. Laubenstein, D. V. Poda, O. G. Polischuk, A. P. Shcherban, D. A. Solopikhin, S. Tessalina, V. I. Tretyak
{"title":"Final results of the measurement to search for rare decays of naturally occurring osmium isotopes with ultra-low background gamma-ray spectrometry","authors":"P. Belli, R. Bernabei, F. Cappella, V. Caracciolo, R. Cerulli, F. A. Danevich, V. Yu. Denisov, A. Incicchitti, D. V. Kasperovych, V. V. Kobychev, G. P. Kovtun, M. Laubenstein, D. V. Poda, O. G. Polischuk, A. P. Shcherban, D. A. Solopikhin, S. Tessalina, V. I. Tretyak","doi":"arxiv-2406.19062","DOIUrl":null,"url":null,"abstract":"A long-term measurement was conducted to search for $\\alpha$, double-$\\alpha$\nand double-$\\beta$ decays with $\\gamma$ quanta emission in naturally occurring\nosmium isotopes. This study took advantage of two ultra-low background HPGe\ndetectors and one ultra-low background BEGe detector at the Gran Sasso National\nLaboratory (LNGS) of the INFN. Over almost 5 years of data were taken using\nhigh-purity osmium samples of approximately 173 g. The half-life limits set for\na decays of $^{184}$Os to the first $2^+$ 103.6 keV excited level of $^{180}$W\n($T_{1/2} > 9.3 \\times 10^{15}$ yr) and of $^{186}$Os to the first $2^+$ 100.1\nkeV of $^{182}$W ($T_{1/2} > 4.8 \\times 10^{17}$ yr) exceed substantially the\npresent theoretical predictions that are at level of $T_{1/2} \\sim (0.6 - 3)\n\\times 10^{15}$ yr for $^{184}$Os and $T_{1/2} \\sim (0.3 - 2) \\times 10^{17}$\nyr for $^{186}$Os. New half-life limits on the 2EC and EC$\\beta^+$ decay of\n$^{184}$Os to the ground and excited levels of $^{184}$W were set at level of\n$T_{1/2} > 10^{16} - 10^{17}$ yr; a lower limit on the $2\\beta^-$ decay of\n$^{192}$Os to the $2^+$ 316.5 keV excited level of $^{192}$Pt was estimated as\n$T_{1/2} > 6.1 \\times 10^{20}$ yr. The half-life limits for $2\\alpha$ decay of\n$^{189}$Os and $^{192}$Os were set for the first time at level of $T_{1/2} >\n10^{20}$ yr.","PeriodicalId":501206,"journal":{"name":"arXiv - PHYS - Nuclear Experiment","volume":"27 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-06-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Nuclear Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2406.19062","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
A long-term measurement was conducted to search for $\alpha$, double-$\alpha$
and double-$\beta$ decays with $\gamma$ quanta emission in naturally occurring
osmium isotopes. This study took advantage of two ultra-low background HPGe
detectors and one ultra-low background BEGe detector at the Gran Sasso National
Laboratory (LNGS) of the INFN. Over almost 5 years of data were taken using
high-purity osmium samples of approximately 173 g. The half-life limits set for
a decays of $^{184}$Os to the first $2^+$ 103.6 keV excited level of $^{180}$W
($T_{1/2} > 9.3 \times 10^{15}$ yr) and of $^{186}$Os to the first $2^+$ 100.1
keV of $^{182}$W ($T_{1/2} > 4.8 \times 10^{17}$ yr) exceed substantially the
present theoretical predictions that are at level of $T_{1/2} \sim (0.6 - 3)
\times 10^{15}$ yr for $^{184}$Os and $T_{1/2} \sim (0.3 - 2) \times 10^{17}$
yr for $^{186}$Os. New half-life limits on the 2EC and EC$\beta^+$ decay of
$^{184}$Os to the ground and excited levels of $^{184}$W were set at level of
$T_{1/2} > 10^{16} - 10^{17}$ yr; a lower limit on the $2\beta^-$ decay of
$^{192}$Os to the $2^+$ 316.5 keV excited level of $^{192}$Pt was estimated as
$T_{1/2} > 6.1 \times 10^{20}$ yr. The half-life limits for $2\alpha$ decay of
$^{189}$Os and $^{192}$Os were set for the first time at level of $T_{1/2} >
10^{20}$ yr.