S. N. Mayburov, E. I. Demikhov, A. S. Kubankin, I. A. Kishin, Yu. E. Titarenko, K. V. Pavlov, V. M. Zhivun, Ya. O. Zaricki
{"title":"太阳活动与55Fe, 60Co核衰变参数的相关性研究","authors":"S. N. Mayburov, E. I. Demikhov, A. S. Kubankin, I. A. Kishin, Yu. E. Titarenko, K. V. Pavlov, V. M. Zhivun, Ya. O. Zaricki","doi":"10.1134/S1062873825711213","DOIUrl":null,"url":null,"abstract":"<p>Temporal variations of nuclei decay parameters are actively studied now; their detection may be a signal of new physical effects of cosmic origin. Correlations of <sup>60</sup>Co, <sup>54</sup>Mn, and <sup>55</sup>Fe weak decay parameters with solar activity, in particular with solar flares, were observed earlier. In our work, correlations of X-class solar flares with <sup>60</sup>Co and <sup>55</sup>Fe decay rate variations are measured via decay γ-ray detection by semiconductor detectors. For <sup>55</sup>Fe decay eight significant deviations of decay counting rate from the expected rate observed at the level ∼0.2% during 48–96 h, correlated with solar flares. For <sup>60</sup>Co decay four analogous flare events were detected with deviations at the level of ∼0.4%. All decay rate deviations have advanced character and begin from 30 to 155 h before solar flare moments at confidence level of 90%.</p>","PeriodicalId":504,"journal":{"name":"Bulletin of the Russian Academy of Sciences: Physics","volume":"89 6","pages":"817 - 820"},"PeriodicalIF":0.4800,"publicationDate":"2025-07-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Search of Correlations of Solar Activity with 55Fe, 60Co Nucleus Decay Parameters\",\"authors\":\"S. N. Mayburov, E. I. Demikhov, A. S. Kubankin, I. A. Kishin, Yu. E. Titarenko, K. V. Pavlov, V. M. Zhivun, Ya. O. Zaricki\",\"doi\":\"10.1134/S1062873825711213\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Temporal variations of nuclei decay parameters are actively studied now; their detection may be a signal of new physical effects of cosmic origin. Correlations of <sup>60</sup>Co, <sup>54</sup>Mn, and <sup>55</sup>Fe weak decay parameters with solar activity, in particular with solar flares, were observed earlier. In our work, correlations of X-class solar flares with <sup>60</sup>Co and <sup>55</sup>Fe decay rate variations are measured via decay γ-ray detection by semiconductor detectors. For <sup>55</sup>Fe decay eight significant deviations of decay counting rate from the expected rate observed at the level ∼0.2% during 48–96 h, correlated with solar flares. For <sup>60</sup>Co decay four analogous flare events were detected with deviations at the level of ∼0.4%. All decay rate deviations have advanced character and begin from 30 to 155 h before solar flare moments at confidence level of 90%.</p>\",\"PeriodicalId\":504,\"journal\":{\"name\":\"Bulletin of the Russian Academy of Sciences: Physics\",\"volume\":\"89 6\",\"pages\":\"817 - 820\"},\"PeriodicalIF\":0.4800,\"publicationDate\":\"2025-07-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Bulletin of the Russian Academy of Sciences: Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S1062873825711213\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin of the Russian Academy of Sciences: Physics","FirstCategoryId":"1085","ListUrlMain":"https://link.springer.com/article/10.1134/S1062873825711213","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
Search of Correlations of Solar Activity with 55Fe, 60Co Nucleus Decay Parameters
Temporal variations of nuclei decay parameters are actively studied now; their detection may be a signal of new physical effects of cosmic origin. Correlations of 60Co, 54Mn, and 55Fe weak decay parameters with solar activity, in particular with solar flares, were observed earlier. In our work, correlations of X-class solar flares with 60Co and 55Fe decay rate variations are measured via decay γ-ray detection by semiconductor detectors. For 55Fe decay eight significant deviations of decay counting rate from the expected rate observed at the level ∼0.2% during 48–96 h, correlated with solar flares. For 60Co decay four analogous flare events were detected with deviations at the level of ∼0.4%. All decay rate deviations have advanced character and begin from 30 to 155 h before solar flare moments at confidence level of 90%.
期刊介绍:
Bulletin of the Russian Academy of Sciences: Physics is an international peer reviewed journal published with the participation of the Russian Academy of Sciences. It presents full-text articles (regular, letters to the editor, reviews) with the most recent results in miscellaneous fields of physics and astronomy: nuclear physics, cosmic rays, condensed matter physics, plasma physics, optics and photonics, nanotechnologies, solar and astrophysics, physical applications in material sciences, life sciences, etc. Bulletin of the Russian Academy of Sciences: Physics focuses on the most relevant multidisciplinary topics in natural sciences, both fundamental and applied. Manuscripts can be submitted in Russian and English languages and are subject to peer review. Accepted articles are usually combined in thematic issues on certain topics according to the journal editorial policy. Authors featured in the journal represent renowned scientific laboratories and institutes from different countries, including large international collaborations. There are globally recognized researchers among the authors: Nobel laureates and recipients of other awards, and members of national academies of sciences and international scientific societies.