Search for periodic modulations of the rate of double-β decay of Mo100 in the NEMO-3 detector
| dc.contributor.author | The NEMO-3 Collaboration | |
| dc.date.accessioned | 2022-01-19T10:52:20Z | |
| dc.date.available | 2022-01-19T10:52:20Z | |
| dc.date.issued | 2021 | |
| dc.identifier.citation | The NEMO-3 Collaboration. (2021). Search for periodic modulations of the rate of double-β decay of Mo100 in the NEMO-3 detector. <i>Physical Review C</i>, <i>104</i>(6), Article L061601. <a href="https://doi.org/10.1103/PhysRevC.104.L061601" target="_blank">https://doi.org/10.1103/PhysRevC.104.L061601</a> | |
| dc.identifier.other | CONVID_103911717 | |
| dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/79430 | |
| dc.description.abstract | Double-beta decays of 100Mo from the 6.0195-year exposure of a 6.914 kg high-purity sample were recorded by the NEMO-3 experiment that searched for neutrinoless double-beta decays. These ultrarare transitions to 100Ru have a half-life of approximately 7×1018 years and have been used to conduct the first-ever search for periodic variations of this decay mode. The Lomb-Scargle periodogram technique, and its error-weighted extension, were employed to look for periodic modulations of the half-life. Data show no evidence at the 95% confidence level of modulations with amplitude greater than 2.5% in the frequency range of 0.33225yr−1 to 360yr−1. | en |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | American Physical Society (APS) | |
| dc.relation.ispartofseries | Physical Review C | |
| dc.rights | In Copyright | |
| dc.title | Search for periodic modulations of the rate of double-β decay of Mo100 in the NEMO-3 detector | |
| dc.type | research article | |
| dc.identifier.urn | URN:NBN:fi:jyu-202201191198 | |
| dc.contributor.laitos | Fysiikan laitos | fi |
| dc.contributor.laitos | Department of Physics | en |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
| dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
| dc.description.reviewstatus | peerReviewed | |
| dc.relation.issn | 2469-9985 | |
| dc.relation.numberinseries | 6 | |
| dc.relation.volume | 104 | |
| dc.type.version | publishedVersion | |
| dc.rights.copyright | © 2021 American Physical Society | |
| dc.rights.accesslevel | openAccess | fi |
| dc.type.publication | article | |
| dc.subject.yso | puoliintumisaika | |
| dc.subject.yso | ydinfysiikka | |
| dc.subject.yso | molybdeeni | |
| dc.subject.yso | isotoopit | |
| dc.format.content | fulltext | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p12173 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p11107 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p6387 | |
| dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
| dc.relation.doi | 10.1103/PhysRevC.104.L061601 | |
| jyx.fundinginformation | We acknowledge support by the grant agencies of the Czech Republic, CNRS/IN2P3 in France, RFBR in Russia (NCNIL No19-52-16002), APVV in Slovakia, the Science and Technology Facilities Council, part of U.K. Research and Innovation, and the NSF in the USA. | |
| dc.type.okm | A1 |
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