High-multiplicity neutron events registered by NEMESIS experiment
dc.contributor.author | Kasztelan Marcin | |
dc.contributor.author | Enqvist, T. | |
dc.contributor.author | Jędrzejczak, K. | |
dc.contributor.author | Joutsenvaara, J. | |
dc.contributor.author | Kotavaara, O. | |
dc.contributor.author | Kuusiniemi, P. | |
dc.contributor.author | Loo, K.K. | |
dc.contributor.author | Orzechowski, J. | |
dc.contributor.author | Puputti, J. | |
dc.contributor.author | Sobkow, A. | |
dc.contributor.author | Słupecki, M. | |
dc.contributor.author | Szabelski, J. | |
dc.contributor.author | Usoskin, I. | |
dc.contributor.author | Trzaska, W.H. | |
dc.contributor.author | Ward, T.E. | |
dc.date.accessioned | 2022-02-08T12:01:10Z | |
dc.date.available | 2022-02-08T12:01:10Z | |
dc.date.issued | 2021 | |
dc.identifier.citation | Kasztelan Marcin, Enqvist, T., Jędrzejczak, K., Joutsenvaara, J., Kotavaara, O., Kuusiniemi, P., Loo, K.K., Orzechowski, J., Puputti, J., Sobkow, A., Słupecki, M., Szabelski, J., Usoskin, I., Trzaska, W.H., Ward, T.E. (2021). High-multiplicity neutron events registered by NEMESIS experiment. In <i>ICRC 2021 : 37th International Cosmic Ray Conference</i> (pp. 1-8). Sissa. POS Proceedings of Science, 497. <a href="https://doi.org/10.22323/1.395.0497" target="_blank">https://doi.org/10.22323/1.395.0497</a> | |
dc.identifier.other | CONVID_104155808 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/79687 | |
dc.description.abstract | Neutron-induced interactions contribute to the signal-mimicking background in deep-underground searches for exotic phenomena such as Dark Matter, neutrino-less double beta decay, proton decay, etc. Apart from radioactive decay, the primary source of neutrons underground are high-energy muons from cosmic showers. While the maximum number of fission neutrons is around six and energies around one MeV, muon-induced interactions may generate hundreds of neutrons, also with high energies. Furthermore, these processes are not yet reproduced in numerical simulations with sufficient reliability. The main goal of the NEMESIS experiment is to improve our knowledge and understanding of cosmic muon-induced neutron production in high-Z targets. NEMESIS (New Emma MEasurementS Including neutronS) is taking data at a depth of 210 m.w.e. in Callio Lab in the Pyhäsalmi mine, Finland. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Sissa | |
dc.relation.ispartof | ICRC 2021 : 37th International Cosmic Ray Conference | |
dc.relation.ispartofseries | POS Proceedings of Science | |
dc.rights | CC BY-NC-ND 4.0 | |
dc.title | High-multiplicity neutron events registered by NEMESIS experiment | |
dc.type | conferenceObject | |
dc.identifier.urn | URN:NBN:fi:jyu-202202081439 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/ConferencePaper | |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | |
dc.description.reviewstatus | nonPeerReviewed | |
dc.format.pagerange | 1-8 | |
dc.relation.issn | 1824-8039 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © Copyright owned by the authors | |
dc.rights.accesslevel | openAccess | fi |
dc.relation.conference | International Cosmic Ray Conference | |
dc.subject.yso | hiukkasfysiikka | |
dc.subject.yso | neutronit | |
dc.subject.yso | fysiikka | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | radioaktiivinen säteily | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15394 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p900 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p458 | |
dc.rights.url | https://creativecommons.org/licenses/by-nc-nd/4.0/ | |
dc.relation.doi | 10.22323/1.395.0497 | |
jyx.fundinginformation | This work was financially supported in part by the EU (INTERREG for Baltic Sea programme) as part of the BSUIN project, and by the Polish Ministry of Science and Higher Education (grant no. 3988/INTERREG BSR/2018/2). | |
dc.type.okm | B3 |