dc.contributor.author | Canete, Laetitia | |
dc.contributor.author | Eronen, Tommi | |
dc.contributor.author | Jokinen, Ari | |
dc.contributor.author | Kankainen, Anu | |
dc.contributor.author | Moore, Iain | |
dc.contributor.author | Nesterenko, Dmitrii | |
dc.contributor.author | Rinta-Antila, Sami | |
dc.contributor.editor | Cognata, M. La | |
dc.contributor.editor | Lattuada, M. | |
dc.contributor.editor | Palmerini, S. | |
dc.contributor.editor | Pizzone, R.G. | |
dc.contributor.editor | Spitaleri, C. | |
dc.date.accessioned | 2018-01-12T10:09:39Z | |
dc.date.available | 2018-01-12T10:09:39Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Canete, L., Eronen, T., Jokinen, A., Kankainen, A., Moore, I., Nesterenko, D., & Rinta-Antila, S. (2017). High-precision mass measurements for the rp-process at JYFLTRAP. In M. L. Cognata, M. Lattuada, S. Palmerini, R. Pizzone, & C. Spitaleri (Eds.), <i>Nuclear Physics in Astrophysics VIII (NPA8 2017) Catania, Italy, June 18-23, 2017</i> (Article 01008). EDP Sciences. EPJ Web of Conferences, 165. <a href="https://doi.org/10.1051/epjconf/201716501008" target="_blank">https://doi.org/10.1051/epjconf/201716501008</a> | |
dc.identifier.other | CONVID_27831097 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/56698 | |
dc.description.abstract | The double Penning trap JYFLTRAP at the University of Jyvaskyla has been successfully used to achieve high-precision mass measurements of nuclei involved in the rapid proton-capture (rp) process. A precise mass measurement of 31Cl is essential to estimate the waiting point condition of 30S in the rp-process occurring in type I x-ray bursts (XRBs). The mass-excess of 31Cl measured at JYFLTRAP, -7034.7(3.4) keV, is 15 more precise than the value given in the Atomic Mass Evaluation 2012. The proton separation energy Sp determined from the new mass-excess value confirmed that 30S is a waiting point, with a lowertemperature limit of 0.44 GK. The mass of 52Co effects both 51Fe(p,γ)52Co and 52Co(p,γ)53Ni reactions. The mass-excess value measured, - 34 331.6(6.6) keV is 30 times more precise than the value given in AME2012. The Q values for the 51Fe(p,γ)52Co and 52Co(p,γ)53Ni reactions are now known with a high precision, 1418(11) keV and 2588(26) keV respectively. The results show that 52Co is more proton bound and 53Ni less proton bound than what was expected from the extrapolated value. | en |
dc.language | eng | |
dc.language.iso | eng | |
dc.publisher | EDP Sciences | |
dc.relation.ispartof | Nuclear Physics in Astrophysics VIII (NPA8 2017) Catania, Italy, June 18-23, 2017 | |
dc.relation.ispartofseries | EPJ Web of Conferences | |
dc.subject.other | Atomic Weights | |
dc.subject.other | Antiprotons | |
dc.subject.other | Ion Traps (Instrumentation) | |
dc.title | High-precision mass measurements for the rp-process at JYFLTRAP | |
dc.type | conference paper | |
dc.identifier.urn | URN:NBN:fi:jyu-201801091123 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.oppiaine | Kiihdytinlaboratorio | fi |
dc.contributor.oppiaine | Accelerator Laboratory | en |
dc.type.uri | http://purl.org/eprint/type/ConferencePaper | |
dc.date.updated | 2018-01-09T13:15:09Z | |
dc.relation.isbn | 978-2-7598-9030-9 | |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2101-6275 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © The Authors, published by EDP Sciences, 2017. This is an open access article distributed under the terms of the Creative Commons License. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | conferenceObject | |
dc.relation.conference | Nuclear Physics in Astrophysics | |
dc.relation.grantnumber | 275389 | |
dc.relation.grantnumber | 284516 | |
dc.subject.yso | protonit | |
dc.subject.yso | nukleonit | |
dc.subject.yso | atomipainot | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p12428 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p12429 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p5801 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1051/epjconf/201716501008 | |
dc.relation.funder | Suomen Akatemia | fi |
dc.relation.funder | Suomen Akatemia | fi |
dc.relation.funder | Academy of Finland | en |
dc.relation.funder | Academy of Finland | en |
jyx.fundingprogram | Akatemiatutkija, SA | fi |
jyx.fundingprogram | Akatemiatutkijan tutkimuskulut, SA | fi |
jyx.fundingprogram | Academy Research Fellow, AoF | en |
jyx.fundingprogram | Research costs of Academy Research Fellow, AoF | en |
jyx.fundinginformation | This work has been supported by the Academy of Finland under projects No. 275389 and 284516 as
well as under the Finnish Centre of Excellence Programme 2012-2017 (Nuclear and Accelerator
Based Physics Research at JYFL) | |
dc.type.okm | A4 | |