Publication: Evidence for the First Excited State of H 7
dc.contributor.author | Bezbakh, A. A. | |
dc.contributor.author | Chudoba, V. | |
dc.contributor.author | Krupko, S. A. | |
dc.contributor.author | Biare, D. | |
dc.contributor.author | Belogurov, S. G. | |
dc.contributor.author | Grigorenko, L. V. | |
dc.contributor.author | Белогуров, Сергей Геннадьевич | |
dc.contributor.author | Григоренко, Леонид Валентинович | |
dc.date.accessioned | 2024-11-25T15:56:33Z | |
dc.date.available | 2024-11-25T15:56:33Z | |
dc.date.issued | 2020 | |
dc.description.abstract | © 2020 American Physical Society.The H7 system was populated in the H2(He8,He3)H7 reaction with a 26 AMeV He8 beam. The H7 missing mass energy spectrum, the H3 energy and angular distributions in the H7 decay frame were reconstructed. The H7 missing mass spectrum shows a peak, which can be interpreted either as unresolved 5/2+ and 3/2+ doublet or one of these states at 6.5(5) MeV. The data also provide indications of the 1/2+ ground state of H7 located at 1.8(5) MeV with quite a low population cross section of ∼25 μb/sr within angular range θc.m.≃(17°-27°). | |
dc.identifier.citation | Evidence for the First Excited State of H 7 / Bezbakh, A.A. [et al.] // Physical Review Letters. - 2020. - 124. - № 2. - 10.1103/PhysRevLett.124.022502 | |
dc.identifier.doi | 10.1103/PhysRevLett.124.022502 | |
dc.identifier.uri | https://www.doi.org/10.1103/PhysRevLett.124.022502 | |
dc.identifier.uri | https://www.scopus.com/record/display.uri?eid=2-s2.0-85078572983&origin=resultslist | |
dc.identifier.uri | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000515350300004 | |
dc.identifier.uri | https://openrepository.mephi.ru/handle/123456789/20218 | |
dc.relation.ispartof | Physical Review Letters | |
dc.title | Evidence for the First Excited State of H 7 | |
dc.type | Article | |
dspace.entity.type | Publication | |
oaire.citation.issue | 2 | |
oaire.citation.volume | 124 | |
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