6533b837fe1ef96bd12a3831

RESEARCH PRODUCT

First β-decay spectroscopy of $^{135}$In and new $β$-decay branches of $^{134}$In

M. Piersa-siłkowskaA. KorgulJ. BenitoL.m. FraileE. AdamskaA.n. AndreyevR. ÁLvarez-rodríguezA.e. BarzakhG. BenzoniT. BerryM.j.g. BorgeM. CarmonaK. ChrysalidisJ.g. CorreiaC. CostacheJ.g. CubissT. Day GoodacreH. De WitteD.v. FedorovV.n. FedosseevG. Fernández-martínezA. FijałkowskaH. FynboD. GalavizP. GalveM. García-díezP.t. GreenleesR. GrzywaczL.j. Harkness-brennanC. HenrichM. HuyseP. IbáñezA. IllanaZ. JanasK. JohnstonJ. JolieD.s. JudsonV. KaranyonchevM. Kicińska-habiorJ. KonkiŁ. KoszukJ. KurcewiczI. LazarusR. LicăA. López-montesH. MachM. MadurgaI. MarroquínB. MarshM.c. MartínezC. MazzocchiK. MiernikC. MihaiN. MărgineanR. MărgineanA. NegretE. NácherJ. OjalaB. OlaizolaR.d. PageJ. PakarinenS. PascuS.v. PaulauskasA. PereaV. PucknellP. RahkilaC. RaisonE. RapisardaK. RezynkinaF. RotaruS. RotheK.p. RykaczewskiJ.-m. RégisK. SchomackerM. SiłkowskiG. SimpsonC. SottyL. StanM. StănoiuM. StryjczykD. Sánchez-parcerisaV. Sánchez-temblequeO. TengbladA. TurturicăJ.m. UdíasP. Van DuppenV. VediaA. VillaS. ViñalsR. WadsworthW.b. WaltersN. WarrS.g. Wilkins

subject

isotoopitmittausAstrophysics::High Energy Astrophysical PhenomenaspektroskopiaNuclear TheoryNuclear Physics - Experimentneutronit[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]fysiikkaydinfysiikkaNuclear ExperimentNuclear Experiment

description

International audience; The $\beta$ decay of the neutron-rich $^{134}$In and $^{135}$In was investigated experimentally in order to provide new insights into the nuclear structure of the tin isotopes with magic proton number $Z=50$ above the $N=82$ shell. The $\beta$-delayed $\gamma$-ray spectroscopy measurement was performed at the ISOLDE facility at CERN, where indium isotopes were selectively laser-ionized and on-line mass separated. Three $\beta$-decay branches of $^{134}$In were established, two of which were observed for the first time. Population of neutron-unbound states decaying via $\gamma$ rays was identified in the two daughter nuclei of $^{134}$In, $^{134}$Sn and $^{133}$Sn, at excitation energies exceeding the neutron separation energy by 1 MeV. The $\beta$-delayed one- and two-neutron emission branching ratios of $^{134}$In were determined and compared with theoretical calculations. The $\beta$-delayed one-neutron decay was observed to be dominant $\beta$-decay branch of $^{134}$In even though the Gamow-Teller resonance is located substantially above the two-neutron separation energy of $^{134}$Sn. Transitions following the $\beta$ decay of $^{135}$In are reported for the first time, including $\gamma$ rays tentatively attributed to $^{135}$Sn. In total, six new levels were identified in $^{134}$Sn on the basis of the $\beta \gamma \gamma$ coincidences observed in the $^{134}$In and $^{135}$In $\beta$ decays. A transition that might be a candidate for deexciting the missing neutron single-particle $13/2^+$ state in $^{133}$Sn was observed in both $\beta$ decays and its assignment is discussed. Experimental level schemes of $^{134}$Sn and $^{135}$Sn are compared with shell-model predictions. Using the fast timing technique, half-lives of the $2^+$, $4^+$ and $6^+$ levels in $^{134}$Sn were determined.

10.1103/physrevc.104.044328http://cds.cern.ch/record/2789022