6533b872fe1ef96bd12d2d48

RESEARCH PRODUCT

β-decay studies of135–137Snusing selective resonance laser ionization techniques

B. A. BrownM. HannawaldP. HoffKarl KratzD. FedorovH. O. U. FynboUlli KösterThomas NilssonJ. J. ResslerV. N. FedoseyevA. A. BickleyHenryk MachA. WöhrK. Wilhelmsen-rolanderWilliam B. WaltersB. PfeifferD. SeweryniakD. SeweryniakJ. ShergurMorten Hjorth-jensenV. I. MishinH. Simon

subject

PhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaIonizationDouble beta decayExcited stateNeutronAtomic physicsMass spectrometryGround stateBeta decayDelayed neutron

description

The decays of the very neutron rich Sn isotopes Sn135-137 were studied at CERN/ISOLDE using isotopic and isobaric selectivity achieved by the use of a resonance ionization laser ion source and mass spectroscopy, respectively. Neutron decay rates, gamma-ray singles, and gamma-gamma coincidence data were collected as a function of time. The half-life (T-1/2) and delayed neutron emission probability (P-n) values of 135 Sn were measured to be 530(20) ms and 21(3)%, respectively. For Sn-136, a T-1/2 of 250(30) ms was determined along with a P-n value of 30(5)%. For Sn-137, a T-1/2 of 190(60) ms and a P-n value of 58(15)% were deduced. Identification of low-energy transitions in Sb-135 was made possible by comparison of laser-on and laser-off gamma-ray spectra. Those data combined with gamma-gamma coincidence spectra were used to construct a level scheme for Sb-135 that includes an unexpectedly low first excited state at 282 keV. A ground state beta branch of 33.2% was measured by following the growth and decay of the Sb-135 daughter. Shell-model calculations are consistent with the observed Sb-135 level structure and can account for a lowered first excited state.

https://doi.org/10.1103/physrevc.65.034313