Engineering topics

Alanssari, M.

Publications and source records attributed to Alanssari, M..

4 records

DOE OSTI2017

Mass determination near N = 20 for Al and Na isotopes

We report on the mass measurements of 31;32 Na and 29;34;35 Al, performed with the TITAN Penning trap mass spectrometer at TRIUMF. The mass excesses were found to be 12246(14) keV and 18638(37) keV for 31;32 Na and -18207:77(37) keV, -3000:5(29) keV, and -223:7(73) keV for 29;34;35 Al, respectively. Our measurements con rm the observation of a crossover in the two-neutron separation energies of 33 Mg and 34 Al. We did not observe the recently reported, long-lived, isomeric state of 34 Al, but, based on the previously measured half-lives, the mass value of the ground state was determined.

73 NUCLEAR PHYSICS AND RADIATION PHYSICS↗

DOE OSTI2016

High energy-resolution measurement of the Se 82 ( He 3 , t ) Br 82 reaction for double- β decay and for solar neutrinos

For this study, a high-resolution ( 3 He,t) charge-exchange experiment at an incident energy of 420 MeV has been performed on the double beta (ββ) decay nucleus 82 Se. A detailed Gamow-Teller (GT - ) strength distribution in 82 Br has been extracted, which provides information to the ββ-decay nuclear matrix elements. Three strong and isolated transitions, which are to the 75, 1484 and the 2087 keV states in 82 Br, are found to dominate the low-excitation region below ≈ 2.1 MeV. Above 2.1 MeV a sudden onset of a strong GT fragmentation is observed. The degree of fragmentation resembles a situation found in the neighboring A = 76 system 76 Ge, whereas the observed concentration of strength in the three low-lying states is reminiscent of the heavier neighbors 96 Zr and 100 Mo. The strong GT transition to the 75 keV (1 + ) state makes 82 Se interesting for solar neutrino detection. The 82 Se(ν e ,e - ) 82 Br solar neutrino capture rate in a nonoscillation scenario is therefore evaluated to 668 ± 12(stat) ± 60(sys) SNU, and some of the advantages of using selenium for solar neutrino studies are discussed.

59 ≤ A ≤ 89↗

DOE OSTI2015

The A=96 system in ββ decay

Properties of the single and double beta decays of {sup 96}Zr are discussed. It is argued that the single beta decay can provide important information to the neutrinoless variant of β β decay, as it provides a test of theories aimed at calculating the nuclear matrix elements (NME) for both decays. An experimental extraction of the NME for the single β decay requires a measurement of the decay Q-value and half-life. It is shown that the present Q-value of the {sup 96}Zr single β decay is insufficiently well known and requires a re-measurement, preferentially using high-precision ion traps. We also describe the geochemical method to determine the total half-life of {sup 96}Zr, from which to set a limit on the single β -decay half-life at a level of ≈15 × 10{sup 19}yr. Further, the geochemical analysis will allow setting a limit on a rather exotic quadruple β decay of {sup 96}Zr.

71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSIC↗

DOE OSTI2015

Progress at the TITAN-EBIT

Precision mass measurements of short-lived isotopes provide insight into a wide array of physics, including nuclear structure, nucleosynthesis, and tests of the Standard Model. The precision of Penning trap mass spectrometry (PTMS) measurements is limited by the lifetime of the isotopes of interest, but scales proportionally with their charge state q, making highly charged ions attractive for mass measurements of nuclides far from stability. TITAN, TRIUMF's Ion Trap(s) for Atomic and Nuclear science, is currently the only setup in the world coupling an EBIT to a rare isotope facility for the purpose of PTMS. Charge breeding ions for Penning trap mass spectrometry, however, entails specific set of challenges. To make use of its potential, efficiencies have to be high, breeding times have to be short and the ion energy spread has to be small. An overview of the TITAN facility and charge-breeding program is given, current and future developments are highlighted and some selected results are presented.

74 ATOMIC AND MOLECULAR PHYSICS↗