2011/05/03 by C. J. Guess, T. Adachi, H. Akimune +47 · 2 citations
Physics and Astronomy · #Atomic physics #Excited state #Multipole expansion #Neutrino #Neutrino Physics Research #Nuclear physics #Nuclear physics research studies #Particle physics theoretical and experimental studies #Physics #Quantum mechanics #nucl-ex #nucl-th
paper · pdf · doi:10.1103/physrevc.83.064318
18 pages, 13 figures, 2 tables
arxiv created 2011/05/03 · openalex publication_date 2011/06/17 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The 150Nd(3He,t) reaction at 140 MeV/u and 150Sm(t,3He) reaction at 115 MeV/u were measured, populating excited states in 150Pm. The transitions studied populate intermediate states of importance for the (neutrinoless) \ensuremathβ\ensuremathβ decay of 150Nd to 150Sm. Monopole and dipole contributions to the measured excitation-energy spectra were extracted by using multipole decomposition analyses. The experimental results were compared with theoretical calculations obtained within the framework of the quasiparticle random-phase approximation, which is one of the main methods employed for estimating the half-life of the neutrinoless \ensuremathβ\ensuremathβ decay (0\ensuremathν\ensuremathβ\ensuremathβ) of 150Nd. The present results thus provide useful information on the neutrino responses for evaluating the 0\ensuremathν\ensuremathβ\ensuremathβ and 2\ensuremathν\ensuremathβ\ensuremathβ matrix elements. The 2\ensuremathν\ensuremathβ\ensuremathβ matrix element calculated from the Gamow-Teller transitions through the lowest 1+ state in the intermediate nucleus is maximally about half that deduced from the half-life measured in 2\ensuremathν\ensuremathβ\ensuremathβ direct counting experiments, and at least several transitions through 1+ intermediate states in 150Pm are required to explain the 2\ensuremathν\ensuremathβ\ensuremathβ half-life. Because Gamow-Teller transitions in the 150Sm(t,3He) experiment are strongly Pauli blocked, the extraction of Gamow-Teller strengths was complicated by the excitation of the 2\ensuremathℏ\ensuremathω, \ensuremathΔL=0, \ensuremathΔS=1 isovector spin-flip giant monopole resonance (IVSGMR). However, the near absence of Gamow-Teller transition strength made it possible to cleanly identify this resonance, and the strength observed is consistent with the full exhaustion of the non-energy-weighted sum rule for the IVSGMR.