@Article{Guess_etal2011,
author="Guess, C. J. et al
and Algora, A.
and Estevez, E.
and Molina, F.
and Rubio, B.",
title="The Nd-150(He-3,t) and Sm-150(t,He-3) reactions with applications to beta beta decay of Nd-150",
journal="Physical Review C",
year="2011",
publisher="Amer Physical Soc",
volume="83",
number="6",
pages="064318--17pp",
abstract="The Nd-150(3He,t) reaction at 140 MeV/u and Sm-150(t,He-3) reaction at 115 MeV/u were measured, populating excited states in Pm-150. The transitions studied populate intermediate states of importance for the (neutrinoless) beta beta decay of Nd-150 to Sm-150. 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 beta beta decay (0 nu beta beta) of Nd-150. The present results thus provide useful information on the neutrino responses for evaluating the 0 nu beta beta and 2 nu beta beta matrix elements. The 2 nu beta beta 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 nu beta beta direct counting experiments, and at least several transitions through 1+ intermediate states in Pm-150 are required to explain the 2 nu beta beta half-life. Because Gamow-Teller transitions in the Sm-150(t,3He) experiment are strongly Pauli blocked, the extraction of Gamow-Teller strengths was complicated by the excitation of the 2 (h) over bar omega, Lambda L = 0, Delta S = 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.",
optnote="ISI:000291729400001",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=649), last updated on Fri, 18 Nov 2011 10:22:57 +0000",
issn="0556-2813",
doi="10.1103/PhysRevC.83.064318",
opturl="http://arxiv.org/abs/1105.0677",
opturl="https://doi.org/10.1103/PhysRevC.83.064318",
archivePrefix="arXiv",
eprint="1105.0677",
language="English"
}