Microscopic calculation of the β- decays of 151Sm, 171Tm, and 210Pb with implications to detection of the cosmic neutrino background
Abstract
The electron spectral shapes corresponding to the low-Q β--decay transitions 151Sm(5/2- g.s.)\,151Eu(5/2+ g.s.), 151Sm(5/2- g.s.)\,151Eu(7/2+1), 171Tm(1/2+ g.s.)\,171Yb(1/2- g.s.), 171Tm(1/2+ g.s.)\,171Yb(3/2-1), 210Pb(0+ g.s.)\,210Bi(1- g.s.), and 210Pb(0+ g.s.)\,210Bi(0-1) have been computed using beta-decay theory with several refinements for these first-forbidden nonunique (ff-nu) β- transitions. These ff-nu β- transitions have non-trivial electron spectral shapes with transition nuclear matrix elements (NMEs) computed by using the microscopic Interacting Boson-Fermion Model (IBFM-2) for the decays of 151Sm and 171Tm, and the nuclear shell model (NSM) for the decay of 210Pb. Within the respective Q windows, the computed ff-nu electron spectral shapes deviate maximally at sub-percent level from the universal allowed shape, except for the transition 210Pb(0+ g.s.)\,210Bi(1- g.s.), where the maximal deviation is some 2.7\%. This confirms that the so-called approximation is fairly good for most of these low-Q β- transitions and thus the allowed shape is a rather good first approximation. Our computed spectral shapes could be of interest for experiments aiming to measure the cosmic neutrino background (C), like the PTOLEMY experiment. We have also derived C cross sections for the ground-state transitions of the considered nuclei at the β endpoint. Our findings indicate that more work on the atomic mismatch correction is needed in the future in order to extract reliable and precise C cross sections for any nuclear target.
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