2018
DOI: 10.48550/arxiv.1802.06277
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Neutron lifetime, dark matter and search for sterile neutrino

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Cited by 11 publications
(25 citation statements)
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“…This case has been already pointed to by Fornal and Grinstein [3]. The neutron separation energy in 11 Li of S n = 396 (13) keV is favorite for the search of the dark decay producing the unbound 10 Li which would promptly decay to 9 Li by emission of a neutron. So in fact the allowed energy window for the dark decay in this case is given by the two-neutron separation energy equal to 369.3 (6) keV.…”
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confidence: 54%
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“…This case has been already pointed to by Fornal and Grinstein [3]. The neutron separation energy in 11 Li of S n = 396 (13) keV is favorite for the search of the dark decay producing the unbound 10 Li which would promptly decay to 9 Li by emission of a neutron. So in fact the allowed energy window for the dark decay in this case is given by the two-neutron separation energy equal to 369.3 (6) keV.…”
mentioning
confidence: 54%
“…So in fact the allowed energy window for the dark decay in this case is given by the two-neutron separation energy equal to 369.3 (6) keV. However, the short half-life of 11 Li, T 1/2 = 8.75 ms, yields the branching ratio B X = 1.3 × 10 −7 . Unfortunately, this value is by three orders of magnitude smaller than the branching ratio for the β-delayed deuteron emission from 11 Li, B d = 1.30(13) × 10 −4 [7], which leads to the same final nucleus 9 Li.…”
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confidence: 89%
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