The α-decay rates for the nuclides 168,170,171,172,173,174,176Yb
and 148,150,152,154Gd have been estimated from transmission probabilities
in a systematic α-nucleus potential and from an improved fit to
α-decay rates in the rare-earth mass region. Whereas α-decay of
152Gd in natural gadolinium is a severe obstacle for the use of gadolinium
as a low-energy solar-neutrino detector, we show that
α-decay does not contribute significantly to the background in a
ytterbium detector. An extremely long α-decay lifetime of 168Yb
is obtained from calculation, which may be close to the sensitivity limit in a
low-background solar neutrino detector.Comment: 12 pages, 1 figure; An author name was correcte