“…The first measurements were followed by other studies [19][20][21][22][23][24][25][26][27][28][29] carried out by several research groups, which essentially confirmed the initial observation but suggested controversial estimations of the absolute VUCN production rates. This controversy is explained by several factors: (a) measurements of such a kind, involving low-probability effects, require careful control of many systematic effects, which could imitate or hide the VUCN production; (b) the rate of VUCN detection depends strongly on the ranges (windows) of initial and final energies of UCN, which have not been under control in some experiments, (c) as we will see from analyses of the spectra presented in this work, very high energy resolution is needed; it has been provided so far only in the Big Gravitational Spectrometer (BGS) spectrometer [26,29]. Thus, the probability of VUCN production per UCN-wall collision might be largely mis-estimated in other experiments; (d) the VUCN production probability depends strongly on the procedure of a sample (surface) treatment or preparation, as has been demonstrated, for instance, in [26].…”