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These values were estimated by plotting, as a function of r, the quantities Fn (β) and Gn (α), which are implied in the calculation of the nth -order anisotropic and isotropic moments [38,39]. We thus observed that Fn and Gn, n=0,2,4,6, get a zero value below 4, 4.5, and 5 bohr for (Ne) 2, Ne-Ar, and (Ar) 2, respectively. As moments are not seen to be affected by separations below those bounds, spectra are not expected to be affected either
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These values were estimated by plotting, as a function of r, the quantities Fn (β) and Gn (α), which are implied in the calculation of the nth -order anisotropic and isotropic moments [38,39]. We thus observed that Fn and Gn, n=0,2,4,6, get a zero value below 4, 4.5, and 5 bohr for (Ne) 2, Ne-Ar, and (Ar) 2, respectively. As moments are not seen to be affected by separations below those bounds, spectra are not expected to be affected either.
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68949128485
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In practice, this combination was slightly corrected in order to account for the aperture of the scattering angle [41]
-
In practice, this combination was slightly corrected in order to account for the aperture of the scattering angle [41].
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42
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68949117404
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Since signals by pairs of unlike atoms scale with density as ρa ρb whereas signals by pairs of like atoms scale as ρa2/2!, the factor 14/45 in Eq. (4) of Ref. should be halved
-
Since signals by pairs of unlike atoms scale with density as ρa ρb whereas signals by pairs of like atoms scale as ρa2 /2!, the factor 14/45 in Eq. (4) of Ref. should be halved.
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48
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68949087925
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To that purpose, use was made of the formula BK (0), α2 =2π N2 M0 / (405 kB T) (CGS), which describes the major contribution to the static Kerr second virial coefficient component [27]; N is Avogadro's number
-
To that purpose, use was made of the formula BK (0), α2 =2π N2 M0 / (405 kB T) (CGS), which describes the major contribution to the static Kerr second virial coefficient component [27]; N is Avogadro's number.
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