Answers are grounded in this paper and cite their sources.
For a dense gas equilibrium mixture of 65 at.% He and 35 at.% Ne at T=39.3 K and p=114 bar, we determine from neutron scattering the total dynamic structure factor S(k,{ω}) as a function of frequency {ω} for wave numbers 4k28 nm^-1. For all k, S(k,{ω}) is a sum of four Lorentzians; two located at {ω}=±{}ωₛ⁽¹⁾(k) (directly visible for smaller k) and two located at {ω}=±{}ωₛ⁽²⁾(k) (not visible). ωₛ⁽¹⁾(k)>ck can be attributed to fast oscillations of the light He particles (fast sound) and ωₛ⁽²⁾(k)ck to slow oscillations of the heavy Ne particles (slow sound), where c is the hydrodynamic (k{→}0) sound velocity of the total mixture. ωₛ⁽¹⁾(k) is virtually indistinguishable from the (extended) sound dispersion measured in pure helium at T=39.3 K and p=114 bar. A kinetic model, consistent with our experiment, predicts that fast sound vanishes at k=0.7 nm^-1 and that slow sound merges into hydrodynamic sound then.
No takes yet. Share an insight, caveat, or question.
Westerhuijs et al. (1992) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: