1937
DOI: 10.1016/s0031-8914(37)80105-6
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Note on the law of sargent

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1939
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Cited by 39 publications
(13 citation statements)
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“…The connection between scattering data and ρ(E) as noticed in [3,8] is briefly repeated here for clarity. While calculating the virial coefficients in the equation of an ideal gas, Beth and Uhlenbeck [9] found that the difference between the density of states (of scattered particles) with the interaction dn l (E)/dE and without dn…”
Section: Density Of Statesmentioning
confidence: 99%
“…The connection between scattering data and ρ(E) as noticed in [3,8] is briefly repeated here for clarity. While calculating the virial coefficients in the equation of an ideal gas, Beth and Uhlenbeck [9] found that the difference between the density of states (of scattered particles) with the interaction dn l (E)/dE and without dn…”
Section: Density Of Statesmentioning
confidence: 99%
“…Beth and Uhlenbeck [33] (the derivation of their result is reproduced in [34], see also [35,36]) found that the difference between the density of states with interaction, n l , and without, n (0) l , is given by the derivative of the scattering phase shift δ l as,…”
Section: Statistical Physics Based Approachmentioning
confidence: 99%
“…For example, for (a/λ) = 2, convergence is obtained only when the sum extends to l max = 33. 4 This may be understood by noting that for small β (high temperature), the damping of the integrand from the Gaussian is less effective, and higher values of the variable k are needed for the convergence. From impact parameter argument [10], the cut-off l max (ka) in the sum over l therefore also increases.…”
Section: Numerical Comparisonmentioning
confidence: 99%
“…For a dilute gas at high temperature, it is the second virial coefficient that gives the dominant contribution. The second virial coefficient may also be calculated quantum mechanically from the Beth-Uhlenbeck formula using the hard-sphere scattering phase shifts in the various partial waves [4]. Contrary to naive expectations, the quantum result for the interaction energy of the Boltzmann gas at high temperatures is substantially different from the classical one, even when the thermal wavelength is only a fraction of the hard-sphere diameter.…”
Section: Introductionmentioning
confidence: 98%