“…We have calculated the main thermodynamic quantities such as the excess internal energy U Ã ¼ U ex =Nk B T and the reduced pressure P Ã ¼ P 3 =" as a function of density at different temperatures and compared the results with the results of Largo and Solana based on second-order perturbation theory [20], the LR-TW EOS due to Betancourt-Cardenas et al, which is based on first-order perturbation theory, and the MCNVT simulation data taken from the literature [23]. Figure 1 shows the reduced pressure as a function of the density at different reduced temperatures for selected values of l. In general, the agreement for the pressures obtained from the MFA-TW EOS, the computer simulation and the LR-TW EOS is good for all values of l. In the case of l ¼ 2, however, it can be seen that, for low temperatures and high densities, the LR-TW EOS and the Largo and Solana EOS are slightly better than the MFA-TW EOS, but, for low and intermediate densities, there is almost no difference between the results at all temperatures.…”