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Fig. 6

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Jupiter interior profiles obtained with various versions of the EOS adjusted at low and high densities and a helium mass fraction YHe = 0.245. (a) Comparison with previous ab initio predictions of Militzer & Hubbard (2013), Nettelmann et al. (2012), and Chabrier et al. (2019). (b) Comparison with the predictions of Miguel et al. (2016) corrected by Miguel et al. (2018). The shaded area corresponds to the result obtained when d0 is varied as indicated in (a).

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