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Table 1
H-He EOSs used in interior models.
| Name of the H-He EOS | H EOS | He EOS | H-He interactions | Notes/references |
|---|---|---|---|---|
| MGF16+MH13 | MGF16-H | SCvH95-He | Included in the H EOS but fixed at Y = 0.245 | Derived by Miguel et al. (2016) from Militzer & Hubbard (2013) |
| MH13* | -- | -- | -- | Adjusted from MGF16+MH13 to fit a Y = 0.245 adiabat from Militzer et al. (2022) |
| CD21 | CD21-H | CMS19-He | Included in the H EOS but fixed at Y = 0.245 | Derived by Chabrier & Debras (2021) from Militzer & Hubbard (2013) |
| HG23+CMS19 | CMS19-H | CMS19-He | HG23 | H and He EOSs from Chabrier et al. (2019) and non-ideal mixing effects from Howard & Guillot (2023) |
| HG23+MLS22 | MLS22-H | CMS19-He | HG23 | H EOS from Mazevet et al. (2022) and non-ideal mixing effects from Howard & Guillot (2023) |
| SCvH95 | SCvH95-H | SCvH95-He | None | H and He EOSs from Saumon et al. (1995) |
Notes. Concerning the heavy elements, the EOSs used for ices and rocks are respectively those of water and dry sand from Lyon & Johnson (1992).
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