O2scl_eos is sub-library for working with equations of state designed to work with O2scl_part and O2scl . It includes

- Several classes for computing the hadronic and quark equations of state of matter near and above the nuclear saturation density
- Classes to solve the TOV equations of neutron star structure
- One class to perform a rudimentary computation of the structure of closed-shell nuclei in the Hartree approximation.

- Equations of State of Hadronic Matter
- Equations of State of Quark Matter
- Solution of the Tolman-Oppenheimer-Volkov equations
- Cold Neutron Stars
- Rotating Neutron Stars
- Neutron Star Outer Crust
- Nuclear structure in the Hartree approximation
- Finite-temperature Equation of State Tables
- Bibliography
- Bug List
- Todo List
- Other Todos
- Ideas for Future Development

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