O2scl Equations of State¶
O2scl_eos is a sub-library for constructing equations of state of dense matter, computing the structure of rotating and non-rotating neutron stars, and computing the of structure of nuclei in the Hartree approximation. O2scl_eos is part of O2scl.
- Equations of State of Hadronic Matter
- Equations of State of Quark Matter
- Solution of the Tolman-Oppenheimer-Volkov Equations
- Moment of Inertia in the Slowly-Rotating Approximation
- Neutron Star Tidal Deformability
- Cold Neutron Star Structure
- Rotating Neutron Stars
- Neutron Star Outer Crust
- Nuclear structure in the Hartree approximation
- Finite-temperature Equation of State Tables
- Bibliography
- Class List
- Todo List