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Nuclear equation of state (EoS) plays an important role in understanding theformation of compact objects such as neutron stars and black holes. The truenature of the EoS has been a matter of debate at any density range not only inthe nuclear physics but also in the astronomy and astrophysics. We haveconstructed a database of EoSs by compiling data from the literature. Ourdatabase contains the basic properties of the nuclear EoS of symmetric nuclearmatter and of pure neutron matter. It also includes the detailed informationabout the theoretical models, for example the adopted methods and assumptionsin individual models. The novelty of the database is to consider newexperimental probes such as the symmetry energy, its slope relative to thebaryon density, and the incompressibility, which enables the users to checktheir model dependences. We demonstrate the performance of the EOSDB throughthe examinations of the model dependence among different nuclear EoSs. It isreveled that some theoretical EoSs, which is commonly used in astrophysics, donot satisfactorily agree with the experimental constraints.

EOSDB: The Database for Nuclear EoS