WG1: Equation of State of dense matter
WG 1 Leader: Dr. Laura Tolos
Task Leader: Dr. Ian Jones
Task Leader: Dr. Enrico Bozzo
PHAROS will aim at answering how can the neutron star Equation of State (EoS) be investigated with different astrophysical and gravitational observations. Answering this question requires the communities to interact with nuclear physicists to set standard parameters for different EoS species to be implemented in astrophysical and gravitational simulations.
• Collaboration between communities to determine standards.
• Provide benchmarks to test the correct implementation/functioning.
• Provide unified and consistent EoSs.
• Collaboration with WG2 to determine consistent transport parameters.