WG 2 Leader: Dr. Patrick Weltrevede 

Task Leader: Dr. Danai Antonopoulou 

Task Leader: Dr. Constança Providencia 


PHAROS will aim at answering how can transport phenomena in neutron stars be modelled after or during their formation, also accounting for superfluidity and superconductivity, consistently with the EoS.



• Determine micro-physical inputs for glitch and gravitational wave modeling.

• Provide consistent transport coefficients and superfluid gaps for EoSs from WG1.

• Provide fitting formulae for numerical use.

• Determine standards for glitch observables, in preparation for SKA data.


Participants: TBD