WG 4 Leader: Dr. Pablo Cerda’ Duran 

Task Leader: Dr. Marica Branchesi 

Task Leader: Dr. Michela Mapelli 


PHAROS will aim at answering how does the magnetic field evolve in isolated and accreting systems, how do turbulence and instabilities affect field formation and evolution and how does this affect the neutron star populations that we observe today.



• Compare different magnetic evolution/formation/oscillations codes.

• Determine systematic differences, verify assumptions and validity in different communities.

• Closer collaboration between observers and theorists to set up observational tests.


Participants: TBD