WG4: Magnetic field formation, evolution, (in)stability and neutron star population study
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/oscillatio
• Determine systematic differences, verify assumptions and validity in different communities.
• Closer collaboration between observers and theorists to set up observational tests.