The evolution of magnetic field and spin‐down of young pulsars

Here, we summarize our recent work on the evolution of magnetic field and spin-down of young pulsars including high-B pulsars and magnetars. Our work includes the following three parts: (a) Based on the estimated ages of their potentially associated supernova remnants (SNRs), we estimate the values of the mean braking indices of eight magnetars with SNRs and find that fivemagnetars have smallermean braking indices of 1

Keywords:

• Magnetic field
• Astrophysics
• Pulsar
• Physics
• Spin-½
• Astronomy

• Correction
• Source
• Cite
• Save
• Machine Reading By IdeaReader