Searching for debris disks around isolated pulsars

• We review the background for debris disk searches around pulsars.
• We review the results from searches around millisecond pulsars, magnetars, CCOs, and regular pulsars.
• We discuss the results and provide a summary.

Different pieces of observational evidence suggest the existence of disks around isolated neutron stars. Such disks could be formed from supernova fallback when neutron stars are born in core-collapse supernova explosions. Efforts have been made to search for disks around different classes of pulsars, which include millisecond pulsars, young neutron star classes (magnetars, central compact objects, and X-ray dim isolated neutron stars), and regular radio pulsars. We review the main results from observations at wavelengths of from optical to sub-millimeter/millimeter.