Isn't most of that mass blown off an ordinary star, not from a neutron star?
When massive stars that are 8 to 15 times the mass of our sun eventually run out of H and collapse, the gravitational pressure becomes so tremendous that the protons and electrons fuse together into neutrons. At some point there’s an implosion that flashes back and outward: a supernova. The super-hot compacted core is what remains. It’s a mass about equivalent to our sun, that’s “squeezed down” to only miles in diameter. So most of this (formerly) large star’s mass is blown out into space.
I don’t know what percent of an “ordinary” star’s mass blows out into space when it explodes and leaves a white dwarf behind. But since it’s a much smaller amount of matter to start with…
If I remember right, supernovas are estimated at about one per 50 years in our galaxy, and that could be about thirty supernovae per second universally.