Neutron Star or a Pulsar - what decides

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The formation of a neutron star or a pulsar is determined by the core's conditions after a supernova explosion. A neutron star becomes a pulsar if it rotates rapidly and possesses a strong magnetic field. Over time, pulsars slow down as they emit electromagnetic energy, eventually losing their pulsar status. The distinction between a neutron star and a pulsar lies in the presence of a strong magnetic field and the star's rotation speed. If a neutron star lacks surrounding matter to accrete, it will not exhibit pulsar characteristics.
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After a supernova what compels the left over core to be either a neutron star or a pulsar?
is it decided before or after explosion?
any thoughts would be appreciated.
 
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Whenever a type 1A supernovae releases it's remnants, if the left over rigid core doesn't exceed TOV limit then in that case a neutron star is formed. I suppose the difference between a neutron star and a pulsar would be on the scale of sizes of the magnetic field as hinted by jimmy's post.
 
A pulsar IS a neutron star, usually very young, energetic, and spinning like a top. Its immense magnetic field is what causes the pulses.
 
Chronos said:
A pulsar IS a neutron star, usually very young, energetic, and spinning like a top. Its immense magnetic field is what causes the pulses.
Ah, I was under the impression that pulsars are old, neutron stars with high angular momentum. Thanks for your correction.
 
Pulsars accrete surrounding matter onto their surface. The strong magnetic field of the neutron star funnels the matter onto the poles of the star, and bright hotspots are created on the surface. If a neutron star has nothing to accrete, there are no hotspots, and there is no pulsar.
 
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