Neutron Star or a Pulsar - what decides

In summary, a newly formed neutron star has the potential to become a pulsar if it has a strong magnetic field and is rotating quickly enough. However, over time, the pulsar will slow down as it loses energy. The difference between a neutron star and a pulsar is mainly related to the strength of their magnetic fields. Pulsars are usually young and energetic, while neutron stars can be older and less active. Pulsars also have hotspots on their surface due to accretion of matter, which is controlled by their magnetic fields. Without accretion, a neutron star will not exhibit pulsar behavior.
  • #1
kranav
34
0
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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  • #3
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.
 
  • #4
A pulsar IS a neutron star, usually very young, energetic, and spinning like a top. Its immense magnetic field is what causes the pulses.
 
  • #5
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.
 
  • #6
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.
 

1. What is a neutron star?

A neutron star is an incredibly dense celestial object that is created when a massive star dies in a supernova explosion. The core of the star collapses under its own gravity, and the protons and electrons combine to form neutrons. This results in a star with a diameter of only about 10 kilometers, but with a mass of about 1.4 times that of our sun.

2. How is a neutron star different from other types of stars?

Neutron stars are much denser and smaller than other types of stars. They also have incredibly strong magnetic fields and rotate at very high speeds, which causes them to emit beams of radiation that can be detected on Earth as pulsating signals.

3. What causes a neutron star to become a pulsar?

A pulsar is a type of neutron star that emits beams of radiation in a specific direction as it rotates. This is caused by the strong magnetic field of the neutron star, which interacts with the rapidly spinning star and creates the pulsating signals that can be detected by telescopes on Earth.

4. How do scientists study neutron stars and pulsars?

Scientists use a variety of tools and techniques to study neutron stars and pulsars. This includes using telescopes that can detect different types of radiation, such as X-rays and radio waves. They also use computer simulations and mathematical models to better understand the physics and behavior of these objects.

5. What factors determine the lifespan of a neutron star or pulsar?

The lifespan of a neutron star or pulsar is determined by several factors, including its mass, rotation rate, and magnetic field strength. Neutron stars and pulsars can also be influenced by their environment, such as if they are in a binary system with another star or if they are in a dense region of space with other objects that can affect their rotation and magnetic field.

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