Formation of neutron stars and black holes.

In summary, the conversation discusses the formation of black holes and neutron stars from large stars, and the question of why stars with more mass than the original black hole can still form one. It is explained that a star's nuclear reactions initially create enough outward pressure to compensate for gravity, but when the star has depleted most of its energy, it may collapse into a white dwarf, neutron star, or black hole depending on its mass. The concept of a neutron star being a star that has collapsed under extreme gravity is also mentioned, and the question of whether a neutron star is essentially a supermassive atomic nucleus is brought up. A resource is provided for further understanding of the topic.
  • #1
LogicalAcid
137
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First of all, I know that that very large stars tend to form black holes, and smaller stars, but still massive in comparison to our sun, tend to form neutron stars. My question is, if matter is lost when a star collapses into a black hole, but can still form one, why is it that it is a star first if it has more mass than the original black hole?
 
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  • #2
LogicalAcid said:
why is it that it is a star first if it has more mass than the original black hole?
During its normal life, the nuclear reactions in the star's core creates outward pressure that compensate the gravity. It is only when the star has radiated most of its energy from nuclear reactions that it has trouble fighting gravity. Depending on its mass at this point, it may collapse to a white dwarf, a neutron star, or a black hole.
 
  • #3
I understand that a neutron star is a star so effected by gravity that the electron shells have been foced into the protons to form neutrons. Presumably these neutrons are packed in tightly together as they have no repulsive charges and are under enormous gravitational pressure. Also, most of an atom is empty space between the nucleus and the electon quanta. If there are no electrons, does that mean that we have effectively a supermassive atomic nucleus? Or is that black hole territory? Or (most likely) I'm missing something!
 
  • #5


This is a great question and one that has been a subject of ongoing research and debate in the scientific community. The formation of neutron stars and black holes is a result of the death of a massive star, known as a supernova explosion.

When a star runs out of fuel, it can no longer sustain the nuclear fusion reactions in its core that keep it stable. This causes the core of the star to collapse under its own gravity, resulting in a supernova explosion. The collapse of the core can continue even after the explosion, leading to the formation of either a neutron star or a black hole.

The main difference between the two is the mass of the original star. Neutron stars typically form from stars with masses between 8 and 20 times that of our sun, while black holes form from stars with masses greater than 20 times that of our sun. This is because the gravitational force of a more massive star is strong enough to overcome the repulsive force of the neutron degeneracy pressure, which is what keeps a neutron star from collapsing further.

So, why does a star first form before collapsing into a black hole if it has more mass? This is because the formation of a black hole is a gradual process. As the star collapses, it becomes more and more dense, and its gravity becomes stronger. At a certain point, the gravity becomes so strong that even light cannot escape its pull, and a black hole is formed.

In contrast, a neutron star is formed when the core of the star collapses to a point where the neutrons are packed so tightly that they resist further collapse. This results in a very dense and compact object, but one that is not dense enough to form a black hole.

In summary, the formation of neutron stars and black holes is a complex process that depends on the mass of the original star and the strength of its gravitational force. While a star may have more mass than a black hole, it is the gradual process of collapse that leads to the formation of these two distinct objects.
 

Related to Formation of neutron stars and black holes.

1. What is the difference between a neutron star and a black hole?

Neutron stars and black holes are both formed from the collapse of a massive star, but they have different properties. A neutron star is a highly dense object made up of tightly packed neutrons, while a black hole is a singularity with infinite density and intense gravitational pull.

2. How are neutron stars and black holes formed?

Neutron stars and black holes are formed when a massive star runs out of fuel and its core collapses under its own gravity. This causes the core to become extremely dense and hot, leading to the formation of either a neutron star or a black hole.

3. What is the role of mass in the formation of neutron stars and black holes?

The mass of a star determines whether it will become a neutron star or a black hole. Stars with masses less than 3 times that of the sun will become neutron stars, while stars with masses greater than 3 times the sun's mass will become black holes.

4. Can neutron stars and black holes be observed?

Neutron stars and black holes cannot be observed directly, as their intense gravitational pull prevents any light from escaping. However, their presence can be detected through their effects on nearby matter, such as X-rays emitted from accretion disks around black holes or pulsating radio waves from neutron stars.

5. Are there any known collisions or mergers of neutron stars and black holes?

Yes, there have been observed collisions and mergers of neutron stars and black holes, which have been detected through gravitational waves. These events are rare and can provide valuable insights into the properties and behavior of these objects.

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