Density to spherical radius collapse ratio?

In summary: Overall, the spatial area to mass ratio is determined by the strength of the inward force, and whether or not it will lead to a singularity depends on the specific conditions and forces at play. In summary, the combination of protons, neutrons, and electrons can result in different forms of matter, including solids, liquids, and gases. However, under certain conditions, such as a strong enough inward force, it is possible for matter to collapse into a singularity, creating a black hole. The specific ratio of spatial area to mass in this scenario depends on the strength of the inward force and various other factors.
  • #1
LykosPF4
3
0
So in the world of protons, neutrons and electrons, these pieces of matter combine to create what we see around us. Solids, liquids and gases.

What I'm trying to figure out is the spatial area to mass ratio before this general structure of protons, neutrons, and electrons collapses into smaller particles meaning a area of matter/energy that contains no protons neutrons and electrons. Can that happen? Would it be due to gravitational forces?

And generally I'm wondering about a small spherical area and what the metrc radius of the spherical area would be with the mass in kilograms compressed inside it. Would it turn into a singularity? Is there a better way of asking this question? I welcome any thoughts and answers on this subject.

One more note. Supose that the inward force compressing the matter was strong enough to prevent a nuclear explosion. It's not a completely necessary addendum though, so exclude it if needs be.

Thank you.
 
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  • #2
The answer to your question is complicated and depends on the strength of the inward force. If the force is strong enough, then it is possible for a given area of space to contain a mass in kilograms that is compressed into a singularity, otherwise known as a black hole. This is due to the fact that the inward force of gravity at the center of the mass will be greater than the outward force created by the pressure of the particles, leading to an infinite compression of the matter. However, in order for this to happen, the inward force must be extremely strong. If the force is not strong enough, then the particles will just collapse into a smaller area and the matter will not become a singularity.
 
  • #3


The density to spherical radius collapse ratio is a fascinating concept to consider in the world of subatomic particles. As you mentioned, protons, neutrons, and electrons make up the building blocks of matter, and their arrangement and interactions determine the physical properties of the world around us.

To answer your question, it is possible for a small area of matter to collapse into a singularity, where the density becomes infinite and the radius approaches zero. This is known as a black hole, and it is caused by the intense gravitational forces of a massive object.

In terms of the specific ratio between density and spherical radius, it would depend on the mass and composition of the matter in question. The more massive and dense the object, the smaller its radius would need to be in order to collapse into a singularity.

It is important to note that this scenario would require an immense amount of energy and conditions that are not typically found in our universe. As you mentioned, the inward force compressing the matter would need to be strong enough to prevent a nuclear explosion, which is a challenging feat to achieve.

Overall, the concept of density to spherical radius collapse ratio is a thought-provoking one, and there is still much to be discovered and understood about the behavior of subatomic particles and the nature of the universe. Thank you for bringing up this interesting topic.
 

Related to Density to spherical radius collapse ratio?

1. What is "Density to spherical radius collapse ratio"?

"Density to spherical radius collapse ratio" is a term used in astrophysics to describe the relationship between the density of matter and the radius of a collapsing spherical object, such as a star or a galaxy. It is a measure of how tightly packed the matter is within a given volume.

2. How is the "Density to spherical radius collapse ratio" calculated?

The "Density to spherical radius collapse ratio" is calculated by dividing the density of the object by the square of its radius. This ratio is used to determine the critical density at which an object will collapse under its own gravity.

3. What factors affect the "Density to spherical radius collapse ratio"?

The "Density to spherical radius collapse ratio" is affected by the mass and size of the object, as well as the type of matter it is composed of. For example, a more massive object with the same density as a smaller object will have a higher collapse ratio.

4. Why is the "Density to spherical radius collapse ratio" important in astrophysics?

The "Density to spherical radius collapse ratio" is important because it helps us understand how objects in the universe form and evolve. It is also a key factor in determining whether an object will form a stable structure, such as a star or a galaxy, or if it will collapse into a black hole.

5. How does the "Density to spherical radius collapse ratio" relate to the formation of stars and galaxies?

The "Density to spherical radius collapse ratio" is crucial in the formation of stars and galaxies. If the collapse ratio is below a certain threshold, the object will not have enough gravity to overcome the pressure of its own hot gases and will not form a star. On the other hand, if the collapse ratio is too high, the object will collapse into a black hole instead of forming a stable structure like a galaxy.

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