Do All Masses Exhibit Schwarzschild Singularities?

In summary, the Schwarzschild solution has two singularities: one at r=0 and one at r=2M. However, not all masses have these singularities, as for the Earth, the actual radius is much greater than 2M and the Schwarzschild metric only describes the field outside the matter. The singularity at r=0 is only present in the case of a black hole, and the singularity at r=2M can be transformed away with a change of coordinates.
  • #1
supakorn
11
0
From the Schwarzschild solution.This solution has two singularities,one at r = 0 and one at r = 2M.I have a questions
1.Every Mass has these singularities ?
2.For singularity at r = 0 it is the center of mass ?
thank you
 
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  • #2
1. No mass has these singularities. If the mass were to contract inside the r=2M boundary, a black-hole is formed ( it is postulated), in which case there is a singularity at r=0. The apparent one at r=2M may be transformed away with a change of coordinates. In the case of the Earth, say, the actual radius is much greater than 2M and the Schwarzschild metric describes the field outside the matter.

2. The interior Schwarzschild metric describes the field inside the matter, and it does not have a singularity a r=0.
 
  • #3


1. Yes, according to the Schwarzschild solution, every mass has both singularities at r=0 and r=2M. This is because the solution is derived from the general theory of relativity, which applies to all masses and objects in the universe.

2. The singularity at r=0 is known as the "central singularity" and is often interpreted as the center of mass for a non-rotating and non-charged black hole. However, it is important to note that the Schwarzschild solution is a mathematical model and does not necessarily represent a physical object. So while the singularity at r=0 can be interpreted as the center of mass, it is not a physical point in space.
 

Related to Do All Masses Exhibit Schwarzschild Singularities?

What is the Schwarzschild Solution?

The Schwarzschild Solution is a mathematical solution to Einstein's field equations in general relativity, which describes the gravitational field outside of a non-rotating, spherically symmetric mass. It is named after Karl Schwarzschild, who first derived the solution in 1916.

What does the solution tell us about black holes?

The Schwarzschild Solution predicts the existence of an event horizon, a boundary beyond which nothing, not even light, can escape the gravitational pull of the mass. This is a key characteristic of black holes, and the Schwarzschild radius is used to calculate the size of the event horizon for a given mass.

How does the Schwarzschild Solution relate to the bending of light?

According to the Schwarzschild Solution, the mass of an object causes the fabric of space-time to curve. This curvature can deflect the path of light, similar to how a lens bends light. This phenomenon is known as gravitational lensing and is one of the key pieces of evidence for the existence of black holes.

Is the Schwarzschild Solution a perfect description of reality?

While the Schwarzschild Solution is a useful tool for describing gravity near a non-rotating, spherically symmetric mass, it does not take into account the effects of rotation, electric charge, or quantum mechanics. Therefore, it is not a complete description of reality, but it is a good approximation in many cases.

How does the Schwarzschild Solution impact our understanding of the universe?

The Schwarzschild Solution, along with other solutions to Einstein's field equations, has greatly expanded our understanding of gravity and its effects on the universe. It has also led to the prediction and discovery of black holes, which have played a crucial role in our understanding of the nature of space, time, and matter.

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