Mass in Schwarzschild's Metric: Exploring Vacuum Solutions

In summary, for the exterior Schwarzschild metric, the parameter M represents the total mass-energy content of the space-time, while the vacuum solution describes the region outside the star. For the interior region, a different metric would be needed to describe the star's mass-energy distribution.
  • #1
ChrisVer
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I think this will be a quick question...
If the Schw's metric is a solution of the vacuum, then what does the mass [itex]M_0[/itex] in the metric correspond to? I thought it was the mass of the star... but if that's true then why is it a vacuum solution?
Or is it vacuum because it describes the regions outside the star of radius [itex]R_{0}[/itex]([itex]r>R_{0},~~ M_0 \equiv M(R_{0}) [/itex]) ?
 
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  • #2
ChrisVer said:
If the Schw's metric is a solution of the vacuum, then what does the mass [itex]M_0[/itex] in the metric correspond to?

For the exterior Schwarzschild metric, the parameter M would technically signify the total mass-energy content of the entire space-time.

but if that's true then why is it a vacuum solution?

Because it describes the exterior vacuum region of the mass-energy distribution, i.e. the region where the energy-momentum tensor vanishes everywhere.
 
  • #3
So would it be wrong to try and describe the interior of the star with a function [itex]M(r)[/itex] instead of [itex]M_{0}[/itex] the total mass?
 
  • #4
ChrisVer said:
So would it be wrong to try and describe the interior of the star with a function [itex]M(r)[/itex] instead of [itex]M_{0}[/itex] the total mass?

Not at all, but the metric won't be the Schwarzschild metric in the interior region. It will, however, have to join smoothly to the Schwarzchilld metric for ##M_0## at the surface.
 
  • #5


The mass M_0 in Schwarzschild's metric corresponds to the mass of the central body, such as a star or a black hole. It is a vacuum solution because it describes the curvature of spacetime in the regions outside of the central body, where there is no matter or energy present. This means that the metric is valid in the vacuum outside of the star or black hole, but it does not account for the mass of the star itself. The vacuum solution is important because it allows us to understand the gravitational effects of the central body on its surroundings, without having to worry about the details of its internal structure. So, while the mass M_0 in the metric may correspond to the mass of the star, the metric itself is describing the vacuum outside of the star.
 

FAQ: Mass in Schwarzschild's Metric: Exploring Vacuum Solutions

What is Schwarzschild's metric?

Schwarzschild's metric is a mathematical description of the spacetime around a spherically symmetric, non-rotating mass, such as a black hole. It was first developed by Karl Schwarzschild in 1916 as a solution to Einstein's field equations in general relativity.

How does mass impact the metric in Schwarzschild's solution?

The mass of the object being studied is the central factor in Schwarzschild's metric. The greater the mass, the more curvature there is in spacetime, leading to stronger gravitational effects. This can be seen in the equation for the metric, where the mass term is directly proportional to the strength of the gravitational field.

What is the significance of exploring vacuum solutions in Schwarzschild's metric?

Exploring vacuum solutions in Schwarzschild's metric allows us to understand the behavior of spacetime in the absence of matter or energy. This is important because it helps us understand how gravity works in empty regions of space, such as around a black hole.

Can Schwarzschild's metric be applied to other objects besides black holes?

Yes, Schwarzschild's metric can be applied to any object that is spherically symmetric and non-rotating. This includes stars and planets, as well as hypothetical objects like cosmic strings or monopoles.

What are some potential implications of studying mass in Schwarzschild's metric?

Studying mass in Schwarzschild's metric can help us to better understand the behavior of gravity in extreme environments, such as near black holes. It can also provide insights into the nature of space and time, and potentially lead to the development of new technologies, such as space travel using gravitational slingshots around massive objects.

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