Coordinate Change & Gravity: A Schwazschild Metric Analysis

In summary: So yes, you're right.In summary, the Schwarzschild metric is a one parameter family of solutions obtained by setting spherical symmetry in the metric and solving the field equation in vacuum. When the parameter M is set to zero, it becomes the Minkowski solution. The flat metric is also a solution when the boundary condition is chosen as empty space everywhere, but it does not induce gravity as there is no curvature. The Schwarzschild spacetime is another solution that represents a spherically symmetric mass distribution. Different choices for the distribution of stress energy will yield different spacetimes, but the gravitational effects will remain the same regardless of the chosen coordinates.
  • #1
jk22
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What I understood is that The Schwazschild metric is obtained by setting spherical symmetry in the metric and solves the field equation in vacuum.

But is the flat metric a solution too, or does it mean that changing the coordinates induces gravity ?
 
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  • #2
The Schwarzschild solution is not a single solution. It is in fact a one parameter family of solutions. If the parameter M is zero you get the Minkowski solution.
 
  • #3
jk22 said:
But is the flat metric a solution too, or does it mean that changing the coordinates induces gravity ?
If you set M to 0 then you get a flat metric. All of the curvature goes to zero. So there is no gravity induced, it is just spherical coordinates in flat spacetime.
 
  • #4
jk22 said:
But is the flat metric a solution too, or does it mean that changing the coordinates induces gravity ?
The Einstein field equations are differential equations, so they have multiple solutions depending on the boundary conditions that we choose. The solution will be a metric tensor that solves the field equations consistent with the particular boundary conditions we've chosen; it determines a particular spacetime geometry.

Flat spacetime is the geometry we get when we choose empty space everywhere as the boundary condition. We can write this solution in many different coordinate systems; for example Minkowski ##ds^2=-dt^2+dx^2+dy^2+dz^2## and polar ##ds^2=-dt^2+dr^2+r^2(d\theta^2+\sin^2\theta{d}\phi^2)## are two different ways of writing the metric tensor for flat spacetime. No matter what coordinates we choose, the curvature tensors will come out zero, there will be no gravity.

Schwarzschild spacetime is another geometry, the one we get when we choose a spherically symmetric mass distribution as the solution. Again, we can write the metric tensor for that spacetime in many different coordinate systems: Schwarzschild coordinates (of course, and it is unfortunate that we use his name both for the spacetime he discovered and for the coordinates he used to describe it - they're different things), or Kruskal, or Painleve, or ... but no matter which we choose, the gravitational effects calculated from the curvature tensors will be the same.

Other choices for the distribution of stress energy yield yet other spacetimes. Again, the gravitational effects in different spacetimes will be different, but they won't change with our choice of coordinates.
 
  • #5
Nugatory said:
Flat spacetime is the geometry we get when we choose empty space everywhere as the boundary condition.
Am I missing something? I would interpret "empty space everywhere" to mean that you are looking for vacuum solutions. But flat space-time is not the only vacuum solution.
 
  • #6
jbriggs444 said:
Am I missing something? I would interpret "empty space everywhere" to mean that you are looking for vacuum solutions. But flat space-time is not the only vacuum solution.
Not missing anything, I'm just being a bit careless about the wording around a non-critical point.
 
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Related to Coordinate Change & Gravity: A Schwazschild Metric Analysis

1. What is a Schwazschild metric analysis?

A Schwazschild metric analysis is a mathematical model that describes the curvature of space-time around a non-rotating, spherically symmetric mass, such as a black hole. It is based on the work of German physicist Karl Schwarzschild and is an important tool for understanding the effects of gravity on objects in space.

2. How does coordinate change affect gravity?

Coordinate change refers to a shift in the reference frame used to describe the position and movement of objects. In the context of gravity, coordinate change can affect the perceived strength and direction of gravitational forces. This is because gravity is described by the curvature of space-time, which can appear different depending on the chosen reference frame.

3. What is the significance of the Schwazschild radius?

The Schwazschild radius is a characteristic distance from the center of a massive object at which the escape velocity equals the speed of light. This radius is important because it marks the boundary of the event horizon of a black hole, beyond which not even light can escape. It is also used in the calculation of the Schwarzschild metric.

4. How does the Schwazschild metric differ from other metrics?

The Schwazschild metric is a solution to Einstein's field equations that describes the curvature of space-time around a non-rotating, spherically symmetric mass. It is different from other metrics, such as the Kerr metric, which is used to describe the curvature of space-time around a rotating mass. The Schwazschild metric is also unique in that it is the only metric that describes the geometry of a non-rotating black hole.

5. What are some practical applications of Schwazschild metric analysis?

Schwazschild metric analysis has many practical applications in astrophysics, including the study of black holes, gravitational lensing, and the motion of objects in strong gravitational fields. It is also used in the field of general relativity to better understand the effects of gravity on the universe and to make accurate predictions about the behavior of objects in space.

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