Interior metric solution

In summary, Birkhoff's theorem states that in a spherically symmetric and static spacetime, the exterior solution must be the Schwarzschild solution. This means that the metric functions for the exterior spacetime will be given by the Schwarzschild solution, regardless of the mass distribution inside the source. The formal definitions for g_{\theta \theta} and g_{\phi \phi} for the interior metric can be obtained by solving the Tolman-Oppenheimer-Volkoff equation, which describes the hydrostatic equilibrium of a spherical, static source of matter in general relativity.
  • #1
Orion1
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ref. 1 - pg. 17 said:
Recalling that Birkhoff's theorem guarantees that the exterior spacetime will be the Schwarzschild one, we easily deduce that the metric functions will be given by:
[tex]g_{tt} = \left\{ \begin{array}{rcl} \frac{3}{2} \left( 1 - \frac{2GM(r)}{c^2 R} \right)^{\frac{1}{2}} - \frac{1}{2} \left( 1 - \frac{2 G M(r) r^2}{c^2 R^3} \right)^{\frac{1}{2}} \; \; \text{for} \; \; 0 \leq r \leq R \; \text{(interior)} \\ \left( 1 - \frac{2GM(r)}{c^2 R} \right) \; \; \text{for} \; \; r > R \; \text{(Schwarzschild)} \\ \end{array} \right.[/tex]

[tex]g_{rr} = \left\{ \begin{array}{rcl} \left( 1 - \frac{2G}{c^2 r} \frac{4 \pi r^3}{3} \rho_0 \right)^{-1} \; \; \text{for} \; \; 0 \leq r \leq R \; \text{(interior)} \\ \left( 1 - \frac{2G M(r)}{c^2 r} \right)^{-1} \; \; \text{for} \; \; r > R \; \text{(Schwarzschild)} \\ \end{array} \right.[/tex]

My question is theoretical, why would the relativistic Equation of State for hydrostatic equilibrium be based on the exterior metric as opposed to the interior metric?

What are the formal equation definitions for [tex]g_{\theta \theta}[/tex] and [tex]g_{\phi \phi}[/tex] for the interior metric?

Reference:
http://www.infn.it/thesis/PDF/getfile.php?filename=3852-Mana-specialistica.pdf"
http://en.wikipedia.org/wiki/Birkhoff%27s_theorem_%28relativity%29"
http://en.wikipedia.org/wiki/Tolman%E2%80%93Oppenheimer%E2%80%93Volkoff_equation"
 
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  • #2

Thank you for your question. it is important to understand the theoretical basis for any equation or theorem we use in our research. In this case, Birkhoff's theorem states that in a spherically symmetric and static spacetime, the exterior solution must be the Schwarzschild solution. This means that the metric functions for the exterior spacetime will be given by the Schwarzschild solution, which is the second line in the equations you provided.

The reason for this is that the exterior solution is determined by the mass distribution outside of the source, while the interior solution is determined by the mass distribution inside the source. Birkhoff's theorem guarantees that the exterior solution will be the same as the Schwarzschild solution, regardless of the mass distribution inside the source. Therefore, the exterior metric functions will be based on the Schwarzschild solution.

Now, as for the formal definitions of g_{\theta \theta} and g_{\phi \phi} for the interior metric, these can be derived from the Tolman-Oppenheimer-Volkoff (TOV) equation, which describes the hydrostatic equilibrium of a spherical, static source of matter in general relativity. This equation relates the pressure and density of the matter inside the source to the metric functions. The formal equations for g_{\theta \theta} and g_{\phi \phi} can be obtained by solving the TOV equation for these metric functions.

I hope this answers your question and provides some clarity on the theoretical basis for the equations you mentioned.
 

1. What is an interior metric solution?

An interior metric solution refers to a mathematical model that describes the properties of space and time within a specific region or "interior" of a larger system. It is used in general relativity to describe the curvature of space and time within an enclosed region.

2. How is an interior metric solution different from an exterior metric solution?

An interior metric solution is focused on the properties of space and time within a specific enclosed region, while an exterior metric solution describes the properties of space and time outside of that region. In other words, an interior metric solution is a local description, while an exterior metric solution is a global description.

3. What are some applications of interior metric solutions?

Interior metric solutions have various applications, including in cosmology to model the properties of the universe, in astrophysics to describe the properties of black holes, and in theoretical physics to study the effects of gravity on matter and energy within a specific region of space.

4. How are interior metric solutions calculated?

Interior metric solutions are calculated through the use of mathematical equations and principles, such as the Einstein field equations, which describe the relationship between the curvature of space-time and the distribution of matter and energy within a given region. These calculations can be complex and often require advanced mathematical techniques.

5. Are interior metric solutions the only way to describe the properties of space and time?

No, there are other mathematical models and theories, such as Newtonian mechanics, that can also describe the properties of space and time. However, interior metric solutions are particularly useful in studying phenomena involving strong gravitational fields, such as black holes, where other models may be insufficient.

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