Q re de Sitter–Schwarzschild metric

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In summary: Hi Ibix:Since τ is absent from the three equations I am working with, if I cannot used/dτ = c×d/dsTau is not actually absent from these equations. They are omitted, but implied. More on this later.The equations you reference are also derived using the assumption that c=1. This can be inferred from the metric, i.e.$$ds^2 = -f(r) dt^2 + \frac{dr^2}{f(r)} + r^2\,(d\theta^2 + \sin^2 \theta d\phi^2)$$
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It's messy, but my computer algebra package is confirming the solution.

The highlights:
$$g(r) = \frac{df(r)}{dr} \quad \dot{t}(\tau)= \frac{E}{f(r(\tau))} \quad \dot{r}(\tau) = \sqrt{E^2 - f(r(\tau))} $$

$$ \ddot{t}(\tau) = -\frac{E\,g(r)}{f^2(r)} \dot{r}= \frac{-E\, g(r(\tau)) \sqrt{ E^2 - f(r(\tau))} } {f^2(r(\tau))} $$

$$ \ddot{r}(\tau) = -\frac{1}{2} \, \frac{g(r)} { \sqrt{E^2-f(r)}} \dot{r} = -\frac{g(r(\tau)) } {2 }$$

The rest is more algebra, substuting ##\ddot{t}## ##\dot{t}## ##\ddot{r}## and ##\dot{r}## into the geodesic equations.

Note that when g(r)=0, ##\ddot{r}=0##, which is consistent with the idea that f(r) is the effective potential, and the metastable peak of the effective potential occurs when g(r) = df/dr = 0.

From the expression for ##\dot{r}## we could write

$$\frac{dr}{\sqrt{E^2 - f(r)}} = d\tau$$

which could be integrated to solve for ##\tau(r)## which could be inverted to get ##r(\tau)##, but this gets very messy very quickly.
 
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<h2> What is the Q re de Sitter-Schwarzschild metric?</h2><p>The Q re de Sitter-Schwarzschild metric is a mathematical equation that describes the curvature of spacetime around a massive, non-rotating object. It combines elements of the de Sitter metric, which describes the curvature of an empty universe, and the Schwarzschild metric, which describes the curvature of spacetime around a non-rotating spherical mass.</p><h2> How is the Q re de Sitter-Schwarzschild metric derived?</h2><p>The Q re de Sitter-Schwarzschild metric is derived from Einstein's field equations, which relate the curvature of spacetime to the distribution of matter and energy. It is a solution to these equations for a specific scenario: a non-rotating, spherically symmetric mass in an otherwise empty universe.</p><h2> What is the significance of the Q re de Sitter-Schwarzschild metric?</h2><p>The Q re de Sitter-Schwarzschild metric is significant because it is one of the few exact solutions to Einstein's field equations. It is also important in understanding the behavior of light and other objects near massive bodies, such as black holes.</p><h2> How does the Q re de Sitter-Schwarzschild metric differ from the Schwarzschild metric?</h2><p>The Q re de Sitter-Schwarzschild metric differs from the Schwarzschild metric in that it includes an additional parameter, Q, which represents the cosmological constant. This constant describes the overall curvature of the universe and can affect the behavior of spacetime near massive objects.</p><h2> What are some real-world applications of the Q re de Sitter-Schwarzschild metric?</h2><p>The Q re de Sitter-Schwarzschild metric has been used in various fields, including astrophysics, cosmology, and gravitational wave detection. It has also been used in the study of black holes and the behavior of light in their vicinity. Additionally, it has implications for our understanding of the expansion and structure of the universe.</p>

FAQ: Q re de Sitter–Schwarzschild metric

What is the Q re de Sitter-Schwarzschild metric?

The Q re de Sitter-Schwarzschild metric is a mathematical equation that describes the curvature of spacetime around a massive, non-rotating object. It combines elements of the de Sitter metric, which describes the curvature of an empty universe, and the Schwarzschild metric, which describes the curvature of spacetime around a non-rotating spherical mass.

How is the Q re de Sitter-Schwarzschild metric derived?

The Q re de Sitter-Schwarzschild metric is derived from Einstein's field equations, which relate the curvature of spacetime to the distribution of matter and energy. It is a solution to these equations for a specific scenario: a non-rotating, spherically symmetric mass in an otherwise empty universe.

What is the significance of the Q re de Sitter-Schwarzschild metric?

The Q re de Sitter-Schwarzschild metric is significant because it is one of the few exact solutions to Einstein's field equations. It is also important in understanding the behavior of light and other objects near massive bodies, such as black holes.

How does the Q re de Sitter-Schwarzschild metric differ from the Schwarzschild metric?

The Q re de Sitter-Schwarzschild metric differs from the Schwarzschild metric in that it includes an additional parameter, Q, which represents the cosmological constant. This constant describes the overall curvature of the universe and can affect the behavior of spacetime near massive objects.

What are some real-world applications of the Q re de Sitter-Schwarzschild metric?

The Q re de Sitter-Schwarzschild metric has been used in various fields, including astrophysics, cosmology, and gravitational wave detection. It has also been used in the study of black holes and the behavior of light in their vicinity. Additionally, it has implications for our understanding of the expansion and structure of the universe.

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