Newtonian limit to schwarschild radial geodesic

In summary, the conversation discusses finding the Newtonian limit to radial geodesic and using the weak field limit to replace d\tau with "t" to recover Newton's Law. However, this approach may not be rigorous and the conversation suggests a more systematic way by rewriting the derivative and considering the Newtonian limit for \frac{dt}{d\tau}=\gamma. There is also a mention of a second order non-linear differential equation that arises from this approach and a request for suggestions.
  • #1
vaibhavtewari
65
0
Hello Everyone,

While trying to find the Newtonian limit to radial geodesic I was able to find that

[tex]\frac{d^2r}{d\tau^2}=\frac{GM}{r^2}[/tex]

In the weak field limit we can naively replace [tex]\tau[/tex] by "t" and recover Newtons Law, this though does not sound very rigorous. Can some-one suggest a much systematic way.

regards,
Vaibhav
 
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  • #2
Rewrite the derivative as

[tex]
\frac{d^2r}{d\tau^2}= \Bigl(\frac{dt}{d\tau}\Bigr)^2 \frac{d^2 r}{dt^2}
[/tex]

and see what the Newtonian limit says about

[tex]
\frac{dt}{d\tau} = \gamma
[/tex]
 
  • #3
Thankyou for replying, I was thinking about that and was writing [tex]\gamma=1-(\frac{dr}{dt})^2[/tex] that leads to a second order non-linear differential equation

[tex]\frac{d^2r}{dt^2}=[1-(\frac{dr}{dt})^2]\frac{Gm}{r^2}[/tex]

any suggestions after this ? What do you think ?
 

What is the Newtonian limit to Schwarzschild radial geodesic?

The Newtonian limit to Schwarzschild radial geodesic refers to the approximation of the motion of a massive object in a static, spherically symmetric gravitational field. It is based on Isaac Newton's law of universal gravitation and is used to describe the motion of objects in the vicinity of a massive body, such as a planet or star.

How is the Newtonian limit to Schwarzschild radial geodesic calculated?

The Newtonian limit to Schwarzschild radial geodesic is calculated using the Schwarzschild metric, which is a solution to Einstein's field equations for a non-rotating, spherically symmetric mass. This metric describes the curvature of spacetime around a massive body and can be used to derive the equations of motion for an object in this gravitational field.

What is the difference between the Newtonian limit and the Schwarzschild limit?

The Newtonian limit is an approximation of the motion of objects in a gravitational field, while the Schwarzschild limit is a specific solution to Einstein's field equations for a non-rotating, spherically symmetric mass. The Newtonian limit is valid for objects moving at low speeds and in weak gravitational fields, while the Schwarzschild limit applies to all speeds and strong gravitational fields.

Can the Newtonian limit to Schwarzschild radial geodesic be applied to all objects?

The Newtonian limit can be applied to any object, as long as its speed is much smaller than the speed of light and the gravitational field is weak. However, the Schwarzschild limit is more accurate and should be used for objects with high speeds or in strong gravitational fields, such as black holes.

Why is the Newtonian limit to Schwarzschild radial geodesic important in physics?

The Newtonian limit to Schwarzschild radial geodesic is important because it provides a simple and accurate way to describe the motion of objects in a gravitational field. It is also the basis for many fundamental concepts in physics, such as the gravitational potential and the escape velocity. Additionally, it helps bridge the gap between classical mechanics and general relativity, providing a link between Newton's laws of motion and Einstein's theory of gravity.

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