General Relativity: Particle velocity travelling on Schwarzchild orbit

In summary, the speed of a particle in the smallest possible circular orbit in the Schwarzschild geometry as measured by a stationary observer at that orbit can be calculated using the normalization condition and the Schwarzschild metric. The relation mentioned in your question allows us to relate the speed of the particle as measured by the observer to the observer's four-velocity. And the reason we can write u_{a}u_{b} * u^{a}u^{b} = (u^{a}u_{a})^{2} is because the four-velocity is a four-vector.
  • #1
stongio
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Homework Statement



What is the speed of a particle in the smallest possible circular orbit in the Schwarzschild
geometry as measured by a stationary observer at that orbit? Note: The orbit in
question happens to be unstable.


Homework Equations



Normalization condition:

[itex]\textbf{u}_{obs}(r)[/itex][itex]\cdot[/itex][itex]\textbf{u}_{obs}(r)[/itex]=[itex]g_{αβ}[/itex][itex]u^{α}_{obs}(r)[/itex][itex]u^{β}_{obs}(r)[/itex]=-1

Schwarzschild Metric...


The Attempt at a Solution



So from the Normalization condition and the Schwarzschild metric it is easy to find the four-velocity of the observer, because the spatial components are zero. My question relates to the observer's measurement of the particle's velocity. If his four-velocity is
[itex]{u}^{a}[/itex]=[1/[itex]\sqrt{1-2m/r}[/itex],0,0,0]
then, how does observe the particle's velocity?
An answer I found somewhere said

[itex]\frac{u^{2}}{1-u^{2}}[/itex]=[itex]u^{a}u^{b}(g_{ab}+u_{a}u_{b})=(u^{a}u_{a})^{2}-1[/itex]

But I have no idea how to arrive at this relation, and why it relates to the observer's measurement of the particle. Is it possibly a derivation of a relation between t and the proper time?

Also, this might seem very rudimentary but I am not sure why we are able to write:

[itex]u_{a}u_{b} \ast u^{a}u^{b} = (u^{a}u_{a})^{2}[/itex]

I'm very new to general relativity, and would really appreciate the help!
Thanks a lot!
 
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  • #2




Thank you for your question. The speed of a particle in the smallest possible circular orbit in the Schwarzschild geometry, as measured by a stationary observer at that orbit, can be calculated using the normalization condition and the Schwarzschild metric. The normalization condition allows us to find the four-velocity of the observer, which is necessary to calculate the particle's speed.

To find the particle's speed, we can use the relation you mentioned, which is derived from the normalization condition and the Schwarzschild metric. This relation, also known as the Lorentz factor, relates the speed of the particle as measured by the observer to the observer's four-velocity. This is why it is used to calculate the particle's speed as measured by the observer.

As for your question about why we can write u_{a}u_{b} * u^{a}u^{b} = (u^{a}u_{a})^{2}, this is due to the fact that the four-velocity is a four-vector, which means it has both a magnitude and direction. When we multiply two four-vectors together, the result is a scalar quantity (a number), not a vector. Therefore, (u^{a}u_{a})^{2} is the magnitude squared of the four-velocity, which is equivalent to the product of the four-velocity with itself.

I hope this helps clarify your doubts. Keep exploring and asking questions about general relativity, it's a fascinating field!
 

FAQ: General Relativity: Particle velocity travelling on Schwarzchild orbit

1. What is general relativity?

General relativity is a theory of gravity developed by Albert Einstein in the early 20th century. It describes how massive objects, like planets, stars, and galaxies, interact with each other in the presence of gravity. It is a fundamental theory in modern physics and has been extensively tested and confirmed through various experiments and observations.

2. What is the Schwarzchild orbit?

The Schwarzchild orbit is a trajectory followed by a particle in the gravitational field of a non-rotating, spherically symmetric mass. It is named after the German physicist Karl Schwarzchild, who first derived the equations describing this orbit in the context of general relativity. This orbit is important in understanding the behavior of particles near massive objects, such as black holes.

3. How does general relativity explain particle velocity on a Schwarzchild orbit?

According to general relativity, massive objects warp the fabric of spacetime, causing objects to follow curved paths in the presence of gravity. In the case of a Schwarzchild orbit, the massive object at the center causes the path of the particle to curve in a specific way, resulting in a stable orbit. The velocity of the particle on this orbit is determined by the balance between the gravitational force pulling the particle towards the center and the centrifugal force pushing it away.

4. Is the particle velocity on a Schwarzchild orbit constant?

Yes, the particle velocity on a Schwarzchild orbit is constant. This is because the gravitational force and the centrifugal force are balanced at all points on the orbit, resulting in a stable velocity. However, this velocity may change if there are other external forces acting on the particle, such as friction or drag.

5. Can general relativity be applied to other orbits?

Yes, general relativity can be applied to any orbit in which gravity plays a significant role. This includes orbits around planets, stars, and even galaxies. However, the equations may become more complex for more massive or non-spherically symmetric objects, making it difficult to find exact solutions. In these cases, approximations and numerical methods are often used to study the behavior of particles on these orbits.

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