Four-Velocity and Schwartzchild Metric

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SUMMARY

The discussion focuses on the calculation of the four-velocity of a stationary observer within the context of the Schwarzschild metric in general relativity. The Schwarzschild metric is defined by the equation d{s^2} = {c^2}\left( {1 - \frac{{2\mu }}{r}} \right)d{t^2} - {\left( {1 - \frac{{2\mu }}{r}} \right)^{ - 1}}d{r^2} - {r^2}d{\theta ^2} - {r^2}{\sin ^2}\theta d{\phi ^2}. The four-velocity is derived as u = ({{\left( {1 - \frac{{2\mu }}{r}} \right)}^{ - 1/2}}, 0, 0, 0), confirming that u² = c² in the rest frame of the observer. This conclusion is supported by the calculations presented, demonstrating the relationship between the metric components and the four-velocity.

PREREQUISITES
  • Understanding of the Schwarzschild metric in general relativity
  • Familiarity with four-velocity concepts in physics
  • Basic knowledge of tensor calculus
  • Proficiency in manipulating equations involving spacetime intervals
NEXT STEPS
  • Study the derivation of the Schwarzschild metric in detail
  • Learn about the implications of four-velocity in curved spacetime
  • Explore the concept of geodesics in general relativity
  • Investigate the relationship between four-velocity and energy-momentum in relativistic physics
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Students and researchers in physics, particularly those focusing on general relativity, cosmology, and theoretical physics, will benefit from this discussion.

DRose87
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Homework Statement


What is the Schwartzchild metric. Calculus the 4-velocity of a stationary observer in this spacetime (u). Show that u2 = c2.

Homework Equations


Schwartzchild Metric
d{s^2} = {c^2}\left( {1 - \frac{{2\mu }}{r}} \right)d{t^2} - {\left( {1 - \frac{{2\mu }}{r}} \right)^{ - 1}}d{r^2} - {r^2}d{\theta ^2} - {r^2}{\sin ^2}\theta d{\phi ^2}

The Attempt at a Solution


I already turned this in... I just want to make sure I understand this properly. I'm pretty sure that \mathbf{u}\cdot\mathbf{u} is always equal to c^2 in the rest frame of a particle... So I think the point of the problem is to figure out the components of the four-velocity based on this fact. So here is my attempt at a solution... how ever I actually arrived at the solution in going from the bottom to the top.

So here's how I attempted to solve it:
From the Schwartzchild metric:
g_{00} = c^2\left(1 - \frac{2\mu }{r}\right)

The four-velocity u of a stationary observer is given by:
<br /> \begin{gathered}<br /> \left[ {{u^\mu }} \right] = \left( {{{\left( {1 - \frac{{2\mu }}{r}} \right)}^{ - 1/2}},0,0,0} \right) \hfill \\<br /> {c^2}\left( {1 - \frac{{2\mu }}{r}} \right){\left[ {{{\left( {1 - \frac{{2\mu }}{r}} \right)}^{ - 1/2}}} \right]^2} = {c^2} \hfill \\<br /> \hfill \\<br /> \end{gathered}

It follows that:
{\mathbf{u}} \cdot {\mathbf{u}} = {g_{ab}}{u^a}{u^b} = {g_{00}}{\left( {{u^0}} \right)^2} = {c^2}\left( {1 - \frac{{2\mu }}{r}} \right){\left[ {{{\left( {1 - \frac{{2\mu }}{r}} \right)}^{ - 1/2}}} \right]^2} = {c^2}
 
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Looks fine to me.
 

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