Derivation of Geodesics Eq from EM Tensor of Point Particle

In summary, we have discussed the energy-momentum tensor of a free particle with mass ##m## moving along its worldline ##x^\mu(\tau)##, which is given by an integral expression (2). We have also looked at the covariant derivative of a tensor and derived the geodesics equation from the energy-momentum tensor of a point particle in General Relativity, which is given by the equation ##\nabla_{\mu} T^{\mu\nu} = 0##. We have explored the integration by parts technique and discussed how the term ##uv=\dot{x}^{\nu}\delta^{(4)}(y-x(\tau))## disappears after integration by parts. We have also mentioned
  • #1
sergiokapone
302
17
The energy-momentum tensor of a free particle with mass ##m## moving along its worldline ##x^\mu (\tau )## is
\begin{equation}
T^{\mu\nu}(y^\sigma)=m\int d \tau \frac{\delta^{(4) }(y^\sigma-x^\sigma(\tau ))}{\sqrt{-g}}\frac{dx^\mu}{d\tau}\frac{dx^\nu}{d\tau}.\tag{2}
\end{equation}
The covariant derivative of tensor gives
\begin{equation}
\nabla_{\mu} T^{\mu\nu} = \frac{1}{\sqrt{-g}} \frac{\partial \left( \sqrt{-g} T^{\mu\nu}\right) }{\partial y^{\mu}} + \Gamma^{\nu}_{\mu\lambda}T^{\mu\lambda}
\end{equation}

And a derivation of geodesics equation from energy-momentum tensor of point particle in GR ##\nabla_{\mu} T^{\mu\nu} = 0## looks like:

\begin{align}

0 &~~~~~~=~ \frac{1}{\sqrt{-g(y)}}\partial^{(y)}_{\mu} \left(\sqrt{-g(y)}T^{\mu\nu}(y)\right)
+\Gamma^{\nu}_{\mu\lambda}(y) T^{\mu\lambda}(y) \cr
&~~~~~~=~\frac{m}{\sqrt{-g(y)}} \int \!\mathrm{d}\tau ~\dot{x}^{\nu}\dot{x}^{\mu}\partial^{(y)}_{\mu}\delta^4(y\!-\!x(\tau )) ~+~\Gamma^{\nu}_{\mu\lambda}(y) T^{\mu\lambda}(y) \cr
&~~~~~~=~\underbrace{-\frac{m}{\sqrt{-g(y)}} \int \!\mathrm{d}\tau ~\dot{x}^{\nu} \frac{d}{d\tau}\delta^4(y\!-\!x(\tau ))}_\text{this term we integrating by parts}
~+~\Gamma^{\nu}_{\mu\lambda}(y) T^{\mu\lambda}(y) \cr
&\stackrel{\text{int. by parts}}{=}~\frac{m}{\sqrt{-g(y)}}\underbrace{ \dot{x}^{\nu}\delta^{(4)}(y−x(τ))}_\text{shoul be =0! Why?} + \cr
&~~~~~\frac{m}{\sqrt{-g(y)}} \int \!\mathrm{d}\tau\underbrace{\left[\ddot{x}^{\nu}+ \Gamma^{\nu}_{\mu\lambda}(x(\tau))\dot{x}^{\mu}\dot{x}^{\lambda} \right]}_\text{=0 geodesics equation}\delta^4(y\!-\!x(\tau )) .
\end{align}Can anyone explain where did the term ##uv=\dot{x}^{\nu}\delta^{(4)}(y−x(τ))## go after integration by parts ##\int udv=uv−\int vdu## in the last term (5)?
 
Last edited:
Physics news on Phys.org
  • #2
Well, you can think that when evaluating the limits of the integral ##\delta^{(4)}(y-x(\tau))## will become 0 because it's basically 0 everywhere. For more rigorous ways you should study generalized functions and it's derivatives. You can look at the Gel'Fand and Shilov book "Generalized Functions Volume I".
 
  • #3
Gaussian97 said:
Well, you can think that when evaluating the limits of the integral ##\delta^{(4)}(y-x(\tau))## will become 0 because it's basically 0 everywhere. For more rigorous ways you should study generalized functions and it's derivatives. You can look at the Gel'Fand and Shilov book "Generalized Functions Volume I".
Can you write appropriate formulae from Gel'Fand and Shilov book's here?
 
  • #4
Well, is not a formula, is an entire book dedicated to generalized functions, but maybe you need the equation of Example 7 of Chapter 2:

$$\int \delta'(x-h)\varphi(x)\text{d}x=-\varphi'(h)$$
 
  • Like
Likes sergiokapone
  • #5
Yes, this formula explain the transition from (4) to (6), but why then mentioned integration by parts?
 
  • #6
Maybe because the author knows that the lector may not be familiarized with derivatives of generalized functions and then uses the argument I said before of "integrating by parts and supposing that ##\delta## outside an integral is 0."
 
  • #7
Gaussian97 said:
Well, you can think that when evaluating the limits of the integral δ(4)(y−x(τ))δ(4)(y−x(τ))\delta^{(4)}(y-x(\tau)) will become 0 because it's basically 0 everywhere.

Gaussian97 said:
"integrating by parts and supposing that δδ\delta outside an integral is 0."

Then I conclude,
##\dot{x}\delta (x) = 0## everywrehe, even in ##x=0##. Does it right?
 
  • #8
Well, you have to be very careful because ##\delta## is not a usual function, but most of the times you can think of it as a function that is 0 everywhere and is not defined at ##x=0##. Usually having a ##\delta## outside an integral is not a good idea.
 
  • Like
Likes sergiokapone

1. What is the significance of deriving geodesic equations from the electromagnetic tensor of a point particle?

The electromagnetic tensor is a mathematical representation of the electromagnetic field, which is a fundamental force in nature. By deriving geodesic equations from this tensor, we can better understand the behavior of particles in the presence of electromagnetic fields, which is crucial in fields such as astrophysics and particle physics.

2. How are geodesic equations related to the curvature of spacetime?

Geodesic equations describe the paths that particles follow in curved spacetime. These paths are known as geodesics, and they are influenced by the curvature of spacetime caused by the presence of massive objects. Therefore, by deriving geodesic equations from the electromagnetic tensor, we can understand how electromagnetic fields affect the curvature of spacetime.

3. Can geodesic equations be used to predict the motion of particles in the presence of electromagnetic fields?

Yes, geodesic equations can be used to predict the motion of particles in the presence of electromagnetic fields. These equations take into account the electromagnetic force acting on the particle and the curvature of spacetime, allowing us to accurately predict the trajectory of the particle.

4. Are there any limitations to using geodesic equations derived from the electromagnetic tensor?

One limitation is that these equations only apply to point particles, which are objects with no size or shape. They do not take into account the effects of the particle's size or shape on its motion in an electromagnetic field. Additionally, these equations are based on classical mechanics and do not account for quantum effects.

5. How do geodesic equations derived from the electromagnetic tensor compare to other methods of predicting particle motion?

Geodesic equations are a more general and fundamental way of predicting particle motion compared to other methods, such as Newton's laws of motion. This is because geodesic equations take into account both the curvature of spacetime and the electromagnetic force, while other methods may only consider one of these factors. However, in certain situations, such as in the absence of strong gravitational fields, other methods may provide more accurate predictions.

Similar threads

Replies
22
Views
3K
Replies
1
Views
1K
  • Special and General Relativity
Replies
2
Views
1K
  • Special and General Relativity
Replies
4
Views
597
  • Special and General Relativity
Replies
4
Views
1K
  • Special and General Relativity
Replies
2
Views
575
  • Special and General Relativity
Replies
7
Views
1K
  • Special and General Relativity
Replies
2
Views
929
  • Special and General Relativity
Replies
4
Views
3K
  • Special and General Relativity
Replies
1
Views
584
Back
Top