How Long Does It Take to Fall into a 5-D Black Hole?

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Homework Help Overview

The discussion centers around a problem involving the 5-dimensional generalization of the Schwarzschild solution in general relativity. The original poster seeks to determine the elapsed time on an observer's clock as they fall into a 5-D black hole, starting from a specific radial distance.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to use Lemaitre coordinates to eliminate singularities in the metric and integrate to find the time of fall. Some participants question the correctness of the integration step and the definitions used for the Lemaitre coordinates. Others suggest that the integration could be approached using the Schwarzschild coordinates instead.

Discussion Status

Participants are actively engaging with the mathematical expressions and definitions presented. There is a recognition of potential errors in the original poster's approach, and some guidance is offered regarding the use of standard texts for deriving expressions related to free-fall trajectories. The discussion reflects a mix of interpretations and suggestions without reaching a consensus.

Contextual Notes

There are indications of confusion regarding the definitions and expressions for Lemaitre coordinates in the context of a 5-D metric. Participants note the need to clarify assumptions about the initial conditions of the observer's fall and the implications of using different coordinate systems.

Confused Physicist
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Hi, I have the following problem:

Given the 5-D generalization of the Schwarszschild solution with line element:

ds^2=-\Bigg(1-\frac{r^2_+}{r^2}\Bigg)dt^2+\Bigg(1-\frac{r^2_+}{r^2}\Bigg)^{-1}dr^2+r^2[d\chi^2+\sin^2(\chi)(d\theta^2+\sin^2(\theta)d\phi^2)]

where ##r_+## is a positive constant. An observer falls radially starting from rest at ##r=10r_+##. How much time elapses on their clock before they hit the singularity at ##r=0##?

MY ATTEMPT HAS BEEN:

Using the Lemaitre coordinates ##\tau##, ##\rho## to eliminate the singularity of ##ds^2## at ##r_+##:

d\tau=dt+\frac{r_+}{r}\frac{dr}{1-\frac{r^2_+}{r^2}}

d\rho=dt+\frac{r}{r_+}\frac{dr}{1-\frac{r_+^2}{r^2}}\quad\quad\quad (1)

we have the following line element where the singularity at ##r_+## is removed:

ds^2=d\tau^2-\frac{r_+}{r}d\rho^2-r^2(d\theta^2+\sin^2(\theta)d\phi^2)

where ##r=\sqrt{2(\rho-\tau)r_+}##, which is obtained by integrating d\rho-d\tau=\frac{r}{r_+}dr.

For a free falling body, ##d\rho=0##, and equation (1) gives:

dt=-\frac{r}{r_+}\frac{1}{1-\frac{r_+}{r}}dr

Integrating this equation from ##r=10r_+## to ##r=0## should give me the time the problem asks for:

\Delta\tau=-\int_{10r_+}^0 \frac{r}{r_+}\frac{1}{1-\frac{r_+}{r}}dr

Is this correct?

Thanks!
 
Last edited:
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I have the feeling the last step, where I integrate ##dt## and get the time the observer takes to fall into the black hole, is not quite correct. But I'm not really sure. Could someone help me out? Thanks, I really appreciate it.
 
Confused Physicist said:
Using the Lemaitre coordinates ##\tau##, ##\rho## to eliminate the singularity of ##ds^2## at ##r_+##:

d\tau=dt+\frac{r_+}{r}\frac{dr}{1-\frac{r^2_+}{r^2}}

d\rho=dt+\frac{r}{r_+}\frac{dr}{1-\frac{r_+^2}{r^2}}\quad\quad\quad (1)
Your expressions here don't appear to correspond to the usual definition of Lemaitre coordinates. You are missing some square roots. Also, should the ##r##'s be squared in the denominators? See https://en.wikipedia.org/wiki/Lemaître_coordinates

[EDIT: Sorry. I overlooked the fact that the ##r##'s are squared in the 5-D version of the metric. I'm not familiar with this. So, your expressions for the Lemaitre coordinates are probably OK.
However, I think there is a typo in your equation

ds^2=d\tau^2-\frac{r_+}{r}d\rho^2-r^2(d\theta^2+\sin^2(\theta)d\phi^2)
Shouldn't the coefficient of ##d\rho^2## on the right be ##\left(\frac{r_+}{r}\right)^2## instead of ##\frac{r_+}{r}##? You have changed the overall sign of ##ds^2## when going from the Schwarzschild coordinates to the Lemaitre coordinates. Also, here your angular part is for 4D rather than 5D.​
For a free falling body, ##d\rho=0##,
##d\rho=0## only holds for radial free-fall if the initial condition corresponds to starting at rest at infinity. For a particle that starts at rest at a finite value of ##r##, ##d\rho \neq 0##.

You can solve the problem sticking with the Schwarzschild coordinates. In standard texts, it is shown how to derive an expression for ##\frac{dt}{d \tau}## in terms of ##r## for any free-fall trajectory. Here, ##\tau## is proper time for the freely falling particle. See the first equation here: http://grwiki.physics.ncsu.edu/wiki/Schwarzschild_Black_Hole#Geodesic_Motion
I think this equation should still be valid in the 5-D spacetime of your problem.

[EDIT: The equation for ##\frac{dt}{d \tau}## will probably change for 5-D. I will try to find the time to work it out. The derivation should be similar to the 4-D derivation.]​

You can use this equation along with the form of the metric to deduce an expression for ##\frac{dr}{d \tau}## as a function of ##r## for radial motion.
 
Last edited:
The 5-D case does appear to work out just as easily as the 4-D case. You should find that the expression for ##\frac{dt}{d\tau}## in the 5D case differs from the 4D case by just replacing ##\frac{r_+}{r}## in the 4D case by ##\left(\frac{r_+}{r}\right)^2##. Then, working out an expression for ##\frac{dr}{d\tau}## from the 5D metric is very similar to working it out in the 4D case. The final integration to obtain the total infall time ##\tau## is actually easier in the 5D case (if I didn't make any mistakes).
 

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