Can Light Rays Cross Near a BH? - Simulated w/ Matlab

In summary: The two parallel light rays pass near a Kerr black hole with an angular momentum pointing towards the ##z## direction. The rays start at ##1\times 10^3~\rm{m}## and ##-1\times 10^3~\rm{m}## and end at ##-667~\rm{m}## and ##667~\rm{m}##, respectively, showing that they cross each other. The parameters of the black hole and initial conditions of the rays are given, and the final positions and wave vectors are calculated. The increase in wave number is attributed to a calculation error.
  • #1
Haorong Wu
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TL;DR Summary
When I simulate that two parallel light rays pass near a Kerr BH, the result shows that they cross each other. Is it possible?
Hi. I use Matlab to simulate that two parallel light rays pass near a Kerr BH. The angular momentum of the BH points to the ##z## direction. The ##z## components of the start points of the two rays are ## 1\times 10^3 ~\rm{m}## and ##- 1\times 10^3 ~\rm{m}##, respectively. The result, as shown in the figure, indicates that the rays cross each other. In the end, the ##z## components of the two rays are ##-667~\rm{m}## and ##667~\rm{m}##, respectively.

I am not sure if this is possible or not. Maybe there are some errors in my model. How can I check if my result is correct or not?

Thanks.
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  • #2
You haven't really explained your initial conditions, so it's hard to comment. I think your rays start symmetrically above and below the equatorial plane. What are their initial directions, and what are the mass and angular momentum parameters of the hole?
 
  • #3
@Ibix

Sorry, I thought that is not important, so I did not mention it. Here are the parameters (all are in Cartesian coordinates):

mass of BH is ##1.988\times10^{30}~\rm{kg}=1.47\times10^3~\rm{m}## ;
angular momentum per unit mass is ##0.9## (along z-axis);
position of BH is ##(0,~0,~0)##;
initial positions of rays are ##(-1\times 10^4,~2\times 10^4,~1\times 10^3)## and ##(-1\times 10^4,~2\times 10^4,~-1\times 10^3)##, respectively;
both initial wave vectors are ##(1.03\times 10^7 ,~1.82\times 10^6 , ~ 0)##;

The results are:
the final positions of rays are ##(9.12\times 10^4,~1.55\times 10^3,~-667)## and ##(9.12\times 10^4,~1.55\times 10^3,~667)##, respectively;
the final wave vectors are ##(1.05\times 10^7,~-2.28\times 10^6,~-1.90\times 10^5)## and ##(1.05\times 10^7,~-2.28\times 10^6,~1.90\times 10^5)##, respectively.

The wave number is increased by ##2.36\times10^5~\rm{m^{-1}}##, but I think that is due to the calculation error of the ode45 algorithm.
 
Last edited:
  • #4
This is gravitational lensing.
 
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FAQ: Can Light Rays Cross Near a BH? - Simulated w/ Matlab

What is the purpose of simulating light rays near a black hole using Matlab?

The purpose of simulating light rays near a black hole using Matlab is to visualize and analyze the behavior of light in the intense gravitational field of a black hole. This helps in understanding phenomena such as gravitational lensing, the bending of light, and the event horizon effects, which are critical for astrophysics and general relativity studies.

How does Matlab simulate the gravitational effects of a black hole on light rays?

Matlab simulates the gravitational effects of a black hole on light rays by solving the equations of motion derived from general relativity. These equations describe how light rays, or photons, travel through the curved spacetime around a black hole. Numerical methods and differential equations are typically used to model the trajectories of light rays as they are influenced by the black hole's gravity.

Can light rays actually cross paths or intersect near a black hole?

Yes, light rays can appear to cross paths or intersect near a black hole due to the extreme curvature of spacetime. This phenomenon is known as gravitational lensing, where the light from a background object is bent around the black hole, causing multiple images or apparent intersections of light paths when viewed from a distance.

What are the key parameters needed for simulating light rays near a black hole in Matlab?

The key parameters needed for simulating light rays near a black hole in Matlab include the mass of the black hole, the initial positions and velocities of the light rays, and the properties of the surrounding spacetime (e.g., Schwarzschild or Kerr metrics). Additionally, numerical settings such as the time step and integration method are crucial for accurate simulations.

What insights can be gained from studying the simulation results of light rays near a black hole?

Studying the simulation results of light rays near a black hole can provide insights into the nature of black holes, the structure of spacetime, and the effects of strong gravitational fields on light. It can also help in understanding observational phenomena such as the appearance of black holes, the formation of accretion disks, and the behavior of light from stars and other objects in the vicinity of a black hole.

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