Time Travel - Between two Kerr metric black holes w/detached event horizons

In summary: Therefore, in summary, the direction of the rotation of the black holes and the Earth would have an impact on your momentum if you were close enough, but would not affect your mass.
  • #1
Dan81
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So imagine your on Earth at a latitude of 30 to 45° N, between two rotating Kerr Metric Blackholes with detached event horizons (dual singularities) allowing you to be shielded from the crushing force of the black holes. Which way do the rotating black holes need to rotate for the past and which way do they need to rotate for the future? Does the Earth's rotation even matter? I don't care about the nay saying that I would be crushed and it wouldn't matter or spaghettified. Which rotational direction would they need to rotate for my mass (spaghettified, intact, or annihilated) to go in the future or past and is momentum required or can you be stationary?
 
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  • #2
The rotational direction of the black holes would not have any effect on your mass, since you would be too far away from them to be affected by their gravity. However, if you were close enough to the black holes, then the rotational direction of the black holes could affect your momentum, as any rotational force/acceleration would be exerted on you. In this case, the direction of the Earth's rotation would matter, as it would determine which way the rotational force/acceleration was exerted on your mass.
 

Related to Time Travel - Between two Kerr metric black holes w/detached event horizons

1. How is time travel possible between two Kerr metric black holes with detached event horizons?

According to the theory of general relativity, time travel is possible when there is a strong gravitational field, such as that of a black hole. In the case of two Kerr metric black holes with detached event horizons, the strong gravitational pull can create a "wormhole" or tunnel through space-time, allowing for the possibility of time travel.

2. What is a Kerr metric black hole?

A Kerr metric black hole is a type of rotating black hole, named after physicist Roy Kerr. It is described by a mathematical solution to Einstein's field equations in general relativity and is characterized by its mass and spin, which determine the shape of the black hole's event horizon.

3. What does it mean for an event horizon to be detached?

An event horizon is the point at which the gravitational pull of a black hole becomes so strong that not even light can escape from it. In the case of a detached event horizon, the gravity of one black hole is not strong enough to completely engulf the other black hole, creating a space between them where light and matter can pass through.

4. Can time travel between two Kerr metric black holes with detached event horizons be achieved?

While the theory of general relativity allows for the possibility of time travel between two Kerr metric black holes with detached event horizons, there is currently no evidence or technology to support the actual achievement of time travel in this manner. The concept remains theoretical and requires further study and understanding of the laws of physics.

5. What are the potential consequences of time travel between two Kerr metric black holes with detached event horizons?

The consequences of time travel between two Kerr metric black holes with detached event horizons are unknown and can only be speculated upon. It is possible that such a journey could result in paradoxes or alterations to the timeline, and could potentially have significant effects on the fabric of space-time. Further research and understanding of the concept is necessary to fully understand the potential consequences of time travel in this scenario.

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