Effects of acceleration on black holes.

In summary, if a black hole was sailing across the universe very near to the speed of light, the relativistic effects would cause the event horizon to change shape and the black hole would live longer due to its velocity. If you were traveling at around half-C toward the oncoming black hole, you could not escape it.
  • #1
Lord Flasheart
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If a black hole was sailing across the universe very near to the speed of light, what would the effects be on it? Would the event horizon change in shape, becoming more bulbous or less so in front of it, and would it live longer due to its relativistic velocity? And if you were traveling at around half-C toward the oncoming black hole, could you escape it? If you couldn't, would you be traveling faster than light for a brief few nano-seconds?
 
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  • #2
Originally posted by Lord Flasheart
If a black hole was sailing across the universe very near to the speed of light, what would the effects be on it? Would the event horizon change in shape, becoming more bulbous or less so in front of it, and would it live longer due to its relativistic velocity? And if you were traveling at around half-C toward the oncoming black hole, could you escape it? If you couldn't, would you be traveling faster than light for a brief few nano-seconds?
You're describing relative effects, so I guess
it's a matter of who's looking. :wink:
The event horizon would indeed change shape
if for you the speed is relativistic.

Live long and prosper.
 
  • #3
Two galaxies, each with a supermassive black hole at its centre, collide.

What will happen?

If the black holes undergo a dance of death, how fast will they be moving, relative to each other (and also a star 100 light years away, at rest relative to the centre of mass of the black holes) when they are 1 light year apart? 1 light day? 1 light hour??

Assume the black holes each have a mass of 10 million Suns (107sol).

Using reasonable assumptions about the universe, how many such supermassive black hole mergers will be 'visible' to us on Earth each year (in the sense that we could detect the 'light' from such a merger from as far away as 10 billion light years)?
 

What is acceleration and how does it affect black holes?

Acceleration is a change in velocity over time, and it can greatly affect black holes. As an object falls into a black hole, it experiences increasing acceleration due to the strong gravitational force. The closer an object gets to the black hole, the faster it falls, eventually reaching the speed of light at the event horizon.

How does acceleration impact the size of a black hole?

The size of a black hole is directly related to its mass, and acceleration can affect the mass of a black hole. As matter falls into a black hole, its mass increases, causing the black hole to grow in size. The rate of acceleration can also impact the size of a black hole, as faster acceleration means more matter can enter the black hole in a shorter amount of time.

What happens to light when it enters a black hole at high acceleration?

As an object approaches the event horizon of a black hole, it experiences extreme acceleration. This acceleration causes the light to stretch and shift towards the red end of the spectrum, making it appear to take longer to reach an observer. At the event horizon, the light is so redshifted that it becomes infinitely redshifted, meaning it never reaches an observer outside the black hole.

Can acceleration prevent a black hole from forming?

Acceleration is necessary for the formation of a black hole. When a massive star runs out of fuel, it can no longer produce enough energy to counteract the force of gravity. This causes the star to collapse, and as it does, it experiences rapid acceleration, eventually forming a black hole.

How do scientists measure the effects of acceleration on black holes?

Scientists use a variety of tools and techniques to study the effects of acceleration on black holes. These include observing the motion of objects around black holes, measuring the redshift of light from objects near black holes, and using computer simulations to model the behavior of matter falling into a black hole at different rates of acceleration.

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