Once you fall into the event horizon of a black hole, you will never leave. There is no speed that you could gain, even the speed of light to allow you to enter. But in General relativity space is curved in the presence of mass and energy, and black holes — one of the most extreme scenarios of this curvature. Is there any way to get into the black hole, cross the event horizon and then leave it when the event horizon will be curved under the action of a massive merger?
When merging two black holes is matter within the event horizon of one black hole, to escape? Can they take and migrate to another (more massive black hole)? How about going beyond both horizons?
This idea is certainly insane. But is it sufficiently crazy to actually work? To answer this question, we will help physicist Ethan Siegel.
When a massive star ceases to exist, or when two sufficiently massive stellar remnant merge, can form a black hole with the event horizon, proportional to its mass, and disk accretion, in which twisted surrounding the black hole matter
A black hole is usually formed in the collapse of the core of a massive star or after a supernova explosion of a star or the merger of neutron stars or direct collapse. As far as we know, each black hole is formed from matter that was part of the star, so in many respects, black holes are the final remains of stars. Some black holes are formed in isolation; others are part of a binary system. Over time black holes can not only curl in a spiral and merge, but to absorb another substance that falls into the event horizon.
In the Schwarzschild black hole fall inside leads to the singularity and the dark. Regardless of which direction you are traveling, as faster and so on, crossing the event horizon is the inevitable collision with the singularity
When something crosses the event horizon of a black hole from the outside, it is doomed. Within seconds the object reaches the singularity at the center of the black hole: the point for non-rotating black holes and rings for rotary. The black hole itself does not remember which particles fell into it or what is their quantum state. Instead, all that remains, from the point of view of information is the total mass, charge and angular momentum of the black hole.
In the last pre-merge, the space-time surrounding a black hole, will be broken, because the matter will continue to drop in both black holes from the environment. In any case, do not assume that something will be able to escape from inside the event horizon
Thus, it is possible to imagine a scenario in which material falls onto the black hole during the final stages of a merger when one black hole that’s connected on the other. Because black holes must always have accretion disks and the interstellar medium is constantly flying matter, the event horizon will be constantly crossing particles. It’s simple, so let’s look at a particle that fell into the event horizon before the final moments of the merger.
Could it theoretically run? Can “jump” from one black hole to another? Let us consider the situation from the point of view of space-time.
Computer simulation of two merging black holes and the curvature of space-time, caused by them. Although gravitational waves are emitted continuously, the substance can’t escape
When two black holes merge, they do it after a long period of twist of the spiral, in which the energy is radiated in form of gravitational waves. Up to the final moments before the merger of the energy is emitted and flies away. But it can’t cause the event horizon or even a black hole shrink; instead, the energy comes from space-time in the center of mass, which is deformed stronger and stronger. With such success it would be possible to steal energy from the planet mercury; it would rotate closer to the Sun, but its properties (or properties of the Sun) does not change.
However, when in the last moments of the merge event horizons of two black holes are deformed by the gravitational presence of each other. Fortunately, numerical relativists have already calculated how the merger affects the event horizon, and it’s impressively informative.
Despite the fact that up to 5% of the total mass of black holes before the merger can be radiated in form of gravitational waves, the event horizon never decreases. It is important that if you take two black holes of equal mass, their event horizons will occupy a certain volume of space. If you combine them with the creation of a black hole double weight, the amount of space occupied by the horizon, will be four times the original volume of the combined black holes. The mass of black holes is proportional to their radius, but the volume is proportional the cube of radius.
Although we have found many black holes, the radius of each of the event horizon is directly proportional to the mass of the hole, always. Double the mass, double radius, but the area will increase four times, and the volume — in eight
It turns out that even if you will keep the maximum particle in a stationary state inside a black hole and it will be possible to slowly fall towards the singularity, there was no way out. The total volume of the combined event horizon during the merger of black holes increases, and regardless of what the trajectory of a particle crossing the event horizon, it is doomed to be swallowed by the singularity of the joint of the two black holes.
In many scenarios, astrophysicists appear to emission when matter escapes from the object during the cataclysm. But in the case of merging black holes, everything inside, stays inside, the outside, is drawn, and only a few of the outside, can escape. Falling into a black hole, you are doomed. And another black hole will not change the balance of power.
Is matter leave the event horizon during the merger of black holes?
Ilya Hel