![1 (2) (1).png](https://cdn.steemitimages.com/DQmaZybirxiNAC22DRi9DMtk8yYXmU8Hw5WUCmRbuz3vCRr/1%20(2)%20(1).png) Some cosmic travelers speculate that after this Universe, a new Universe may arise. One of the most popular assumptions is the idea of infinite Universes, which suggests that our Universe is one of the many Universes that constantly appear and disappear in an infinite cycle. This theory is supported by some physicists who have proposed a scientific model that suggests our Universe will collapse and then a new Universe will arise. Some researchers also suggest that each Universe has its own unique properties, such as size and composition, which may differ from each other, and that such differences may explain some of the phenomena we observe, such as contradictory science. Although this theory has attracted much attention, it has yet to be confirmed. The multiverse also suggests that many of our own solutions may work in other universes. Thus, we can apply the laws of our universe when we explore others. With the multiverse, we can also study other types of universes, including those that are not understandable in our own universe. This allows us to understand more about our own universe and also helps us to understand how it interacts with other universes. ![1 (1) (1).png](https://cdn.steemitimages.com/DQmTJs36BqixTNXCKPunv4nHMtaunCrApBDDZYQoL6UQ9wj/1%20(1)%20(1).png)

How does the interaction between universes take place?

Universes cannot interact directly since they are located far enough from each other. However, interaction between universes can happen on the level of matter and energy. For example, one universe may affect another by emitting radiation such as gamma rays or cosmic rays. These radiations can have a significant effect on the universe they enter and may even cause changes in the structure of space-time.

The Theory of the Big Bang

is the idea that the Universe randomly emerged from a very small and very hot state in a very short period of time. This led to the creation of all kinds of matter, antimatter, and the entire structure seen in our Universe. This idea was proposed in 1929 by astrophysicist George Gamow ^{[1](https://en.wikipedia.org/wiki/George_Gamow)}. It was further improved and developed by astrophysicists Albert Einstein^{[2](https://en.wikipedia.org/wiki/Albert_Einstein)} and Stephen Hawking^{[3](https://en.wikipedia.org/wiki/Stephen_Hawking)}.

What changes have occurred to the multiverse after the Big Bang?

After the Big Bang, the multiverse underwent huge changes. Universes that were connected before the Big Bang were separated and scattered throughout the universe. This led to the expansion of the universe, and all things in it stretched out and grew. A new element also began to be used - antimatter, which was divided into two different types - antimatter and anti-energy. These two types of antimatter play an important role in the expansion of the universe and its structure.

How to get into a multiverse?

At this point there is no access to a multiverse. This concept can only take place in fantasy stories and dystopias. Some people may attempt to create their own multiverse using scientific methods such as data analysis and artificial intelligence. But this is not possible yet.

Is it possible to die in a multiverse?

No, as multiverses are conceptual concepts that usually don't exist in the real world. There is no real death in a multiverse, and nobody can die in this universe. Multiverse ideas may be linked to mental projects and games, but not to real universes and objects.

How far can our research into the multiverse reach?

At the moment, we cannot reach the multiverse. The research we have presented can lead us to an understanding of the nature and dynamics of our Universe, but not beyond its boundaries. Astronomers are working on understanding how different multiverses can interact with each other, but there are no concrete data yet. Our research can help us get closer to understanding the nature and dynamics of the multiverse, but there is still a long way to go.