Stephen Hawking and his colleagues made an assumption that information is not locked within a black hole, but rather is stored on its visible boundary – the event horizon. They seek to explain the way how information about the matter is preserved when the particle dives into the depth before the black hole evaporates and disappears. The less active quantum particles – the soft hair, enclose the black hole at the event horizon and, upon interaction with light rays, preserve traces of the information which has penetrated it.

The spherical event horizon is full of quantum particle-antiparticle pairs, which continuously merge and split apart, appear and disappear. Standing next to the black hole, one half of the pair may fall into it leaving the other half without its partner. The other may decide to follow its partner or choose another scenario and become radiation of the black hole.

In context of the exhibition, the topic acts like a push.

Inside, outside, and the event horizon in-between. The boundary is the space between. The interspace is considered a potential-bearing opportunity; standing there, the process runs in multiple directions. One can meet an interspace by touching it.

Each object or event has a clear boundary to distinguish it from all the rest. Either blurry, or sharp. The field of vision draws the boundaries of the selected area – the visible stays inside, while the rest is left outside. Even in the case of uncertainty we tend to create it. It may be in the form of a wall, an abstract line or a field. Each object turns into substance or a container of meanings.

The exhibition addresses optional ambiguity solutions by means of multiple spatial approaches, along with the communication difficulties in terms of information transfer between quanta and other bodies.