The Collapse of the Event Horizon in the de Sitter Universe
Vitaly Kuyukov Petrovich
Abstract
Vitaly Kuyukov Petrovich
Abstract
In this article reviews the evolution of the future of the Universe with a cosmological constant. When restricting the event horizon of the Universe, there exists a nonzero temperature of the Hawking. This effect leads to the reduction of the cosmological event horizon after a stage of expansion of the Universe with constant density of dark energy. Time compression in this Universe is determined only cosmological constant.
A significance statement is not available in the OpenAlex record.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
In this article reviews the evolution of the future of the Universe with a cosmological constant. When restricting the event horizon of the Universe, there exists a nonzero temperature of the Hawking. This effect leads to the reduction of the cosmological event horizon after a stage of expansion of the Universe with constant density of dark energy. Time compression in this Universe is determined only cosmological constant.
Key concepts: De Sitter universe, Event horizon, Cosmological constant, Physics, Particle horizon, Metric expansion of space, Universe, Dark energy