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The Collapse of the Event Horizon in the de Sitter Universe

Vitaly Kuyukov Petrovich

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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.

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What this paper is about

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.

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Available 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.

Key concepts: De Sitter universe, Event horizon, Cosmological constant, Physics, Particle horizon, Metric expansion of space, Universe, Dark energy

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