2005Unpublished venueRequires access

Dark energy and de Sitter space

Cai Rong

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Abstract

Recent astronomical observations indicate that expansion of our universe is speeding up, rather than slowing down. To explain this accelerated expansion, the energy density of the universe has to include a dark energy component. In this article we discuss possible candidates for the dark energy. In particular, we emphasize the cosmological constant, cosmological constant problem, de Sitter space and various related fundamental problems.

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What this paper is about

Recent astronomical observations indicate that expansion of our universe is speeding up, rather than slowing down. To explain this accelerated expansion, the energy density of the universe has to include a dark energy component. In this article we discuss possible candidates for the dark energy. In particular, we emphasize the cosmological constant, cosmological constant problem, de Sitter space and various related fundamental problems.

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Available abstract

Recent astronomical observations indicate that expansion of our universe is speeding up, rather than slowing down. To explain this accelerated expansion, the energy density of the universe has to include a dark energy component. In this article we discuss possible candidates for the dark energy. In particular, we emphasize the cosmological constant, cosmological constant problem, de Sitter space and various related fundamental problems.

Key concepts: Dark energy, De Sitter universe, Physics, Cosmological constant, Metric expansion of space, Universe, De Sitter space, Lambda-CDM model

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