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arXiv · 1302.1748

A natural cosmological constant from chameleons

Horatiu Nastase·Amanda Weltman
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Abstract

We present a simple model where the effective cosmological constant appears from chameleon scalar fields. For a Kachru-Kallosh-Linde-Trivedi (KKLT)-inspired form of the potential and a particular chameleon coupling to the local density, patches of approximately constant scalar field potential cluster around regions of matter with density above a certain value, generating the effect of a cosmological constant on large scales. This construction addresses both the cosmological constant problem (why $Λ$ is so small, yet nonzero) and the coincidence problem (why $Λ$ is comparable to the matter density now).

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Horatiu Nastase, Amanda Weltman. 2015-04-06. A natural cosmological constant from chameleons. https://doi.org/10.1016/j.physletb.2015.05.066

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