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Higgs Dark Energy

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arxiv 1404.0532 v4 pith:XTJOF2L3 submitted 2014-04-02 astro-ph.CO gr-qchep-th

classification astro-ph.COgr-qchep-th
keywords theoryhiggsuniverseacceleratedaccountattractivebosonicclassical
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We study the classical dynamics of a non-abelian Higgs theory coupled to gravity in an isotropic and homogeneous Universe. For non-minimal coupling, this theory leads to a model of cosmic inflation that is very attractive due to its simplicity and consistency with the latest experimental data. We show that this theory can also explain the current accelerated expansion of the Universe, provided that all the gravitational and bosonic degrees of freedom, together with their symmetries, are correctly taken in account.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Black Holes and Higgs Dark Energy

    astro-ph.CO 2025-02 reject novelty 5.0 of 10

    The paper claims black holes can trap Higgs field energy as dark energy during stellar collapse, giving a 2:1 matter-to-dark-energy ratio and a 57 microsecond collapse time.

  2. Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution

    gr-qc 2017-05 accept novelty 2.0 of 10

    Modified gravity theories supply viable mathematical frameworks for inflation, bounces, and dark energy eras that match observational data.

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