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Dark energy from non-degenerate Higgs-vacuum

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arxiv 2407.09840 v1 pith:QTWXHAXP submitted 2024-07-13 hep-ph gr-qc

classification hep-phgr-qc
keywords darkenergydoubletfieldshiggsmodelcandidatescomponent
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Scalar fields are favorite among the possible candidates for the dark energy. Most frequently discussed are those with degenerate minima at $\pm \phi_{min}$. In this paper, a slightly modified two-Higgs doublet model is taken to contain the Higgs field(s) as the dark energy candidate(s). The model considered has two non-degenerate minima at $\phi_{\pm}$, instead of one degenerate minimum at $\pm\phi_{min}$. The component fields of one SU(2) doublet ($\phi_1$) act as the standard model (SM) Higgs, while the component fields of the second doublet ($\phi_2$) are taken to be the dark energy candidates (lying in the true vacuum). It is found that one \emph{can} arrange for late time acceleration (dark energy) by using an SU(2) Higgs doublet, whose vacuum expectation value is zero, in the quintessential regime.

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Cited by 1 Pith paper

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.

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