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arxiv: 1411.3660 · v2 · pith:UBAU2ORNnew · submitted 2014-11-13 · 🌌 astro-ph.CO · gr-qc· hep-ph

Quintessence with Yukawa Interaction

classification 🌌 astro-ph.CO gr-qchep-ph
keywords modeldarkinteractinginteractionquintessenceyukawaappropriateconclude
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We consider a quintessence model for dark energy interacting with dark matter via a Yukawa interaction. To put constraints on this model we use the CMB measurements from the Planck satellite together with BAO, SNIa and $H_0$ data. We conclude that this is a viable model and an appropriate scalar potential can favor the interacting scenario.

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  1. Interacting Dark Sector field theory with phantom crossing

    astro-ph.CO 2026-05 unverdicted novelty 5.0

    An interacting dark sector model with Yukawa-coupled fermionic DM and Born-Infeld tachyonic scalar produces recent double phantom crossing in effective w_DE, fits DESI+Planck+SN data, and predicts ultralight DM mass o...