XCDM: a running vacuum strategy for crossing the phantom divide
Joan Solà Peracaula, Adrià Gómez-Valent, Alex González-Fuentes
astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-07-28
Comments: LaTeX, 19 pages, 2 Tables and 6 Figures, extended discussion
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Dark Energy Survey Year 6 Results: Cosmological Constraints from Cosmic Shear
- A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions
- $\Lambda_{\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions
- Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus
- Constraints on Coupled Dark Energy in the DESI Era
- The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
- GetDist: a Python package for analysing Monte Carlo samples
- Robust Preference for Dark Sector Interactions
- Hubble tension: the shape wall
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