Constraining interacting dark energy models with flux destabilization

DOI10.1016/j.physletb.2007.07.058zbMath1246.83259arXiv0707.2299OpenAlexW2056066785MaRDI QIDQ446766

Raul Horvat, Diego Pavón

Publication date: 8 September 2012

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0707.2299

zbMATH Keywords

flux destabilizationinteracting dark energy models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Other elementary particle theory in quantum theory (81V25)

Related Items (1)

Interacting holographic dark energy, future singularity and polytropic gas model of dark energy in closed FRW universe

Cites Work

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• Curvature phase transition in \(\mathbb{R}^ 2\) quantum gravity and induction of Einstein gravity
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point

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