No-Go Theorem for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>k</mml:mi></mml:math>-Essence Dark Energy

DOI10.1103/PhysRevLett.97.081303zbMath1228.83119arXivastro-ph/0606584WikidataQ51931624 ScholiaQ51931624MaRDI QIDQ3107866

Ruth Durrer, Chiara Caprini, Camille Bonvin

Publication date: 26 December 2011

Published in: Physical Review Letters (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0606584

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items

k-evolution: a relativistic N-body code for clustering dark energy ⋮ Relativistic effects in the large-scale structure with effective dark energy fluids ⋮ UNIFIED DARK MATTER IN SCALAR FIELD COSMOLOGIES ⋮ Instabilities appearing in cosmological effective field theories: when and how? ⋮ The causal structure of QED in curved spacetime: analyticity and the refractive index ⋮ WORMHOLES OF K-ESSENCE IN ARBITRARY SPACE–TIME DIMENSIONS ⋮ Causality and the speed of sound ⋮ Gravitational collapse of K-essence matter in Painlevè-Gullstrand coordinates ⋮ RECENT STATUS OF DARK ENERGY ⋮ Dark Energy: Observational Status and Theoretical Models ⋮ Dark energy and dark gravity: theory overview ⋮ Interaction of neutrinos with a cosmological k-essence scalar ⋮ DARK ENERGY IN PRACTICE ⋮ Comparison of different approaches to the quasi-static approximation in Horndeski models

Cites Work

• Dynamics of k -essence
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• \(k\)-inflation
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