How to test stringy dark energy?

DOI10.1016/S0370-2693(03)00055-8zbMath1008.83036arXivastro-ph/0209037OpenAlexW2044995062MaRDI QIDQ1855599

Paul H. Frampton

Publication date: 5 February 2003

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0209037

zbMATH Keywords

equation of statenegative pressurecosmological expansion

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30)

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Phantom Friedmann cosmologies and higher-order characteristics of expansion ⋮ PROBING DYNAMICS OF DARK ENERGY WITH SUPERNOVA, GALAXY CLUSTERING AND THE THREE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS ⋮ Redshift drift in varying speed of light cosmology ⋮ Phantom model for Tsallis holographic dark energy ⋮ Phantom cosmology with non-minimally coupled real scalar field ⋮ Constructing phantom with a nonminimally coupled complex scalar field ⋮ Determination of Cosmological Parameters from Cosmic Microwave Background Anisotropies

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