Can brane cosmology with a vanishing explain the observations?

DOI10.1088/0264-9381/20/11/306zbMath1028.83035arXivastro-ph/0211285OpenAlexW3104248883WikidataQ126113720 ScholiaQ126113720MaRDI QIDQ4407002

Parampreet Singh, R. G. Vishwakarma

Publication date: 26 January 2004

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0211285

zbMATH Keywords

dark energybrane cosmologycosmic microwave backgroundwarped brane model

Mathematics Subject Classification ID

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

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Transition from decelerated to accelerated cosmic expansion in braneworld universes ⋮ Phantom appearance of non-phantom matter in anisotropic cosmological model ⋮ Phantom appearance of non-phantom matter in Bianchi type-I cosmological model ⋮ Chaplygin DGP cosmologies ⋮ ACCELERATION OF THE UNIVERSE DRIVEN BY THE CASIMIR FORCE ⋮ Constraining bouncing cosmology caused by the Casimir effect ⋮ GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS ⋮ Phantom appearance of non-phantom matter ⋮ VACUUM POLARIZATION IN AN ANTI-DE SITTER SPACE AS AN ORIGIN FOR A COSMOLOGICAL CONSTANT IN A BRANE WORLD ⋮ DARK ENERGY FROM FIFTH-DIMENSIONAL BRANS–DICKE THEORY

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