Effect of the chameleon scalar field on brane cosmological evolution

DOI10.1016/J.PHYSLETB.2017.10.035zbMath1403.83047arXiv1710.07949OpenAlexW2766680166MaRDI QIDQ1631891

Y. Aharonov

Publication date: 7 December 2018

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

Full work available at URL: https://arxiv.org/abs/1710.07949

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Kaluza-Klein and other higher-dimensional theories (83E15)

Related Items (1)

Deflation of vacuum energy during inflation due to Bulk-Brane interaction

Cites Work

• The hierarchy problem and new dimensions at a millimeter
• The fundamental constants and their variation: observational and theoretical status
• Large Mass Hierarchy from a Small Extra Dimension
• An Alternative to Compactification
• Thermodynamics and cosmology

This page was built for publication: Effect of the chameleon scalar field on brane cosmological evolution