Dark energy on higher dimensional spherically symmetric Brans-Dicke universe

DOI10.1016/j.cjph.2019.05.003OpenAlexW2945785553WikidataQ127795174 ScholiaQ127795174MaRDI QIDQ6201257

Kangujam Priyokumar Singh, Pheiroijam Suranjoy Singh

Publication date: 25 March 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cjph.2019.05.003

zbMATH Keywords

spherically symmetricholographic dark energyBrans-Dickefive dimensional space time

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15) General relativity (83Cxx)

Cites Work

• \(f(R)\) theories
• Statefinder parameters for interacting dark energy
• Holographic dark energy
• Bulk viscous cosmological model in Brans-Dicke theory with new form of time varying deceleration parameter
• An interacting scalar field and the recent cosmic acceleration
• Über einen verallgemeinerten affinen Zusammenhang
• A quintessence scalar field in Brans-Dicke theory
• The cosmological constant and dark energy
• Mach's Principle and a Relativistic Theory of Gravitation
• DYNAMICS OF DARK ENERGY
• THE COSMOLOGICAL DYNAMICS OF INTERACTING HOLOGRAPHIC DARK ENERGY MODEL
• Brans–Dicke cosmology mimicking running vacuum
• Two-loop scalar self-mass during inflation
• Large–scale structure and matter in the Universe
• SELF-INTERACTING HOLOGRAPHIC DARK ENERGY
• Mimetic F(R) gravity: Inflation, dark energy and bounce
• The cosmological constant
• Interacting quintessence

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