A note on gravitational baryogenesis within Bianchi type I universe

DOI10.1007/S10509-013-1355-ZzbMath1276.83057OpenAlexW2078592044WikidataQ125124939 ScholiaQ125124939MaRDI QIDQ383448

V. Fayaz, Hossien Hossienkhani

Publication date: 4 December 2013

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-013-1355-z

zbMATH Keywords

gravitational interactionanisotropic universebaryogenesisbaryon asymmetry

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

Related Items (3)

Interacting generalized ghost dark energy in non-isotropic background ⋮ Anisotropy effects on baryogenesis in f(R) theories of gravity ⋮ Instability of interacting ghost dark energy model in an anisotropic universe

Cites Work

• Dark energy models with variable equation of state parameter
• Bianchi type III anisotropic dark energy models with constant deceleration parameter
• SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY

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