Bianchi type-II string cosmological model with magnetic field in \(f(R,T)\) gravity
DOI10.1007/s10773-014-2089-6zbMath1300.83056OpenAlexW2041903416MaRDI QIDQ458513
J. Herrera, D. Rodríguez-Gómez
Publication date: 8 October 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-014-2089-6
magnetic fieldBianchi type-II space-time\(f(R,T)\) gravitymassive stringconstant deceleration parameter
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Electromagnetic theory (general) (78A25)
Related Items (8)
Cites Work
- Bianchi type-II dark energy model in \(f(R,T)\) gravity
- Some Bianchi type cosmological models in \(f(R)\) gravity
- Some exact solutions of string cosmological models in Bianchi type-II space-time
- String cosmological models in Lyra geometry
- String cosmological models of Bianchi type-III
- Some exact solutions of string cosmological models in Bianchi type-V space-time
- Some spatially homogeneous string cosmological models
- The cosmological constant and dark energy
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- The gravitational field of plane symmetric thick domain walls
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
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