Calculating luminosity distance versus redshift in FLRW cosmology via homotopy perturbation method

DOI10.1134/S0202289317020098zbMath1380.85021arXiv1511.07459MaRDI QIDQ681418

V. K. Shchigolev

Publication date: 12 February 2018

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1511.07459

zbMATH Keywords

redshiftFriedmann-Lemaître-Robertson-Walker (FLRW)homotopy perturbation method (HPM)FLRW cosmologycalculating luminosity distance

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (2)

A new model for strange stars ⋮ Studying gravitational deflection of light by Kiselev black hole via homotopy perturbation method

Cites Work

• Homotopy-perturbation method for pure nonlinear differential equation
• A coupling method of a homotopy technique and a perturbation technique for nonlinear problems
• Homotopy perturbation technique
• Cosmography: Cosmology without the Einstein equations
• Jerk, snap and the cosmological equation of state
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The Hubble series: convergence properties and redshift variables

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