Studying the optical depth behavior of parametrized deceleration parameter in non-flat universe

DOI10.1142/S0219887823501104OpenAlexW4313551923MaRDI QIDQ6181062

Unnamed Author, Anirudh Pradhan, Ujjal Debnath

Publication date: 22 January 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887823501104

zbMATH Keywords

gravitational lensingdark energydeceleration parameteroptical depth

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Observational Constraining Study of New Deceleration Parameters in FRW Universe

Cites Work

• Accretion of some classes of holographic DE onto higher-dimensional Schwarzschild black holes
• On the theory and applications of modern cosmography
• A divergence-free parametrization of deceleration parameter for scalar field dark energy
• DYNAMICS OF DARK ENERGY
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• GENERALIZED HOLOGRAPHIC DARK ENERGY AND ITS OBSERVATIONAL CONSTRAINTS
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Model-independent analysis of dark energy: supernova fitting result

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