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Modeling transit dark energy in f(R,Lm)-gravity - MaRDI portal

Modeling transit dark energy in f(R,Lm)-gravity (Q6181054)

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scientific article; zbMATH DE number 7792319

Language	Label	Description	Also known as
English	Modeling transit dark energy in f(R,Lm)-gravity	scientific article; zbMATH DE number 7792319

Statements

scholarly article

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Modeling transit dark energy in f(R,Lm)-gravity (English)

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Anirudh Pradhan

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Dinesh Chandra Maurya

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Aroonkumar Beesham

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International Journal of Geometric Methods in Modern Physics

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publication date

22 January 2024

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full work available at URL

https://arxiv.org/abs/2209.14269

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zbMATH Keywords

flat FLRW universe

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modified \(f(R, L_m)\)-gravity

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dark energy

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observational constraints

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MaRDI profile type

MaRDI publication profile

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Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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Type Ia Supernova Discoveries at<i>z</i>> 1 from the<i>Hubble Space Telescope</i>: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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The cosmological constant problem

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DYNAMICS OF DARK ENERGY

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Cosmology with curvature-saturated gravitational Lagrangian \(R/\sqrt{1 + l^4 R^2}\)

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Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?

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Constraining \(f(R)\) gravity in solar system, cosmology and binary pulsar systems

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Cosmology in scalar-tensor gravity.

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Energy conditions in <i>f</i> ( <i>R</i> , <i> L <sub>m</sub> </i> ) gravity

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Cosmology in \(f(R, L_m)\) gravity

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LRS Bianchi type II perfect fluid cosmological models in normal gauge for Lyra's manifold

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LRS Bianchi type-I universe in Barber's second self creation theory

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A class of homogeneous cosmological models

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Extended gravity cosmography

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Cosmography: Cosmology without the Einstein equations

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On the theory and applications of modern cosmography

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Connecting early and late universe by f(R) gravity

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Dark energy from entanglement entropy

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Cosmographic study of the universe's specific heat: a landscape for cosmology?

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Cosmological degeneracy versus cosmography: A cosmographic dark energy model

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Evaluating backreaction with the ellipsoidal collapse model

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Self-accelerated universe induced by repulsive effects as an alternative to dark energy and modified gravities

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Evolution of vacuum bubbles embedded in inhomogeneous spacetimes

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Minimal cosmography

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Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

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Identifiers

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10.1142/s0219887823501050

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Mathematics Subject Classification ID

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zbMATH DE Number

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Sitelinks

Mathematics(1 entry)

mardi Publication:6181054

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