Reconstruction of quintessence field for the THDE with swampland correspondence in f(R,T) gravity

DOI10.1142/s0219887821500316arXiv2005.03979OpenAlexW3023715845WikidataQ124990831 ScholiaQ124990831MaRDI QIDQ6204319

Umesh Kumar Sharma

Publication date: 27 March 2024

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

Full work available at URL: https://arxiv.org/abs/2005.03979

zbMATH Keywords

quintessenceswampland\(f(R, T)\) gravityTHDE

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

Related Items

Diagnosing the Sharma-Mittal holographic dark energy model through the statefinder

Cites Work

• Unnamed Item
• Unnamed Item
• Implications, consequences and interpretations of generalized entropy in the cosmological setups
• Holographic tachyon model of dark energy
• Modified non-local-\(F(R)\) gravity as the key for the inflation and dark energy
• The quantum state of the universe from deformation quantization and classical-quantum correlation
• Holographic Chaplygin gas model
• Holographic tachyon model
• \( F (R)\) gravity with an axion-like particle: dynamics, gravity waves, late and early-time phenomenology
• On the geometry of the string landscape and the swampland
• Holographic dark energy in a non-flat universe with Granda-Oliveros cut-off
• Dark energy models through nonextensive Tsallis' statistics
• Do we live in the swampland?
• Implications of the generalized entropy formalisms on the Newtonian gravity and dynamics
• Possible generalization of Boltzmann-Gibbs statistics.
• Modified Friedmann equations from Tsallis entropy
• Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state
• Model independent analysis of supernova data, dark energy, trans-Planckian censorship and the swampland
• Quantum fine-tuning in stringy quintessence models
• Dark energy beyond quintessence: constraints from the swampland
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• Holographic dark energy
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• RECONSTRUCTING THE POTENTIALS FOR THE QUINTESSENCE AND TACHYON DARK ENERGY, FROM THE HOLOGRAPHIC PRINCIPLE
• DYNAMICS OF DARK ENERGY
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Dilaton Cosmology and Phenomenology
• Effective Field Theory, Black Holes, and the Cosmological Constant
• The world as a hologram
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• RECONSTRUCTION OF NEW HOLOGRAPHIC SCALAR FIELD MODELS OF DARK ENERGY IN BRANS–DICKE UNIVERSE
• The cosmological constant problem
• Runaway quintessence, out of the swampland
• An alternative to quintessence
• The Landscape, the Swampland and the Era of Precision Cosmology

This page was built for publication: Reconstruction of quintessence field for the THDE with swampland correspondence in f(R,T) gravity