Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection

DOI10.1142/S0218271820500571zbMath1443.83028arXiv1808.05015MaRDI QIDQ5125332

Sandro M. R. Micheletti

Publication date: 6 October 2020

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

Full work available at URL: https://arxiv.org/abs/1808.05015

zbMATH Keywords

interacting dark energy modelsstatistical model selectioncosmological parameters from observational datafield theory in curved spacetime

Mathematics Subject Classification ID

Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47) Observational and experimental questions in relativity and gravitational theory (83B05) Dark matter and dark energy (83C56)

Related Items (1)

Deriving the dark matter-dark energy interaction term in the continuity equation from the Boltzmann equation

Uses Software

• ElemStatLearn

Cites Work

• Unnamed Item
• Exact solutions for the interacting tachyonic-dark matter system
• Estimating the dimension of a model
• Tachyons in string theory
• Dark Energy
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• SPACE–TIME IN LIGHT OF KÁROLYHÁZY UNCERTAINTY RELATION
• Model Selection and Multimodel Inference
• A new look at the statistical model identification

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