Observational constraints on the free parameters of an interacting Bose-Einstein gas as a dark-energy model

DOI10.1007/S10714-018-2473-2zbMath1409.83238arXiv1802.07232OpenAlexW2788599498WikidataQ128993143 ScholiaQ128993143MaRDI QIDQ1709986

Hiram E. Lucatero-Villaseñor, Germán Izquierdo, Jaime Besprosvany

Publication date: 15 January 2019

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1802.07232

zbMATH Keywords

interacting dark energyobservational constraintslikelihood regionslate acceleration of the Universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of statistics to physics (62P35) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (1)

Primordial gravitational waves spectrum in the interacting Bose-Einstein gas model

Uses Software

• GitHub
• april

Cites Work

• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• DYNAMICS OF DARK ENERGY
• Accelerated expansion of a universe containing a self-interacting Bose–Einstein gas
• Statistical Methods in Cosmology
• Coincidence problem within dark energy as a coupled self-interacting Bose–Einstein gas
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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