A model of interacting dark fluids tested with supernovae and Baryon Acoustic Oscillations data

DOI10.1016/J.NUCLPHYSB.2019.01.001zbMath1414.83103arXiv1702.03185OpenAlexW2908863304WikidataQ128628073 ScholiaQ128628073MaRDI QIDQ1731679

She-Sheng Xue, Clément Stahl, Damien Bégué

Publication date: 13 March 2019

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1702.03185

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (3)

Interacting tachyonic scalar field ⋮ Constraining the spectrum of cosmological perturbations from statistical thermal fluctuations ⋮ Dynamics of chiral cosmology

Cites Work

• How universe evolves with cosmological and gravitational constants
• Dark energy from structure: a status report
• Quintessence: a review
• Inhomogeneous cosmological models: exact solutions and their applications
• Cosmic perturbations with running G and Λ

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