Viscous self interacting dark matter cosmology for small redshift

DOI10.1088/1475-7516/2019/02/045OpenAlexW2898129979WikidataQ128355410 ScholiaQ128355410MaRDI QIDQ5862075

Jitesh R. Bhatt, Abhishek Atreya, Arvind Kumar Mishra

Publication date: 4 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1810.11666

zbMATH Keywords

dark matter theorydark energy theorygalaxy clusterssupernova type Ia-standard candles

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (2)

Can the Hubble tension be resolved by bulk viscosity? ⋮ Gravitational wave luminosity distance in viscous cosmological models

Cites Work

• Viscous inflationary universe models
• Dark matter self-interactions and small scale structure
• Can neutrino viscosity drive the late time cosmic acceleration?
• Bulk viscosity driving the acceleration of the universe
• DYNAMICS OF DARK ENERGY
• THEORETICAL MODELS OF DARK ENERGY
• Analysing dissipative effects in the ΛCDM model
• Viscous cosmology for early- and late-time universe
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem

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