Growth of linear perturbations in a universe with superfluid dark matter

DOI10.1088/1475-7516/2020/07/034zbMath1492.83026arXiv2001.02591OpenAlexW3104819746MaRDI QIDQ5070280

Shreya Banerjee, Sayantani Bera, David F. Mota

Publication date: 11 April 2022

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

Full work available at URL: https://arxiv.org/abs/2001.02591

zbMATH Keywords

power spectrumdark matter theoryrotation curves of galaxies

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Spectrum, resolvent (47A10) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Perturbations in context of PDEs (35B20) Orbital mechanics (70M20) Superfluids (classical aspects) (76A25) Dark matter and dark energy (83C56)

Cites Work

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• Varying constants, gravitation and cosmology
• A new type of isotropic cosmological models without singularity
• THE FAILURES OF THE STANDARD MODEL OF COSMOLOGY REQUIRE A NEW PARADIGM
• Chiral gravitational waves and baryon superfluid dark matter
• Unified superfluid dark sector

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