From Landau two-fluid model to de Sitter Universe
G.E. Volovik

TL;DR
This paper explores the analogy between superfluid helium hydrodynamics and the de Sitter universe, proposing a multi-fluid model that links quantum vacuum, dark matter, and relativistic matter, offering insights into cosmological phenomena.
Contribution
It introduces a novel analogy between condensed matter two-fluid hydrodynamics and the de Sitter universe, connecting dark matter, quantum vacuum, and cosmological expansion.
Findings
De Sitter expansion resembles a multi-fluid system with three components.
The local temperature of the de Sitter horizon influences matter and gravitational components.
Energy exchange leads to decay and correct magnitude of dark matter and vacuum energy.
Abstract
The condensed matter analogs are useful for consideration of the phenomena related to the quantum vacuum. This is because in condensed matter we know physics both in the infrared and in the ultraviolet limits, while in particle physics and gravity the physics at trans-Planckian scale is unknown. One of the corner stones of the connections between the non-relativistic condensed matter and the modern relativistic theories is the two-fluid hydrodynamics of superfluid helium. The dynamics and thermodynamics of the de Sitter state of the expansion of the Universe bear some features of the multi-fluid system. There are actually three components: the quantum vacuum, the gravitational component and relativistic matter. The expanding de Sitter vacuum serves as the thermal bath with local temperature, which is twice the Gibbons-Hawking temperature related to the cosmological horizon. This local…
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Taxonomy
TopicsCosmology and Gravitation Theories · Astronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena
