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Extending the scope of models for large-scale structure formation in the Universe

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arxiv astro-ph/9709218 v2 pith:ORXF4VDZ submitted 1997-09-23 astro-ph

classification astro-ph
keywords modelformationlarge-scalemodelsnoisepressurestructureuniverse
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We propose a phenomenological generalization of the models of large-scale structure formation in the Universe by gravitational instability in two ways: we include pressure forces to model multi-streaming, and noise to model fluctuations due to neglected short-scale physical processes. We show that pressure gives rise to a viscous-like force of the same character as that one introduced in the ``adhesion model'', while noise leads to a roughening of the density field yielding a scaling behavior of its correlations.

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  1. Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions

    astro-ph.CO 2025-02 conditional novelty 5.0 of 10

    An ensemble-averaged stochastic cosmology with a 'little ado' noise term produces an emergent dark energy that fits late-time data and claims to relieve the H0 and f sigma8 tensions.

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