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The large-scale structure of the Universe

5 Pith papers cite this work. Polarity classification is still indexing.

5 Pith papers citing it
abstract

Research over the past 25 years has led to the view that the rich tapestry of present-day cosmic structure arose during the first instants of creation, where weak ripples were imposed on the otherwise uniform and rapidly expanding primordial soup. Over 14 billion years of evolution, these ripples have been amplified to enormous proportions by gravitational forces, producing ever-growing concentrations of dark matter in which ordinary gases cool, condense and fragment to make galaxies. This process can be faithfully mimicked in large computer simulations, and tested by a variety of observations that probe the history of the Universe starting from just 400,000 yr after the Big Bang.

years

2026 4 2025 1

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representative citing papers

Information Content of the Cosmic Web

astro-ph.CO · 2026-05-20 · unverdicted · novelty 4.0

The paper defines a continuous Shannon entropy from the tidal tensor eigenvalue sign patterns of the cosmic web and shows that its redshift evolution constrains the linear growth rate f(z) complementary to redshift-space distortions.

The Large-Scale Structure of the Universe through the SKA lenses

astro-ph.CO · 2026-06-30 · unverdicted · novelty 1.0

This review chapter summarizes the cosmic web's theoretical framework, recent radio observations of diffuse gas, and the expected impact of the SKA on detecting baryons in filaments and cluster outskirts.

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Showing 4 of 4 citing papers after filters.

  • Probing scalar-neutrino and scalar-dark-matter interactions with PandaX-4T hep-ex · 2025-11-17 · unverdicted · none · ref 2 · internal anchor

    PandaX-4T reports the first direct spectral search for scalar-mediated neutrino self-interactions in 136Xe double beta decay, setting new upper limits for mediator masses below 2 MeV/c².

  • Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations astro-ph.GA · 2026-06-08 · unverdicted · none · ref 77 · internal anchor

    PRFM-vol is a new subgrid star formation model for cosmological simulations that computes SFR from ambient densities via PRFM theory and a modified effective EOS, producing taller stellar scale heights, slightly higher stellar mass, and morphology changes including Toomre-driven clumps compared to p

  • Information Content of the Cosmic Web astro-ph.CO · 2026-05-20 · unverdicted · none · ref 2 · internal anchor

    The paper defines a continuous Shannon entropy from the tidal tensor eigenvalue sign patterns of the cosmic web and shows that its redshift evolution constrains the linear growth rate f(z) complementary to redshift-space distortions.

  • The Large-Scale Structure of the Universe through the SKA lenses astro-ph.CO · 2026-06-30 · unverdicted · none · ref 39 · internal anchor

    This review chapter summarizes the cosmic web's theoretical framework, recent radio observations of diffuse gas, and the expected impact of the SKA on detecting baryons in filaments and cluster outskirts.