πΈοΈ Cosmic Web
Watch the large-scale structure of the Universe emerge spontaneously. Tiny density fluctuations grow under gravity into the stunning web of filaments, voids, and galaxy clusters we observe today.
Gravitational Instability & the Cosmic Web
The large-scale structure of the Universe β filaments, walls, voids and clusters β grew entirely from gravitational amplification of tiny quantum fluctuations (~10β5 amplitude) imprinted during inflation.
This simulation solves Newton's direct-summation N-body problem with softened gravity:
a_i = GΒ·Ξ£_j m_jΒ·(r_jβr_i) / (|r_jβr_i|Β² + Ρ²)^(3/2),
where Ξ΅ prevents singularities when particles approach each other.
Periodic boundary conditions wrap particles at the box edges, mimicking
a representative volume of the Universe.
Initial conditions use a uniform grid plus small sine-wave density perturbations (Zel'dovich approximation) to seed the collapse. The density field (colour map) is computed by counting particles per grid cell β brighter regions host more mass. Over time, matter streams from voids into filaments and collapses into dense nodes.